Multiparticle production and initial quasi-temperature from proton induced carbon collisions at $p_{Lab}=31$ GeV/$c$

TL;DR

This study analyzes charged particle spectra from proton-carbon collisions at 31 GeV/c using a thermal model, revealing dependencies of temperature and other parameters on emission angle and target thickness.

Contribution

It introduces a multisource thermal model analysis of proton-carbon collision data, extracting parameters like initial quasi-temperature and demonstrating their angular and positional dependencies.

Findings

Effective temperature varies with emission angle.

Initial quasi-temperature is derived from transverse momentum data.

Model results agree with experimental measurements.

Abstract

The momentum spectra of charged pions ($\pi^+$ and $\pi^-$) and kaons ($K^+$ and $K^-$), as well as protons ($p$), produced in the beam protons induced collisions in a 90-cm-long graphite target [proton-carbon ($p$-C) collisions] at the beam momentum $p_{Lab}=31$ GeV/$c$ are studied in the framework of a multisource thermal model by using Boltzmann distribution and Monte Carlo method. The theoretical model results are approximately in agreement with the experimental data measured by the NA61/SHINE Collaboration. The related free parameters (effective temperature, rapidity shifts, and fraction of non-leading protons) and derived quantities (average transverse momentum and initial quasi-temperature) under given experimental conditions are obtained. It is shown that the considered free parameters and derived quantities to be strongly dependent on emission angle over a range from 0 to 380 mrad and weakly dependent on longitudinal position (graphite target thickness) over a range from 0 to 90 cm.

Tables

Figure	$T$ (GeV)	$y_{\max }$	$y_{\min }$	$N_0(\times 0.001)$	${\chi }^2$/ndof
	$0.320\pm 0.005$	$2.30\pm 0.02$	$1.10\pm 0.02$	$0.143\pm 0.010$	22/2
Fig. 1(a)	$0.138\pm 0.004$	$3.25\pm 0.05$	$1.72\pm 0.06$	$0.962\pm 0.020$	42/12
0$\le$$z$18	$0.195\pm 0.006$	$2.47\pm 0.04$	$1.57\pm 0.03$	$2.918\pm 0.100$	93/12
	$0.205\pm 0.003$	$2.36\pm 0.04$	$1.47\pm 0.03$	$6.431\pm 0.200$	87/9
	$0.220\pm 0.005$	$2.09\pm 0.04$	$1.00\pm 0.03$	$11.108\pm 0.400$	85/9
	$0.222\pm 0.004$	$2.00\pm 0.03$	$0.80\pm 0.04$	$14.541\pm 0.300$	60/9
Fig. 1(b)	$0.169\pm 0.003$	$2.20\pm 0.04$	$0.78\pm 0.02$	$16.701\pm 0.340$	15/9
0$\le$$z$18	$0.166\pm 0.003$	$2.10\pm 0.03$	$0.45\pm 0.02$	$17.572\pm 0.260$	16/6
	$0.166\pm 0.002$	$2.00\pm 0.03$	$0.65\pm 0.03$	$19.149\pm 0.300$	37/6
	$0.166\pm 0.002$	$1.90\pm 0.02$	$0.65\pm 0.02$	$18.495\pm 0.340$	57/6
	$0.166\pm 0.001$	$1.80\pm 0.02$	$0.65\pm 0.02$	$17.839\pm 0.200$	70/6
Fig. 1(c)	$0.136\pm 0.002$	$2.08\pm 0.06$	$0.75\pm 0.04$	$31.163\pm 0.720$	35/3
0$\le$$z$18	$0.160\pm 0.003$	$1.75\pm 0.03$	$0.55\pm 0.02$	$25.050\pm 0.560$	28/2
	$0.115\pm 0.004$	$2.08\pm 0.08$	$0.90\pm 0.05$	$26.483\pm 0.800$	12/1
	$0.115\pm 0.004$	$2.08\pm 0.04$	$0.85\pm 0.10$	$25.278\pm 1.200$	2/$-$
	$0.320\pm 0.010$	$2.50\pm 0.02$	$1.48\pm 0.01$	$0.571\pm 0.020$	49/3
Fig. 1(d)	$0.210\pm 0.004$	$2.73\pm 0.02$	$1.50\pm 0.04$	$5.224\pm 0.080$	48/12
18$\le$$z$36	$0.198\pm 0.003$	$2.56\pm 0.04$	$1.57\pm 0.03$	$17.336\pm 0.400$	76/12
	$0.215\pm 0.004$	$2.30\pm 0.03$	$1.35\pm 0.02$	$28.156\pm 1.000$	90/9
	$0.224\pm 0.004$	$2.09\pm 0.03$	$1.00\pm 0.02$	$31.294\pm 0.400$	67/9
	$0.222\pm 0.005$	$1.90\pm 0.04$	$0.70\pm 0.03$	$31.345\pm 0.800$	70/9
Fig. 1(e)	$0.169\pm 0.004$	$2.20\pm 0.03$	$0.80\pm 0.05$	$30.855\pm 0.400$	29/9
18$\le$$z$36	$0.172\pm 0.005$	$2.10\pm 0.02$	$0.45\pm 0.02$	$28.588\pm 0.600$	3/6
	$0.168\pm 0.002$	$1.90\pm 0.04$	$0.55\pm 0.05$	$25.800\pm 0.400$	19/6
	$0.166\pm 0.001$	$1.90\pm 0.02$	$0.65\pm 0.01$	$24.237\pm 0.200$	50/6
	$0.167\pm 0.002$	$1.78\pm 0.03$	$0.65\pm 0.02$	$22.902\pm 0.400$	64/6
Fig. 1(f)	$0.137\pm 0.001$	$1.95\pm 0.02$	$0.75\pm 0.02$	$38.121\pm 0.800$	44/3
18$\le$$z$36	$0.160\pm 0.002$	$1.75\pm 0.03$	$0.45\pm 0.03$	$33.929\pm 0.800$	22/2
	$0.155\pm 0.002$	$1.70\pm 0.03$	$0.45\pm 0.02$	$30.541\pm 0.800$	6/1
	$0.182\pm 0.003$	$0.70\pm 0.02$	$0.55\pm 0.03$	$31.012\pm 0.600$	7/0
	$0.300\pm 0.002$	$2.50\pm 0.02$	$1.40\pm 0.02$	$1.064\pm 0.030$	38/3
Fig. 1(g)	$0.193\pm 0.003$	$2.85\pm 0.01$	$1.55\pm 0.02$	$10.836\pm 0.200$	108/12
36$\le$$z$54	$0.195\pm 0.003$	$2.60\pm 0.05$	$1.57\pm 0.03$	$23.318\pm 0.400$	85/12
	$0.215\pm 0.005$	$2.30\pm 0.03$	$0.95\pm 0.03$	$21.566\pm 0.600$	60/9
	$0.220\pm 0.003$	$2.09\pm 0.02$	$0.90\pm 0.02$	$27.103\pm 0.400$	69/9
	$0.242\pm 0.002$	$1.88\pm 0.02$	$0.25\pm 0.03$	$26.968\pm 0.600$	42/9
Fig. 1(h)	$0.169\pm 0.003$	$2.20\pm 0.02$	$0.70\pm 0.03$	$26.177\pm 0.400$	29/9
36$\le$$z$54	$0.168\pm 0.003$	$2.10\pm 0.04$	$0.40\pm 0.05$	$22.962\pm 0.400$	13/6
	$0.166\pm 0.005$	$1.95\pm 0.03$	$0.30\pm 0.02$	$21.297\pm 0.600$	40/6
	$0.166\pm 0.002$	$1.93\pm 0.03$	$0.35\pm 0.04$	$19.830\pm 0.500$	44/6
	$0.166\pm 0.002$	$1.70\pm 0.07$	$0.25\pm 0.05$	$17.778\pm 0.300$	97/6
Fig. 1(i)	$0.138\pm 0.002$	$1.95\pm 0.03$	$0.75\pm 0.04$	$32.081\pm 0.800$	37/3
36$\le$$z$54	$0.160\pm 0.003$	$1.75\pm 0.05$	$0.20\pm 0.04$	$23.055\pm 0.600$	5/2
	$0.155\pm 0.005$	$1.70\pm 0.05$	$0.35\pm 0.04$	$26.196\pm 0.800$	6/1
	$0.186\pm 0.005$	$0.70\pm 0.07$	$0.50\pm 0.05$	$21.033\pm 0.600$	22/1
	$0.300\pm 0.004$	$2.70\pm 0.02$	$0.80\pm 0.04$	$1.561\pm 0.040$	66/3
Fig. 1(j)	$0.188\pm 0.001$	$2.93\pm 0.02$	$1.60\pm 0.02$	$11.850\pm 0.200$	145/12
54$\le$$z$72	$0.195\pm 0.003$	$2.60\pm 0.03$	$1.50\pm 0.02$	$18.466\pm 0.400$	81/12
	$0.215\pm 0.005$	$2.30\pm 0.03$	$0.80\pm 0.03$	$21.028\pm 0.500$	60/9
	$0.220\pm 0.004$	$2.10\pm 0.03$	$0.80\pm 0.02$	$21.284\pm 0.400$	72/9
	$0.242\pm 0.005$	$1.80\pm 0.02$	$0.50\pm 0.03$	$19.705\pm 0.300$	76/9
Fig. 1(k)	$0.169\pm 0.002$	$2.20\pm 0.02$	$0.85\pm 0.03$	$19.159\pm 0.400$	36/9
54$\le$$z$72	$0.168\pm 0.004$	$2.10\pm 0.04$	$0.30\pm 0.03$	$16.753\pm 0.400$	13/6
	$0.165\pm 0.001$	$1.60\pm 0.01$	$0.30\pm 0.01$	$14.510\pm 0.200$	87/6
	$0.166\pm 0.001$	$1.85\pm 0.03$	$0.30\pm 0.02$	$15.317\pm 0.300$	35/6
	$0.166\pm 0.001$	$1.70\pm 0.05$	$0.35\pm 0.03$	$14.737\pm 0.200$	94/6
Fig. 1(l)	$0.138\pm 0.002$	$2.20\pm 0.02$	$0.60\pm 0.02$	$26.931\pm 0.400$	22/3
54$\le$$z$72	$0.160\pm 0.002$	$1.75\pm 0.03$	$0.20\pm 0.03$	$23.055\pm 0.400$	5/2
	$0.155\pm 0.002$	$1.50\pm 0.04$	$0.35\pm 0.03$	$20.234\pm 0.240$	8/1
	$0.182\pm 0.001$	$0.85\pm 0.02$	$0.65\pm 0.01$	$17.919\pm 0.280$	16/1
	$0.320\pm 0.005$	$2.60\pm 0.03$	$1.00\pm 0.03$	$1.791\pm 0.020$	49/3
Fig. 1(m)	$0.210\pm 0.003$	$2.80\pm 0.02$	$1.60\pm 0.03$	$10.081\pm 0.300$	56/12
72$\le$$z$90	$0.195\pm 0.002$	$2.65\pm 0.03$	$1.30\pm 0.03$	$13.984\pm 0.400$	67/12
	$0.215\pm 0.004$	$2.30\pm 0.02$	$0.70\pm 0.03$	$15.619\pm 0.300$	52/9
	$0.220\pm 0.003$	$2.10\pm 0.03$	$0.50\pm 0.03$	$15.793\pm 0.400$	66/9
	$0.242\pm 0.003$	$1.80\pm 0.02$	$0.40\pm 0.02$	$15.019\pm 0.300$	64/9
Fig. 1(n)	$0.169\pm 0.003$	$2.14\pm 0.02$	$0.85\pm 0.03$	$14.177\pm 0.400$	73/9
72$\le$$z$90	$0.168\pm 0.004$	$2.10\pm 0.03$	$0.30\pm 0.03$	$12.801\pm 0.300$	9/6
	$0.210\pm 0.003$	$1.60\pm 0.03$	$0.30\pm 0.02$	$11.752\pm 0.200$	14/6
	$0.175\pm 0.003$	$1.80\pm 0.05$	$0.20\pm 0.03$	$11.763\pm 0.200$	36/6
	$0.166\pm 0.005$	$1.70\pm 0.04$	$0.25\pm 0.05$	$11.174\pm 0.200$	66/6
Fig. 1(o)	$0.138\pm 0.002$	$2.00\pm 0.03$	$0.50\pm 0.03$	$18.580\pm 0.400$	35/3
72$\le$$z$90	$0.160\pm 0.002$	$1.75\pm 0.02$	$0.20\pm 0.02$	$18.836\pm 0.200$	13/2
	$0.155\pm 0.002$	$1.50\pm 0.06$	$0.35\pm 0.02$	$14.886\pm 0.400$	3/1
	$0.200\pm 0.003$	$0.85\pm 0.04$	$0.45\pm 0.03$	$14.089\pm 0.400$	19/1
	$0.320\pm 0.001$	$2.60\pm 0.01$	$1.00\pm 0.01$	$16.231\pm 0.200$	46/3
Fig. 1(p)	$0.200\pm 0.003$	$2.80\pm 0.02$	$1.60\pm 0.03$	$20.333\pm 0.200$	97/12
$z$$=$90	$0.195\pm 0.005$	$2.62\pm 0.03$	$1.30\pm 0.03$	$16.733\pm 0.200$	88/12
	$0.210\pm 0.004$	$2.30\pm 0.02$	$0.70\pm 0.03$	$13.641\pm 0.300$	50/9
	$0.210\pm 0.002$	$2.00\pm 0.01$	$0.40\pm 0.02$	$10.621\pm 0.200$	104/9
	$0.242\pm 0.003$	$1.60\pm 0.02$	$0.10\pm 0.02$	$14.572\pm 0.400$	83/9
Fig. 1(q)	$0.169\pm 0.003$	$1.80\pm 0.03$	$0.90\pm 0.02$	$8.858\pm 0.400$	64/6
$z$$=$90	$0.170\pm 0.002$	$1.60\pm 0.03$	$0.60\pm 0.02$	$7.038\pm 0.120$	118/6
	$0.240\pm 0.002$	$1.00\pm 0.02$	$0.20\pm 0.03$	$4.561\pm 0.240$	71/3
	$0.150\pm 0.003$	$1.82\pm 0.03$	$0.10\pm 0.02$	$3.306\pm 0.200$	29/2

Figure	$T$ (GeV)	$y_{\max }$	$y_{\min }$	$N_0(\times 0.001)$	${\chi }^2$/ndof
	$0.320\pm 0.005$	$2.30\pm 0.02$	$1.10\pm 0.02$	$0.077\pm 0.002$	33/2
Fig. 2(a)	$0.138\pm 0.004$	$3.00\pm 0.03$	$1.72\pm 0.03$	$0.702\pm 0.020$	116/12
0$\le$$z$18	$0.195\pm 0.004$	$2.40\pm 0.02$	$1.00\pm 0.03$	$1.987\pm 0.060$	71/12
	$0.208\pm 0.003$	$2.36\pm 0.04$	$0.70\pm 0.03$	$4.859\pm 0.100$	88/9
	$0.230\pm 0.003$	$2.10\pm 0.02$	$0.40\pm 0.04$	$8.318\pm 0.120$	18/9
	$0.260\pm 0.004$	$1.80\pm 0.02$	$0.40\pm 0.02$	$11.530\pm 0.200$	33/9
Fig. 2(b)	$0.169\pm 0.002$	$2.14\pm 0.05$	$0.65\pm 0.03$	$13.579\pm 0.200$	18/9
0$\le$$z$18	$0.168\pm 0.004$	$2.05\pm 0.03$	$0.30\pm 0.03$	$14.905\pm 0.300$	27/6
	$0.200\pm 0.003$	$1.60\pm 0.02$	$0.50\pm 0.03$	$14.783\pm 0.300$	50/6
	$0.175\pm 0.003$	$1.77\pm 0.02$	$0.35\pm 0.04$	$15.571\pm 0.300$	37/6
	$0.210\pm 0.030$	$1.35\pm 0.03$	$0.25\pm 0.02$	$15.253\pm 0.200$	39/6
Fig. 2(c)	$0.138\pm 0.002$	$2.00\pm 0.04$	$0.50\pm 0.03$	$27.457\pm 0.400$	28/3
0$\le$$z$18	$0.138\pm 0.002$	$1.75\pm 0.04$	$0.60\pm 0.03$	$23.691\pm 0.400$	38/2
	$0.155\pm 0.003$	$1.05\pm 0.02$	$0.65\pm 0.02$	$21.444\pm 0.400$	12/1
	$0.160\pm 0.003$	$0.85\pm 0.02$	$0.75\pm 0.03$	$30.222\pm 0.400$	2/$-$
	$0.280\pm 0.004$	$2.40\pm 0.03$	$0.06\pm 0.03$	$0.313\pm 0.020$	57/3
Fig. 2(d)	$0.138\pm 0.002$	$3.00\pm 0.02$	$1.52\pm 0.03$	$3.618\pm 0.140$	73/12
18$\le$$z$36	$0.225\pm 0.003$	$2.30\pm 0.02$	$1.00\pm 0.02$	$11.850\pm 0.200$	84/12
	$0.208\pm 0.003$	$2.36\pm 0.03$	$0.70\pm 0.03$	$19.958\pm 0.300$	69/9
	$0.228\pm 0.002$	$2.10\pm 0.01$	$0.50\pm 0.02$	$24.746\pm 0.400$	9/9
	$0.262\pm 0.002$	$1.70\pm 0.02$	$0.20\pm 0.02$	$25.438\pm 0.300$	57/9
Fig. 2(e)	$0.182\pm 0.004$	$2.00\pm 0.01$	$0.65\pm 0.03$	$25.160\pm 0.200$	64/9
18$\le$$z$36	$0.169\pm 0.003$	$2.05\pm 0.03$	$0.30\pm 0.05$	$24.000\pm 0.300$	21/6
	$0.200\pm 0.005$	$1.60\pm 0.03$	$0.40\pm 0.02$	$22.373\pm 0.300$	30/6
	$0.175\pm 0.002$	$1.77\pm 0.01$	$0.35\pm 0.05$	$21.727\pm 0.400$	55/6
	$0.270\pm 0.004$	$1.00\pm 0.02$	$0.35\pm 0.03$	$19.006\pm 0.200$	84/6
Fig. 2(f)	$0.139\pm 0.003$	$2.00\pm 0.04$	$0.50\pm 0.03$	$35.492\pm 0.600$	28/3
18$\le$$z$36	$0.138\pm 0.002$	$1.75\pm 0.05$	$0.60\pm 0.03$	$31.840\pm 0.600$	52/2
	$0.155\pm 0.003$	$1.00\pm 0.02$	$0.65\pm 0.02$	$28.264\pm 0.600$	7/1
	$0.080\pm 0.005$	$1.40\pm 0.02$	$1.16\pm 0.03$	$23.464\pm 0.600$	176/0
	$0.280\pm 0.004$	$2.40\pm 0.03$	$0.06\pm 0.03$	$0.690\pm 0.020$	36/3
Fig. 2(g)	$0.149\pm 0.003$	$3.00\pm 0.03$	$1.52\pm 0.04$	$7.345\pm 0.159$	95/12
36$\le$$z$54	$0.225\pm 0.003$	$2.45\pm 0.03$	$0.60\pm 0.02$	$16.629\pm 0.360$	79/12
	$0.208\pm 0.002$	$2.36\pm 0.03$	$0.60\pm 0.03$	$19.895\pm 0.300$	58/9
	$0.218\pm 0.002$	$2.10\pm 0.02$	$0.30\pm 0.03$	$20.966\pm 0.400$	33/9
	$0.260\pm 0.003$	$1.70\pm 0.02$	$0.20\pm 0.02$	$22.186\pm 0.400$	48/9
Fig. 2(h)	$0.182\pm 0.002$	$2.00\pm 0.03$	$0.55\pm 0.03$	$20.936\pm 0.360$	63/9
36$\le$$z$54	$0.170\pm 0.002$	$2.05\pm 0.03$	$0.30\pm 0.03$	$20.232\pm 0.300$	25/6
	$0.210\pm 0.004$	$1.60\pm 0.04$	$0.40\pm 0.03$	$17.743\pm 0.200$	9/6
	$0.175\pm 0.002$	$1.77\pm 0.01$	$0.35\pm 0.02$	$18.830\pm 0.300$	41/6
	$0.270\pm 0.002$	$1.00\pm 0.01$	$0.15\pm 0.01$	$16.232\pm 0.200$	74/6
Fig. 2(i)	$0.140\pm 0.002$	$2.00\pm 0.01$	$0.50\pm 0.02$	$31.730\pm 0.640$	30/3
36$\le$$z$54	$0.138\pm 0.002$	$1.75\pm 0.02$	$0.40\pm 0.02$	$24.610\pm 0.400$	47/2
	$0.155\pm 0.002$	$1.05\pm 0.02$	$0.70\pm 0.03$	$23.472\pm 0.600$	9/1
	$0.090\pm 0.003$	$1.40\pm 0.02$	$0.16\pm 0.01$	$19.198\pm 0.400$	8/0
	$0.280\pm 0.004$	$2.50\pm 0.03$	$0.06\pm 0.03$	$0.943\pm 0.020$	41/3
Fig. 2(j)	$0.149\pm 0.003$	$3.05\pm 0.02$	$1.52\pm 0.03$	$7.362\pm 0.200$	65/12
54$\le$$z$72	$0.225\pm 0.004$	$2.40\pm 0.02$	$0.60\pm 0.02$	$13.744\pm 0.200$	61/12
	$0.208\pm 0.003$	$2.36\pm 0.01$	$0.60\pm 0.03$	$15.998\pm 0.200$	60/9
	$0.220\pm 0.003$	$2.08\pm 0.02$	$0.30\pm 0.03$	$16.243\pm 0.240$	13/9
	$0.260\pm 0.004$	$1.70\pm 0.02$	$0.30\pm 0.02$	$16.868\pm 0.240$	50/9
Fig. 2(k)	$0.184\pm 0.002$	$2.00\pm 0.02$	$0.55\pm 0.03$	$15.986\pm 0.200$	70/9
54$\le$$z$72	$0.170\pm 0.003$	$2.05\pm 0.03$	$0.20\pm 0.02$	$15.533\pm 0.200$	28/6
	$0.210\pm 0.004$	$1.55\pm 0.02$	$0.20\pm 0.03$	$13.369\pm 0.200$	48/6
	$0.175\pm 0.003$	$1.77\pm 0.03$	$0.35\pm 0.02$	$14.123\pm 0.200$	25/6
	$0.280\pm 0.004$	$1.00\pm 0.03$	$0.15\pm 0.03$	$12.808\pm 0.100$	66/6
Fig. 2(l)	$0.140\pm 0.002$	$2.00\pm 0.02$	$0.40\pm 0.02$	$23.940\pm 0.400$	31/3
54$\le$$z$72	$0.138\pm 0.002$	$1.75\pm 0.03$	$0.40\pm 0.04$	$19.141\pm 0.400$	44/2
	$0.155\pm 0.002$	$1.05\pm 0.03$	$0.70\pm 0.02$	$15.698\pm 0.400$	16/1
	$0.135\pm 0.003$	$2.70\pm 0.02$	$0.66\pm 0.02$	$15.298\pm 0.400$	26/1
	$0.280\pm 0.002$	$2.50\pm 0.03$	$0.06\pm 0.02$	$1.019\pm 0.020$	43/3
Fig. 2(m)	$0.149\pm 0.003$	$3.05\pm 0.03$	$1.52\pm 0.03$	$6.509\pm 0.240$	73/12
72$\le$$z$90	$0.225\pm 0.002$	$2.37\pm 0.02$	$0.60\pm 0.03$	$9.724\pm 0.200$	88/12
	$0.208\pm 0.002$	$2.30\pm 0.03$	$0.40\pm 0.03$	$11.638\pm 0.200$	86/9
	$0.220\pm 0.002$	$2.02\pm 0.02$	$0.25\pm 0.02$	$12.192\pm 0.200$	23/9
	$0.260\pm 0.003$	$1.60\pm 0.02$	$0.30\pm 0.02$	$12.207\pm 0.200$	51/9
Fig. 2(n)	$0.188\pm 0.002$	$1.90\pm 0.03$	$0.55\pm 0.03$	$11.864\pm 0.200$	33/9
72$\le$$z$90	$0.170\pm 0.003$	$2.05\pm 0.02$	$0.20\pm 0.03$	$11.571\pm 0.200$	7/6
	$0.210\pm 0.003$	$1.55\pm 0.02$	$0.20\pm 0.02$	$11.074\pm 0.200$	45/6
	$0.175\pm 0.003$	$1.77\pm 0.02$	$0.35\pm 0.03$	$11.769\pm 0.200$	41/6
	$0.280\pm 0.003$	$1.00\pm 0.03$	$0.15\pm 0.04$	$10.322\pm 0.200$	50/6
Fig. 2(o)	$0.140\pm 0.003$	$2.00\pm 0.04$	$0.30\pm 0.03$	$18.405\pm 0.400$	23/3
72$\le$$z$90	$0.138\pm 0.004$	$1.75\pm 0.04$	$0.40\pm 0.05$	$15.381\pm 0.400$	30/2
	$0.155\pm 0.004$	$1.05\pm 0.03$	$0.70\pm 0.03$	$12.841\pm 0.600$	15/1
	$0.135\pm 0.002$	$2.70\pm 0.04$	$0.06\pm 0.04$	$11.641\pm 0.400$	19/1
	$0.280\pm 0.006$	$2.60\pm 0.04$	$0.06\pm 0.01$	$9.687\pm 0.200$	47/3
Fig. 2(p)	$0.147\pm 0.002$	$3.10\pm 0.02$	$1.32\pm 0.02$	$14.156\pm 0.140$	18/12
$z$$=$90	$0.225\pm 0.003$	$2.32\pm 0.03$	$0.60\pm 0.03$	$11.283\pm 0.200$	70/12
	$0.208\pm 0.002$	$2.30\pm 0.02$	$0.40\pm 0.03$	$10.248\pm 0.160$	66/9
	$0.220\pm 0.003$	$2.00\pm 0.02$	$0.30\pm 0.02$	$8.134\pm 0.200$	64/9
	$0.260\pm 0.004$	$1.55\pm 0.01$	$0.30\pm 0.02$	$12.255\pm 0.400$	91/9
Fig. 2(q)	$0.188\pm 0.004$	$1.80\pm 0.02$	$0.25\pm 0.02$	$8.593\pm 0.400$	30/6
$z$$=$90	$0.165\pm 0.002$	$1.80\pm 0.03$	$0.20\pm 0.03$	$5.816\pm 0.320$	37/6
	$0.210\pm 0.005$	$1.30\pm 0.01$	$0.10\pm 0.03$	$4.394\pm 0.120$	13/3
	$0.175\pm 0.003$	$1.33\pm 0.03$	$0.05\pm 0.04$	$3.019\pm 0.040$	34/2

Figure	$T$ (GeV)	$y_{\max }$	$y_{\min }$	$N_0(\times 0.001)$	${\chi }^2$/ndof
	$0.400\pm 0.004$	$1.91\pm 0.02$	$1.50\pm 0.02$	$1.622\pm 0.040$	48/12
	$0.400\pm 0.004$	$1.92\pm 0.03$	$1.37\pm 0.02$	$6.272\pm 0.100$	57/12
Fig. 3(a)	$0.400\pm 0.004$	$1.97\pm 0.02$	$1.37\pm 0.02$	$10.672\pm 0.200$	95/12
20$\le$$\theta$40	$0.400\pm 0.003$	$2.05\pm 0.01$	$1.30\pm 0.02$	$11.335\pm 0.240$	55/12
	$0.400\pm 0.005$	$2.05\pm 0.02$	$1.30\pm 0.02$	$8.904\pm 0.240$	68/12
	$0.340\pm 0.001$	$2.22\pm 0.01$	$1.20\pm 0.02$	$19.874\pm 0.400$	231/12
	$0.200\pm 0.004$	$2.01\pm 0.03$	$0.80\pm 0.02$	$30.276\pm 0.400$	30/9
	$0.230\pm 0.003$	$1.90\pm 0.02$	$0.20\pm 0.02$	$58.805\pm 1.600$	19/9
Fig. 3(b)	$0.228\pm 0.002$	$1.89\pm 0.03$	$0.20\pm 0.02$	$46.620\pm 1.600$	11/9
100$\le$$\theta$140	$0.230\pm 0.003$	$1.86\pm 0.02$	$0.10\pm 0.02$	$34.882\pm 0.800$	17/9
	$0.220\pm 0.004$	$1.85\pm 0.03$	$0.35\pm 0.02$	$26.181\pm 0.600$	20/9
	$0.235\pm 0.003$	$1.75\pm 0.02$	$0.10\pm 0.02$	$12.809\pm 0.400$	37/9
	$0.440\pm 0.005$	$1.80\pm 0.02$	$0.30\pm 0.03$	$1.034\pm 0.020$	57/12
	$0.400\pm 0.004$	$1.92\pm 0.03$	$0.50\pm 0.03$	$4.136\pm 0.200$	16/12
Fig. 3(c)	$0.400\pm 0.004$	$1.97\pm 0.03$	$0.30\pm 0.02$	$7.232\pm 0.160$	52/12
20$\le$$\theta$40	$0.400\pm 0.005$	$2.00\pm 0.03$	$0.30\pm 0.03$	$7.329\pm 0.200$	23/12
	$0.444\pm 0.004$	$1.82\pm 0.02$	$0.50\pm 0.02$	$5.935\pm 0.100$	26/12
	$0.345\pm 0.005$	$2.08\pm 0.02$	$0.60\pm 0.02$	$12.610\pm 0.200$	40/12
	$0.202\pm 0.002$	$2.03\pm 0.02$	$0.30\pm 0.02$	$24.814\pm 0.480$	17/9
	$0.230\pm 0.005$	$1.86\pm 0.02$	$0.10\pm 0.02$	$48.532\pm 0.800$	15/9
Fig. 3(d)	$0.230\pm 0.004$	$1.81\pm 0.02$	$0.10\pm 0.02$	$40.351\pm 0.600$	36/9
100$\le$$\theta$140	$0.240\pm 0.004$	$1.73\pm 0.02$	$0.23\pm 0.02$	$30.234\pm 0.800$	11/9
	$0.245\pm 0.002$	$1.70\pm 0.02$	$0.22\pm 0.02$	$23.424\pm 0.520$	27/9
	$0.245\pm 0.002$	$1.68\pm 0.02$	$0.10\pm 0.02$	$10.480\pm 0.520$	36/9

Figure	$T$ (GeV)	$y_{\max }$	$y_{\min }$	$N_0(\times 0.001)$	${\chi }^2$/ndof
	$0.300\pm 0.003$	$2.00\pm 0.03$	$1.20\pm 0.03$	$0.335\pm 0.012$	18/2
Fig. 4(a)	$0.300\pm 0.003$	$1.90\pm 0.02$	$1.10\pm 0.03$	$3.079\pm 0.120$	30/2
0$\le$$z$18	$0.300\pm 0.003$	$1.45\pm 0.03$	$1.10\pm 0.03$	$4.787\pm 0.180$	24/2
	$0.300\pm 0.004$	$1.10\pm 0.02$	$0.60\pm 0.03$	$6.462\pm 0.300$	31/2
	$0.400\pm 0.003$	$2.00\pm 0.03$	$1.20\pm 0.03$	$2.569\pm 0.060$	8/2
Fig. 4(b)	$0.300\pm 0.003$	$2.00\pm 0.03$	$1.10\pm 0.02$	$9.552\pm 0.300$	26/2
18$\le$$z$36	$0.400\pm 0.004$	$1.00\pm 0.02$	$0.95\pm 0.01$	$8.080\pm 0.180$	27/2
	$0.320\pm 0.004$	$1.08\pm 0.02$	$0.70\pm 0.03$	$8.773\pm 0.100$	25/2
	$0.420\pm 0.004$	$1.75\pm 0.02$	$1.35\pm 0.02$	$3.828\pm 0.060$	47/4
Fig. 4(c)	$0.300\pm 0.004$	$1.85\pm 0.04$	$1.10\pm 0.03$	$7.922\pm 0.180$	39/2
36$\le$$z$54	$0.280\pm 0.004$	$1.45\pm 0.04$	$1.35\pm 0.03$	$6.561\pm 0.240$	21/2
	$0.316\pm 0.004$	$1.15\pm 0.03$	$0.40\pm 0.04$	$7.016\pm 0.500$	14/2
	$0.400\pm 0.005$	$2.00\pm 0.03$	$1.30\pm 0.02$	$4.065\pm 0.180$	38/4
Fig. 4(d)	$0.300\pm 0.003$	$1.80\pm 0.03$	$1.05\pm 0.03$	$5.934\pm 0.300$	18/2
54$\le$$z$72	$0.360\pm 0.005$	$1.35\pm 0.03$	$0.60\pm 0.06$	$4.578\pm 0.180$	13/2
	$0.275\pm 0.002$	$1.02\pm 0.01$	$1.00\pm 0.01$	$5.361\pm 0.200$	38/2
	$0.400\pm 0.004$	$2.20\pm 0.03$	$1.35\pm 0.03$	$3.806\pm 0.120$	14/4
Fig. 4(e)	$0.300\pm 0.004$	$1.80\pm 0.03$	$1.05\pm 0.03$	$4.641\pm 0.120$	32/2
72$\le$$z$90	$0.280\pm 0.003$	$1.45\pm 0.03$	$1.20\pm 0.03$	$3.491\pm 0.120$	17/2
	$0.300\pm 0.004$	$1.10\pm 0.03$	$0.50\pm 0.04$	$4.315\pm 0.150$	22/2
Fig. 4(f)	$0.400\pm 0.003$	$2.20\pm 0.03$	$1.00\pm 0.03$	$6.300\pm 0.120$	10/5
$z$$=$90	$0.300\pm 0.006$	$1.79\pm 0.03$	$1.00\pm 0.02$	$3.123\pm 0.060$	36/2

Figure	$T$ (GeV)	$y_{\max }$	$y_{\min }$	$N_0(\times 0.001)$	${\chi }^2$/ndof
	$0.280\pm 0.005$	$1.90\pm 0.03$	$1.80\pm 0.03$	$0.191\pm 0.006$	27/2
Fig. 5(a)	$0.300\pm 0.005$	$1.70\pm 0.03$	$1.10\pm 0.02$	$1.173\pm 0.060$	18/2
0$\le$$z$18	$0.300\pm 0.003$	$1.20\pm 0.01$	$1.10\pm 0.01$	$1.997\pm 0.060$	67/2
	$0.290\pm 0.005$	$1.10\pm 0.04$	$0.50\pm 0.02$	$2.685\pm 0.100$	19/2
	$0.400\pm 0.005$	$1.73\pm 0.03$	$1.20\pm 0.03$	$0.966\pm 0.060$	39/2
Fig. 5(b)	$0.300\pm 0.003$	$1.50\pm 0.03$	$1.30\pm 0.03$	$3.386\pm 0.120$	72/2
18$\le$$z$36	$0.400\pm 0.003$	$1.00\pm 0.02$	$0.70\pm 0.01$	$2.796\pm 0.090$	18/2
	$0.320\pm 0.003$	$0.91\pm 0.02$	$0.70\pm 0.02$	$3.752\pm 0.150$	25/2
	$0.420\pm 0.005$	$1.45\pm 0.02$	$1.40\pm 0.01$	$1.247\pm 0.030$	33/4
Fig. 5(c)	$0.340\pm 0.003$	$1.65\pm 0.03$	$1.10\pm 0.03$	$3.308\pm 0.150$	18/2
36$\le$$z$54	$0.248\pm 0.003$	$1.45\pm 0.03$	$1.30\pm 0.03$	$2.580\pm 0.090$	18/2
	$0.300\pm 0.003$	$1.10\pm 0.03$	$0.60\pm 0.01$	$2.800\pm 0.100$	29/2
	$0.440\pm 0.010$	$1.45\pm 0.07$	$1.30\pm 0.05$	$1.211\pm 0.060$	67/4
Fig. 5(d)	$0.300\pm 0.004$	$1.70\pm 0.03$	$1.05\pm 0.03$	$2.225\pm 0.060$	21/2
54$\le$$z$72	$0.330\pm 0.005$	$1.10\pm 0.03$	$1.03\pm 0.03$	$2.058\pm 0.090$	17/2
	$0.288\pm 0.002$	$1.00\pm 0.02$	$0.95\pm 0.02$	$2.131\pm 0.100$	55/2
	$0.330\pm 0.004$	$1.85\pm 0.03$	$1.28\pm 0.02$	$0.894\pm 0.060$	39/4
Fig. 5(e)	$0.260\pm 0.004$	$2.00\pm 0.04$	$0.60\pm 0.04$	$1.811\pm 0.060$	10/2
72$\le$$z$90	$0.245\pm 0.004$	$1.45\pm 0.03$	$1.00\pm 0.02$	$1.496\pm 0.060$	5/2
	$0.300\pm 0.004$	$0.95\pm 0.03$	$0.63\pm 0.02$	$1.773\pm 0.100$	23/2
Fig. 5(f)	$0.350\pm 0.003$	$2.00\pm 0.02$	$1.00\pm 0.02$	$1.640\pm 0.060$	36/5
$z$$=$90	$0.300\pm 0.004$	$1.60\pm 0.04$	$1.20\pm 0.03$	$1.283\pm 0.060$	39/2

Figure	$T$ (GeV)	$k$	$y_{\max }$	$y_{\min }$	$y_{L\max }$	$y_{L\min }$	$N_0(\times 0.001)$	${\chi }^2$/ndof
	$0.400\pm 0.004$	$0.40\pm 0.01$	$1.60\pm 0.05$	$1.00\pm 0.10$	$4.00\pm 0.07$	$3.55\pm 0.08$	$2.996\pm 0.200$	10/$-$
Fig. 6(a)	$0.280\pm 0.004$	$0.40\pm 0.02$	$1.50\pm 0.10$	$1.20\pm 0.10$	$3.10\pm 0.10$	$2.70\pm 0.10$	$1.337\pm 0.020$	118/9
0$\le$$z$18	$0.200\pm 0.005$	$0.40\pm 0.02$	$1.50\pm 0.08$	$1.20\pm 0.10$	$3.45\pm 0.10$	$2.00\pm 0.08$	$2.145\pm 0.100$	86/7
	$0.127\pm 0.003$	$0.40\pm 0.01$	$1.55\pm 0.07$	$1.50\pm 0.06$	$3.45\pm 0.05$	$2.20\pm 0.05$	$7.216\pm 0.160$	202/6
	$0.125\pm 0.005$	$0.45\pm 0.01$	$1.55\pm 0.05$	$0.90\pm 0.05$	$3.45\pm 0.08$	$2.00\pm 0.05$	$10.156\pm 0.400$	128/6
	$0.115\pm 0.003$	$0.40\pm 0.01$	$0.98\pm 0.02$	$0.80\pm 0.02$	$3.90\pm 0.08$	$1.30\pm 0.05$	$11.629\pm 0.400$	50/3
Fig. 6(b)	$0.150\pm 0.004$	$0.54\pm 0.02$	$0.80\pm 0.03$	$0.70\pm 0.03$	$2.80\pm 0.07$	$0.60\pm 0.10$	$13.653\pm 0.400$	57/3
0$\le$$z$18	$0.164\pm 0.004$	$0.53\pm 0.02$	$0.80\pm 0.03$	$0.70\pm 0.03$	$3.50\pm 0.10$	$0.60\pm 0.20$	$13.653\pm 0.400$	57/$-$
	$0.177\pm 0.005$	$0.53\pm 0.02$	$0.80\pm 0.05$	$0.70\pm 0.05$	$3.00\pm 0.12$	$1.50\pm 0.10$	$12.291\pm 0.800$	28/$-$
	$0.140\pm 0.010$	$0.35\pm 0.02$	$0.40\pm 0.05$	$0.30\pm 0.05$	$3.50\pm 0.10$	$1.00\pm 0.05$	$27.176\pm 0.800$	5/$-$
	$0.450\pm 0.010$	$0.53\pm 0.02$	$1.60\pm 0.10$	$1.00\pm 0.10$	$4.00\pm 0.10$	$3.55\pm 0.05$	$8.988\pm 0.400$	9/$-$
Fig. 6(c)	$0.280\pm 0.006$	$0.43\pm 0.02$	$1.50\pm 0.20$	$1.20\pm 0.20$	$3.10\pm 0.03$	$2.70\pm 0.03$	$7.496\pm 0.300$	117/9
18$\le$$z$36	$0.200\pm 0.003$	$0.49\pm 0.01$	$1.50\pm 0.05$	$1.20\pm 0.06$	$3.45\pm 0.05$	$2.10\pm 0.03$	$14.518\pm 0.400$	42/7
	$0.130\pm 0.006$	$0.45\pm 0.02$	$1.60\pm 0.02$	$1.30\pm 0.03$	$3.45\pm 0.03$	$2.20\pm 0.01$	$28.178\pm 0.800$	171/6
	$0.125\pm 0.005$	$0.45\pm 0.02$	$1.55\pm 0.03$	$0.85\pm 0.03$	$3.45\pm 0.05$	$2.00\pm 0.05$	$22.773\pm 0.480$	118/7
	$0.115\pm 0.003$	$0.40\pm 0.01$	$1.00\pm 0.03$	$0.80\pm 0.03$	$3.90\pm 0.04$	$1.40\pm 0.04$	$20.745\pm 0.600$	40/3
Fig. 6(d)	$0.120\pm 0.003$	$0.54\pm 0.01$	$0.65\pm 0.03$	$0.60\pm 0.03$	$2.80\pm 0.05$	$0.90\pm 0.05$	$20.636\pm 0.600$	50/3
18$\le$$z$36	$0.158\pm 0.003$	$0.57\pm 0.03$	$0.60\pm 0.04$	$0.50\pm 0.04$	$3.50\pm 0.10$	$0.80\pm 0.05$	$19.404\pm 0.400$	18/$-$
	$0.167\pm 0.002$	$0.55\pm 0.02$	$0.65\pm 0.02$	$0.55\pm 0.02$	$3.00\pm 0.30$	$1.50\pm 0.08$	$19.730\pm 0.400$	18/$-$
	$0.180\pm 0.006$	$0.34\pm 0.01$	$0.40\pm 0.03$	$0.36\pm 0.02$	$3.50\pm 0.06$	$1.50\pm 0.02$	$47.883\pm 0.800$	6/$-$
	$0.455\pm 0.005$	$0.53\pm 0.01$	$1.60\pm 0.05$	$1.00\pm 0.06$	$4.06\pm 0.06$	$3.55\pm 0.05$	$18.555\pm 0.400$	11/$-$
Fig. 6(e)	$0.290\pm 0.004$	$0.53\pm 0.01$	$1.50\pm 0.15$	$1.20\pm 0.15$	$3.10\pm 0.02$	$2.70\pm 0.03$	$15.862\pm 0.300$	94/9
36$\le$$z$54	$0.200\pm 0.005$	$0.50\pm 0.01$	$1.50\pm 0.08$	$1.20\pm 0.10$	$3.45\pm 0.05$	$2.10\pm 0.03$	$22.391\pm 0.600$	35/7
	$0.130\pm 0.004$	$0.45\pm 0.01$	$1.60\pm 0.01$	$1.30\pm 0.03$	$3.45\pm 0.03$	$2.15\pm 0.01$	$28.281\pm 0.400$	173/6
	$0.125\pm 0.003$	$0.45\pm 0.02$	$1.55\pm 0.02$	$0.88\pm 0.02$	$3.45\pm 0.02$	$2.00\pm 0.02$	$20.981\pm 0.400$	118/6
	$0.115\pm 0.002$	$0.35\pm 0.01$	$1.00\pm 0.02$	$0.80\pm 0.02$	$4.00\pm 0.03$	$1.50\pm 0.02$	$19.587\pm 0.400$	42/3
Fig. 6(f)	$0.120\pm 0.004$	$0.58\pm 0.02$	$0.70\pm 0.02$	$0.50\pm 0.02$	$2.80\pm 0.02$	$0.90\pm 0.03$	$18.925\pm 0.400$	48/3
36$\le$$z$54	$0.164\pm 0.001$	$0.60\pm 0.02$	$0.60\pm 0.03$	$0.50\pm 0.03$	$3.50\pm 0.20$	$0.80\pm 0.08$	$17.285\pm 0.400$	23/$-$
	$0.155\pm 0.005$	$0.55\pm 0.01$	$0.65\pm 0.04$	$0.55\pm 0.04$	$3.00\pm 0.20$	$1.50\pm 0.10$	$16.519\pm 0.400$	12/$-$
	$0.178\pm 0.004$	$0.43\pm 0.01$	$0.53\pm 0.03$	$0.36\pm 0.03$	$3.50\pm 0.15$	$1.50\pm 0.02$	$37.825\pm 0.960$	7/$-$
	$0.450\pm 0.004$	$0.53\pm 0.01$	$1.60\pm 0.20$	$1.00\pm 0.20$	$4.00\pm 0.05$	$3.55\pm 0.05$	$24.718\pm 0.500$	13/$-$
Fig. 6(g)	$0.290\pm 0.003$	$0.53\pm 0.01$	$1.50\pm 0.03$	$1.20\pm 0.15$	$3.10\pm 0.02$	$2.70\pm 0.03$	$19.202\pm 0.240$	32/9
54$\le$$z$72	$0.200\pm 0.005$	$0.50\pm 0.01$	$1.50\pm 0.10$	$1.20\pm 0.10$	$3.30\pm 0.06$	$2.10\pm 0.05$	$18.359\pm 0.200$	31/7
	$0.130\pm 0.002$	$0.45\pm 0.01$	$1.60\pm 0.01$	$1.30\pm 0.01$	$3.45\pm 0.03$	$2.15\pm 0.01$	$23.629\pm 0.400$	174/6
	$0.130\pm 0.003$	$0.45\pm 0.01$	$1.55\pm 0.02$	$0.88\pm 0.02$	$3.45\pm 0.03$	$2.00\pm 0.03$	$17.502\pm 0.400$	129/6
	$0.145\pm 0.003$	$0.45\pm 0.02$	$0.90\pm 0.02$	$0.70\pm 0.03$	$4.00\pm 0.10$	$0.95\pm 0.03$	$15.343\pm 0.400$	32/3
Fig. 6(h)	$0.115\pm 0.005$	$0.55\pm 0.01$	$0.65\pm 0.03$	$0.50\pm 0.03$	$3.00\pm 0.05$	$1.00\pm 0.05$	$14.933\pm 0.400$	66/3
54$\le$$z$72	$0.160\pm 0.003$	$0.60\pm 0.02$	$0.55\pm 0.03$	$0.50\pm 0.03$	$3.50\pm 0.20$	$0.80\pm 0.02$	$14.798\pm 0.400$	9/$-$
	$0.150\pm 0.004$	$0.55\pm 0.02$	$0.65\pm 0.05$	$0.55\pm 0.05$	$3.00\pm 0.10$	$1.50\pm 0.05$	$13.657\pm 0.400$	16/$-$
	$0.170\pm 0.003$	$0.43\pm 0.01$	$0.53\pm 0.03$	$0.36\pm 0.03$	$3.50\pm 0.07$	$1.50\pm 0.03$	$29.279\pm 0.960$	37/$-$
	$0.450\pm 0.004$	$0.53\pm 0.01$	$1.60\pm 0.03$	$1.00\pm 0.05$	$4.00\pm 0.10$	$3.55\pm 0.10$	$26.965\pm 0.600$	6/$-$
Fig. 6(i)	$0.290\pm 0.003$	$0.53\pm 0.01$	$1.50\pm 0.10$	$1.20\pm 0.15$	$3.10\pm 0.03$	$2.70\pm 0.03$	$17.031\pm 0.280$	33/9
72$\le$$z$90	$0.160\pm 0.004$	$0.50\pm 0.01$	$1.50\pm 0.03$	$1.20\pm 0.02$	$3.45\pm 0.03$	$2.10\pm 0.03$	$13.722\pm 0.240$	19/7
	$0.140\pm 0.004$	$0.60\pm 0.01$	$1.60\pm 0.03$	$0.50\pm 0.03$	$3.60\pm 0.02$	$1.80\pm 0.03$	$18.999\pm 0.480$	99/6
	$0.130\pm 0.004$	$0.50\pm 0.01$	$1.55\pm 0.03$	$0.88\pm 0.02$	$3.45\pm 0.03$	$0.90\pm 0.03$	$13.342\pm 0.520$	133/6
	$0.145\pm 0.005$	$0.53\pm 0.01$	$0.90\pm 0.04$	$0.40\pm 0.05$	$4.00\pm 0.04$	$0.95\pm 0.05$	$12.922\pm 0.520$	8/3
Fig. 6(j)	$0.120\pm 0.001$	$0.55\pm 0.01$	$0.65\pm 0.02$	$0.50\pm 0.01$	$3.00\pm 0.02$	$1.00\pm 0.03$	$11.877\pm 0.480$	51/3
72$\le$$z$90	$0.160\pm 0.002$	$0.63\pm 0.02$	$0.55\pm 0.01$	$0.50\pm 0.01$	$3.50\pm 0.15$	$0.80\pm 0.05$	$11.686\pm 0.320$	10/$-$
	$0.155\pm 0.006$	$0.60\pm 0.03$	$0.65\pm 0.03$	$0.55\pm 0.03$	$3.00\pm 0.15$	$1.20\pm 0.06$	$10.773\pm 0.400$	25/$-$
	$0.170\pm 0.003$	$0.50\pm 0.01$	$0.53\pm 0.02$	$0.36\pm 0.03$	$3.50\pm 0.20$	$1.50\pm 0.05$	$20.968\pm 0.400$	56/$-$
	$0.450\pm 0.010$	$0.53\pm 0.02$	$1.60\pm 0.10$	$1.00\pm 0.04$	$4.15\pm 0.15$	$3.55\pm 0.15$	$193.715\pm 0.460$	44/1
Fig. 6(k)	$0.290\pm 0.005$	$0.53\pm 0.01$	$1.50\pm 0.10$	$1.20\pm 0.10$	$3.10\pm 0.01$	$2.70\pm 0.03$	$36.734\pm 0.460$	186/9
$z$$=$90	$0.160\pm 0.002$	$0.55\pm 0.01$	$1.50\pm 0.03$	$1.20\pm 0.02$	$3.45\pm 0.04$	$2.10\pm 0.03$	$15.771\pm 0.500$	192/9
	$0.140\pm 0.004$	$0.60\pm 0.01$	$1.60\pm 0.03$	$0.50\pm 0.05$	$3.60\pm 0.07$	$1.80\pm 0.06$	$14.012\pm 0.400$	104/6
Fig. 6(l)	$0.130\pm 0.005$	$0.48\pm 0.01$	$1.55\pm 0.03$	$0.88\pm 0.02$	$3.45\pm 0.12$	$1.90\pm 0.03$	$6.526\pm 0.200$	146/6
$z$$=$90	$0.160\pm 0.004$	$0.60\pm 0.01$	$0.65\pm 0.05$	$0.30\pm 0.03$	$2.30\pm 0.02$	$0.60\pm 0.04$	$4.851\pm 0.200$	30/1
	$0.120\pm 0.001$	$0.55\pm 0.01$	$0.65\pm 0.03$	$0.50\pm 0.02$	$3.00\pm 0.02$	$1.00\pm 0.04$	$3.167\pm 0.200$	51/1

Equations

$$f_{p^{\prime }}(p^{\prime })=C{p}^{\prime 2}\exp \left(-\frac{\sqrt{p^{\prime 2}+m_0^2}}{T}\right),$$

$$f_{p^{\prime }}(p^{\prime })=\sum _j{k}_j{C}_j{p}^{\prime 2}\exp \left(-\frac{\sqrt{p^{\prime 2}+m_0^2}}{T_j}\right),$$

$${\int }_0^{p^{\prime }}{f}_{p^{\prime }}(p^{\prime \prime })d{p}^{\prime \prime }<R_1<{\int }_0^{p^{\prime }+\delta p^{\prime }}{f}_{p^{\prime }}(p^{\prime \prime })d{p}^{\prime \prime },$$

$$f_{{\theta }^{\prime }}({\theta }^{\prime })=\frac{1}{2}\sin {\theta }^{\prime }$$

$${\theta }^{\prime }=2\arcsin \left(\sqrt{R_2}\right)$$

$$p_T^{\prime }=p^{\prime }\sin {\theta }^{\prime },$$

$$p_z^{\prime }=p^{\prime }\cos {\theta }^{\prime },$$

$$E^{\prime }=\sqrt{p^{\prime 2}+m_0^2},$$

$$y^{\prime }\equiv \frac{1}{2}\ln \left(\frac{E^{\prime }+p_z^{\prime }}{E^{\prime }-p_z^{\prime }}\right).$$

$$y=y^{\prime }+y_x$$

$$y_x=(y_{\max }-y_{\min })R_3+y_{\min }.$$

$$y_x=(y_{L\max }-y_{L\min })R_4+y_{L\min }.$$

$$p_T=p_T^{\prime },$$

$$p_z=\sqrt{p_T^2+m_0^2}\sinh y,$$

$$p=\sqrt{p_T^2+p_z^2},$$

$$\theta =\arctan \left(\frac{p_T}{p_z}\right).$$

Full text

Multiparticle production and initial quasi-temperature from proton induced carbon collisions at $p_{Lab}=31$ GeV/$c$

Pei-Pin Yang1**E-mail: yangpeipin@qq.com, Mai-Ying Duan1,†††E-mail: duanmaiying@sxu.edu.cn, Fu-Hu Liu1,‡‡‡Corresponding author. E-mail: fuhuliu@163.com; fuhuliu@sxu.edu.cn, Raghunath Sahoo2,*§§§E-mail: Raghunath.Sahoo@cern.ch; raghunath.phy@gmail.com

1*Institute of Theoretical Physics and Department of Physics and

State Key Laboratory of Quantum Optics and Quantum Optics Devices, Shanxi University, Taiyuan, Shanxi 030006, China*

2Discipline of Physics, School of Basic Sciences, Indian Institute of Technology Indore, Simrol, Indore 453552, India

Abstract: The momentum spectra of charged pions ($\pi^{+}$ and $\pi^{-}$) and kaons ($K^{+}$ and $K^{-}$), as well as protons ($p$), produced in the beam protons induced collisions in a 90-cm-long graphite target [proton-carbon ($p$-C) collisions] at the beam momentum $p_{Lab}=31$ GeV/$c$ are studied in the framework of a multisource thermal model by using Boltzmann distribution and Monte Carlo method. The theoretical model results are approximately in agreement with the experimental data measured by the NA61/SHINE Collaboration. The related free parameters (effective temperature, rapidity shifts, and fraction of non-leading protons) and derived quantities (average transverse momentum and initial quasi-temperature) under given experimental conditions are obtained. It is shown that the considered free parameters and derived quantities to be strongly dependent on emission angle over a range from 0 to 380 mrad and weakly dependent on longitudinal position (graphite target thickness) over a range from 0 to 90 cm.

Keywords: Momentum spectra, effective temperature, rapidity shift, average transverse momentum, initial quasi-temperature

PACS: 14.40.-n, 14.20.-c, 24.10.Pa

1 Introduction

High energy (relativistic) nucleus-nucleus (heavy ion) collisions with nearly zero impact parameter (central collisions) are believed to form Quark-Gluon Plasma (QGP) or quark matter [1, 2, 3] in the laboratory. High energy nucleus-nucleus collisions with large impact parameter are not expected to form QGP due to low particle multiplicity yielding lower energy density and temperature [4]. Small collision systems such as proton-nucleus and proton-proton collisions at high energy, produce usually low multiplicity, which are not expected to form QGP, but are useful to study the multiparticle production processes. However, a few of proton-nucleus and proton-proton collisions at the LHC energies can produce high multiplicity due to nearly zero “impact parameter”, which are possibly expected to form QGP, where the concept “impact parameter” or “centrality” used in nuclear collisions are used in proton-proton collisions [5]. Degree of collectivity, long-range correlations, strangeness enhancement etc., which are considered as QGP-like signatures, are recently observed in these high multiplicity events [6, 7, 8].

Assuming nucleus-nucleus collisions as a mere superposition of proton-proton collisions in the absence of any nuclear effects, usually one considers proton-proton collisions as the baseline measurements. On the other hand, proton-nucleus collisions [9, 10, 11, 12, 13] serve as studying the initial state effects and making a bridge between proton-proton [14, 15, 16, 17, 18] to nucleus-nucleus collisions [19, 20, 21, 22, 23] while studying the multiparticle production processes, though fewer particles are produced in proton-nucleus collisions than in nucleus-nucleus collisions.

There are different types of models or theories being introduced in the studies of high energy collisions [24, 25]. Among these models or theories, different versions of thermal and statistical models [26, 27, 28, 29] characterize some of the aspects of high-energy nuclear collisions, while there are many other aspects that are studied by other approaches. As a basic concept, temperature is ineluctable to be used in analyses. In fact, not only the “temperature is surely one of the central concepts in thermodynamics and statistical mechanics” [30], but also it is very important due to its extremely wide applications in experimental measurements and theoretical studies in subatomic physics, especially in high energy and nuclear physics.

In view of this importance, in this paper, we are interested in the study of proton-nucleus collisions at high energy by using the Boltzmann distribution and the Monte Carlo Method in the framework of the multisource thermal model [31]. The theoretical model results are compared with the experimental data of the beam protons induced collisions in a 90-cm-long graphite target [proton-carbon ($p$-C) collisions] at the beam momentum $p_{Lab}=31$ GeV/$c$ measured by the NA61/SHINE Collaboration [32] at the Super Proton Synchrotron (SPS), the European Organisation for Nuclear Research or the European Laboratory for Particle Physics (CERN).

The remainder of this paper is structured as follows. The formalism and method are shortly described in Section 2. Results and discussion are given in Section 3. In Section 4, we summarize our main observations and conclusions.

2 Formalism and method

According to the multisource thermal model [31], it is assumed that there are many local emission sources to be formed in high energy collisions due to different excitation degrees, rapidity shifts, reaction mechanisms, impact parameters (or centralities). In the transverse plane, the local emission sources with the same excitation degree form a (large) emission source. In the rapidity space, the local emission sources with the same rapidity shift form a (large) emission source. In the rest frame of an emission source with a determined excitation degree, the particles are assumed to be emitted isotropically.

In the rest frame of a given emission source, let $T$ denote the temperature parameter. The particles with rest mass $m_{0}$ produced in the rest frame of the emission source are assumed to have the simplest Boltzmann distribution of momenta $p^{\prime}$ [33]. That is

[TABLE]

where $C$ is the normalization constant which is related to $T$. As a probability density function, Eq. (1) is naturally normalized to 1.

If we need to consider multiple sources, we can use a superposition of different equations with different temperatures and fractions. We have

[TABLE]

where $k_{j}$, $C_{j}$, and $T_{j}$ are the fraction, normalization constant, and temperature for the $j$-th source or component. The average temperature obtained from Eq. (2) is $T=\sum_{j}k_{j}T_{j}/\sum_{j}k_{j}=\sum_{j}k_{j}T_{j}$ due to $\sum_{j}k_{j}=1$. The derived parameter $T$ is the weighted average over various components, but not the simple weighted sum.

It should be noted that $T$ or $T_{j}$ is not the “real” temperature of the emission source, but the effective temperature due to the fact that the flow effect is not excluded in the momentum spectrum. The “real” temperature is generally smaller than the effective temperature which contains the contribution of collective radial flow effect. To disengage the thermal motion and collective flow effect, one may use different methods such as the blast-wave model [34, 35] or any alternative method [36, 37]. As an example, we shall discuss shortly the results of the blast-wave model in section 3.

The contribution of spin being small, is not included in Eq. (1). The effect of chemical potential ($\mu$) is not included in Eq. (1) as well, due to the fact that $\mu$ affects only the normalization, but not the trend, of the spectrum if the spin effect is neglected. Our previous work [38] shows that the spin effect together with $\mu\gg m_{0}$ or $\mu\ll m_{0}$ is so small ($<1\%$) that we do not need to consider it in studying momentum or transverse momentum spectra in high energy collisions. Only the combination of spin and $\mu\approx m_{0}$ causes an obvious effect, which is not the case in this paper.

In the Monte Carlo method [39, 40], let $R_{1,2,3,4}$ denote random numbers distributed evenly in $[0,1]$. To obtain a concrete value of $p^{\prime}$ which satisfies Eq. (1) or one of the components in Eq. (2), we can perform the solution of

[TABLE]

where $\delta p^{\prime}$ denotes a small shift relative to $p^{\prime}$.

Under the assumption of isotropic emission in the rest frame of emission source, the emission angle $\theta^{\prime}$ of the considered particle has the probability density function:

[TABLE]

which is a half sine distribution in $[0,\pi]$, and the azimuth $\phi^{\prime}$ obeys the probability density function $f_{\phi^{\prime}}(\phi^{\prime})=1/(2\pi)$ which is an even distribution in $[0,2\pi]$ [41]. In the Monte Carlo method, $\theta^{\prime}$ satisfies

[TABLE]

which is the solution of $\int_{0}^{\theta^{\prime}}(1/2)\sin\theta^{\prime\prime}d\theta^{\prime\prime}=R_{2}$.

Considering $p^{\prime}$ and $\theta^{\prime}$ obtained from Eqs. (3) and (5), we have the transverse momentum $p^{\prime}_{T}$ to be

[TABLE]

the longitudinal momentum $p_{z}^{\prime}$ to be

[TABLE]

the energy $E^{\prime}$ to be

[TABLE]

and the rapidity $y^{\prime}$ to be

[TABLE]

In the center-of-mass reference frame or the laboratory reference frame, the rapidity of the considered emission source is assumed to be $y_{x}$ in the rapidity space. Then, the rapidity of the considered particle in the center-of-mass or laboratory reference frame is

[TABLE]

due to the additivity of rapidity. Multiple emission sources are assumed to distribute evenly in the rapidity range $[y_{\min},y_{\max}]$, where $y_{\min}$ and $y_{\max}$ are the minimum and maximum rapidity shifts of the multiple sources. In the Monte Carlo method,

[TABLE]

In particular, comparing with small mass particles, protons exhibit large effect of leading particles which are assumed to distribute evenly in the rapidity range $[y_{L\min},y_{L\max}]$, where $y_{L\min}$ and $y_{L\max}$ are the minimum and maximum rapidity shifts of the leading protons. We have

[TABLE]

The fraction of the non-leading (leading) protons in total protons is assumed to be $k$ ($1-k$). The effects of leading pions and kaons are small and can be neglected in this paper.

In the center-of-mass or laboratory reference frame, the transverse momentum $p_{T}$ is

[TABLE]

the longitudinal momentum $p_{z}$ is

[TABLE]

the momentum $p$ is

[TABLE]

and the emission angle $\theta$ is

[TABLE]

The whole calculation is performed by the Monte Carlo method, though only random numbers are used for the numerical calculation. To compare the theoretical model results with the experimental momentum spectra in a given $\theta$ range, we analyze the momentum distribution of particles which are in the given $\theta$ range. It should be noted that another experimental selection, i.e. the longitudinal position $z$ [32], is not regarded as the selected condition in the theoretical model work due to the fact that $z$ is only a reflection of target thickness in a 90-cm-long graphite target. From $z=0$ to $z=90$ cm, the beam momentum slightly decreases, which is neglected in this paper. In the calculation using random numbers, the energy-momentum conservation was demanded at each step. The results violating the energy-momentum conservation are not considered for our discussions.

It should be noticed that the Boltzmann distribution, Eq. (1), can be used to describe low momentum spectra in the source’s rest frame or low transverse momentum spectra after analytic derivation [41] or via the Monte Carlo method, Eqs. (3), (5), and (6). In the case of considering high momentum spectra in the source’s rest frame or high transverse momentum spectra, one may use possibly the multi-component Boltzmann distribution, Eq. (2). This paper treats multiple sources moving directly in a rapidity range, $[y_{\min},y_{\max}]$ or $[y_{L\min},y_{L\max}]$, which results in high momentum in laboratory reference frame. However, in the rest frame of each source, the total momentum and transverse momentum are small. As a consequence, Eq. (1) is valid in all momentum range, after the transformation from source’s rest frame to laboratory reference frame.

3 Results and discussion

Figures 1 and 2 present the momentum spectra, $(1/N_{pot})d^{2}n/dpd\theta$, of charged pions ($\pi^{+}$ and $\pi^{-}$) produced in $p$-C collisions at 31 GeV/$c$ in the laboratory reference frame respectively, where $N_{pot}$ denotes the number of protons on target and $n$ denotes the number of particles. Panels (a)–(c), (d)–(f), (g)–(i), (j)–(l), (m)–(o), and (p)–(q) represent the spectra for $z=0$–18, 18–36, 36–54, 54–72, 72–90, and 90 cm, respectively. For clarity, spectra in different $\theta$ ranges are scaled by adding different numbers (marked in the panels) are represented by different symbols, which are the experimental data measured by the NA61/SHINE Collaboration [32]. The curves are our results fitted by the multisource thermal model using to Eq. (1) and Monte Carlo method. The values of free parameters ($T$, $y_{\max}$ and $y_{\min}$), normalization constant ($N_{0}$), $\chi^{2}$, and number of degree of freedom (ndof) corresponding to the fits for the spectra of $\pi^{+}$ and $\pi^{-}$ are listed in Tables A1 and A2 in the appendix, respectively. In two cases, ndof in the fittings are negative which appear in the tables with “$-$” signs and the corresponding curves are for eye guiding only. One can see that the theoretical model results are approximately in agreement with the NA61/SHINE experimental data of $\pi^{+}$ and $\pi^{-}$.

Figure 3 presents the momentum spectra of (a)–(b) $\pi^{+}$ and (c)–(d) $\pi^{-}$ in (a)–(c) $\theta=20$–40 mrad and (b)–(d) $\theta=100$–140 mrad in six $z$ ranges with different scaled amounts shown in the panels. The symbols represent the experimental data [32]. The curves are our results fitted by the model. The values of $T$, $y_{\max}$, $y_{\min}$, $N_{0}$, $\chi^{2}$, and ndof corresponding to the fits for the spectra of $\pi^{+}$ and $\pi^{-}$ are listed in Table A3 in the appendix. One can see again that the theoretical model results are approximately in agreement with the experimental data of $\pi^{+}$ and $\pi^{-}$.

Similar to Figs. 1 and 2, Figs. 4 and 5 show the momentum spectra of positively and negatively charged kaons ($K^{+}$ and $K^{-}$) produced in $p$-C collisions at 31 GeV/$c$ respectively. Panels (a), (b), (c), (d), (e), and (f) represent the spectra for $z=0$–18, 18–36, 36–54, 54–72, 72–90, and 90 cm, respectively. The values of $T$, $y_{\max}$, $y_{\min}$, $N_{0}$, $\chi^{2}$, and ndof corresponding to the fits for the spectra of $K^{+}$ and $K^{-}$ are listed in Tables A4 and A5 respectively in the appendix. One can see that the theoretical model results are approximately in agreement with the experimental data of $K^{+}$ and $K^{-}$.

Similar to Fig. 1, Fig. 6 shows the momentum spectra of $p$ emitted in $p$-C collisions at 31 GeV/$c$. Panels (a)–(b), (c)–(d), (e)–(f), (g)–(h), (i)–(j), and (k)–(l) represent the spectra for $z=0$–18, 18–36, 36–54, 54–72, 72–90, and 90 cm, respectively. The values of $T$, $k$, $y_{\max}$, $y_{\min}$, $y_{L\max}$, $y_{L\min}$, $N_{0}$, $\chi^{2}$, and ndof corresponding to the fits for the spectra are listed in Table A6 in the appendix. In a few cases, ndof are negative which appear in the table in terms of “$-$” and the corresponding curves are just for eye guiding only. It should be noted that the contributions of leading protons have to be considered in the spectra. One can see that the theoretical model results are approximately in agreement with the experimental data.

We notice from Tables A1–A6 that different $T$ for a range of $z$ and its dependence with $\theta$ or $y$ are observed, but the development of the model in our previous work [42] concludes that $T$ is independent of $y$. We would like to explain here that this paper treats $T$ as differential function of $\theta$ or $y$, which is more detailed. While, our previous work treats $T$ as integral or mean quantity over $y$. As for which case should be used, it depends on experimental data.

We now analyze the dependences of free parameters on $\theta$ and $z$. Figures 7 and 8 show respectively the dependences of $T$ and $\Delta y$ ($=y_{\max}-y_{\min}$) on (a)–(e) $\theta$, which are extracted from the data samples within different $z$ ranges for $\pi^{+}$, $\pi^{-}$, $K^{+}$, $K^{-}$, and $p$ respectively, and on (f) $z$, which are extracted from the data samples within different $\theta$ ranges for $\pi^{+}$ and $\pi^{-}$, where we use $\Delta y$ to denote the difference between $y_{\max}$ and $y_{\min}$ to avoid trivialness in using both $y_{\max}$ and $y_{\min}$. In particular, in Fig. 8(e), the results with $\Delta y>1$ are mainly for leading protons and obtained by $y_{L\max}-y_{L\min}$. One can see that, for $\pi^{\pm}$ and $K^{\pm}$, $T$ and $\Delta y$ decrease slightly with the increase of $\theta$, and do not change obviously with the increase of $z$. The obtained $T$ ($\Delta y$) values for negative and positive pions or kaons seem to be very similar as we expect. The data for antiproton ($\overline{p}$) are not available in ref. [32], which forbids in making a comparison for $p$ and $\overline{p}$ in this paper. In fact, the situation for $p$ is more complex due to the effect of leading protons.

The dependences of $T$ and $\Delta y$ on $\theta$ for the productions of $\pi^{\pm}$ and $K^{\pm}$ can be explained by the effect of cascade collisions in the target and by the nuclear stopping of the target. The cascade collisions can cause larger $\theta$ and more energy loss and then lower $T$. The nuclear stopping can cause smaller $\Delta y$. Combining with cascade collisions and nuclear stopping, one can obtain low $T$ and small $\Delta y$ at large $\theta$ for the productions of $\pi^{\pm}$ and $K^{\pm}$. Because of the effect of leading particles, the situation for the emissions of $p$ is more complex, which shows different trends from those of $\pi^{\pm}$ and $K^{\pm}$. Meanwhile, the flow effect can cause larger $T$, which is related to more complex mechanism.

The dependences of $T$ and $\Delta y$ on $z$, which are extracted from the data samples within different $\theta$ ranges for (a) $\pi^{+}$, (b) $\pi^{-}$, (c) $K^{+}$, (d) $K^{-}$, and (e) $p$, are given in Figs. 9 and 10 respectively. In particular, large $\Delta y$ ($=y_{L\max}-y_{L\min}>1$) in Fig. 10(e) represent mainly the rapidity shifts of leading protons. In principle, there is no obvious increase or decrease in $T$ and $\Delta y$ with the increase of $z$, but some statistical fluctuations in few cases. This result is natural due to the fact that $z$ is not the main factor in a 90-cm-long graphite target. It is expected that $T$ and $\Delta y$ will decrease with the increase of $z$ in a very long graphite target in which the energy loss of the beam protons has to be considered. The NA61/SHINE experimental data analyzed in this paper are not obtained from a long graphite target and hence it is not necessary to consider the energy loss of the beam protons.

Figure 11 displays the dependences of fraction $k$ of non-leading protons on (a) $\theta$ and (b) $z$, which are extracted from the data samples within different $z$ and $\theta$ ranges, respectively. One can see that there is no obvious change in the dependence of $k$ on $\theta$, but some statistical fluctuations. There is a slight increase in the dependence of $k$ on $z$ with the increase of $z$, which can be explained by more energy loss of the beam protons at larger $z$. This energy loss is small in a not too large $z$ range, which does not affect obviously other free parameters such as $T$ and $\Delta y$ due to their less sensitivity at the energy in the $z$ range considered in this paper. It is natural that the larger (fewer) fraction $k$ ($1-k$) of protons appears as non-leading (leading) particles at lower energy or larger $z$. Indeed, the fraction is mainly determined by the collision energy, and the leading protons are considerable at the SPS. In fact, the leading protons are those existed in the projectile with high momentum and small emission angle, but not the produced protons. With the increase of collision energy up to dozens of GeV and above at which meson-dominated final states appear [43], $k$ will increase due to the increase of accompanied produced protons. With the decrease of collision energy down to several GeV and below at which baryon-dominated final states appear [43], $k$ will also increase due to the increase of target stopping which causes the decrease of leading protons.

Figures 12 and 13 show respectively the dependences of average $p_{T}$ ($\langle p_{T}\rangle$) and $T_{i}$ on (a)–(e) $\theta$, which are extracted from the data samples within different $z$ ranges for $\pi^{+}$, $\pi^{-}$, $K^{+}$, $K^{-}$, and $p$ respectively, and on (f) $z$, which are extracted from the data samples within different $\theta$ ranges for $\pi^{+}$ and $\pi^{-}$, where $T_{i}$ denotes the initial quasi-temperature which is given by the root-mean-square $p_{T}$ ($\sqrt{\langle p_{T}^{2}\rangle}$) over $\sqrt{2}$ ($\sqrt{\langle p_{T}^{2}\rangle/2}$) according to the color string percolation model [44, 45, 46]. It should be noted that $\sqrt{\langle p_{T}^{2}\rangle/2}$ in Refs.  [44, 45, 46] is regarded as the initial temperature. In that model there are free parameters associated to the medium created in a high energy collision, which is not the case for this paper at low energy. So we call $\sqrt{\langle p_{T}^{2}\rangle/2}$ the initial quasi-temperature in this paper. The dependences of $\langle p_{T}\rangle$ and $T_{i}$ on $z$ are presented in Figs. 14 and 15 respectively, which are extracted from the data samples within different $\theta$ ranges. One can see that, for pions and kaons, there are increases in $\langle p_{T}\rangle$ and $T_{i}$ when $\theta$ increases. The situation is complex for protons due to the effect of leading protons which have high momenta and result in high $\langle p_{T}\rangle$ and $T_{i}$ at small $\theta$. The produced protons which are non-leading should have similar trend in $\langle p_{T}\rangle$ and $T_{i}$ as those for pions and kaons. As a combination, the final protons are the sum of leading and produced protons. There is no obvious change in $\langle p_{T}\rangle$ and $T_{i}$ when $z$ increases due to not too large energy loss in a 90-cm-long graphite target.

We would like to point out that there are different definitions [47] for leading particles in experiments. There are at least four production mechanisms [48, 49] for leading protons in electron induced deep-inelastic scattering on proton. Among these mechanisms, at HERA energy, diffractive deep-inelastic scattering [50, 51] in which 72% of leading protons have momentum being larger than 0.9$p_{Lab}$ occupy about 26% [48] of leading protons, which are not enough to cover all leading protons. In particular, for leading protons with momenta being (0.5–0.98)$p_{Lab}$, a large fraction (77%) comes from non-diffractive deep-inelastic scatterings. In proton-proton and proton-nucleus collisions at the considered energy of this paper, the fraction of diffractive process is about 20% [52] in inelastic events, which is only a half of the fraction of leading protons. Even in nucleus-nucleus collisions, the effect of leading protons in forward rapidity region is also obvious [42, 53, 54, 55], which also reflects in high momentum region and is not only from diffractive process.

Naturally, there are other additional arguments to explain the behavior of Figs. 12 and 13 for the proton case. In fact, there are multiple or cascade secondary scatterings among produced particles and target nucleons. As low mass particles, the emission angles of pions and kaons increase obviously after multiple scatterings. This results in large $\langle p_{T}\rangle$ and $T_{i}$ due to large $\theta$ for pions and kaons. Contrary to this, the emission angles of protons increase in smaller amount after multiple scatterings due to higher mass of protons compared to pions and kaons. This results in small $\langle p_{T}\rangle$ and $T_{i}$ due to small $\theta$ for protons. However, non-negligible leading protons which have high momenta and smaller angles do not experience much multiple scatterings, which renders large $\langle p_{T}\rangle$ and $T_{i}$ at small $\theta$. As a competitive result, protons present different case from pions and kaons.

One can see naturally the coincident trend for $\langle p_{T}\rangle$ and $T_{i}$ in different $\theta$ and $z$ ranges. Due to the flow effect not being excluded, the trend of $T$ is inconsistent with that of $T_{i}$. As an all-around result, the effects of transverse and longitudinal flows are complex. The flow effect can obviously affect $T$, which is model dependent. The flow effect also affects $\langle p_{T}\rangle$ and $T_{i}$ which are also model dependent. Therefore, we mention here that $T$ is not a “real” temperature, but the effective temperature. In our opinion, the temperature and flow velocity should be independent of models, which is usually not the case more often, as some formalisms are used to extract the radial flow and the real/thermal temperature, which estimate the real temperature of the system being dependent of models.

The experimental data cannot be clearly distinguished into two parts: One part is the contribution of thermal motion, which reflects the “real” temperature at the kinetic freeze-out. The other part is the contribution of the collective flow. The current blast-wave model [34, 35] treats the thermal motion and flow effect by using the kinetic freeze-out temperature and transverse flow velocity, respectively. After fitting the spectra with ${\rm ndof}>1$ and using $p_{T}$ coverage as widely as possible ($p_{T}=0$–3 GeV/$c$), our study using the blast-wave model with flow profile parameter being 2 can obtain similar fit results as the curves in Figs. 1–6. To protrude the fit results of thermal model, the fit results of blast-wave model are not displayed in these figures. The relation between $T_{0}$ and $\beta_{T}$ for different cases from the spectra of positive particles are plotted in Fig. 16, where the circles, squares, and triangles represent the results from $\pi^{+}$, $K^{+}$, and $p$ spectra, respectively. One can see considerable flow-like effect in $p$-C collisions at 31 GeV/$c$, which shows a positive correlation between $T_{0}$ and $\beta_{T}$. The kinetic freeze-out temperature $T_{0}$ is about from 0.080 to 0.135 GeV. The corresponding transverse flow velocity $\beta_{T}$ is about from $0.21$ to $0.42c$. Massive particles such as $p$ correspond to larger $T_{0}$ and smaller $\beta_{T}$ comparing to $\pi^{+}$ at the same or similar $\theta$, which is in agreement with hydrodynamic type behavior. The flow-like effect observed in this work is slightly less than the flow velocity ($0.3c$ in peripheral and $0.5c$ in central gold-gold collisions) obtained from the yield ratio of $p/\pi$ in a simple afterburner model [56]. The difference is due to the fact that lower energy small system with minimum-bias sample is studied in this paper. In some cases, the results on kinetic freeze-out temperature or transverse flow velocity obtained from different models are not always harmonious [36, 37].

It should be noted that there is entanglement in determining $T_{0}$ and $\beta_{T}$. For a give $p_{T}$ spectrum, $T_{0}$ and $\beta_{T}$ are negatively correlated, which means an increase in $T$ should result in a decrease of $\beta_{T}$. But for a set of $p_{T}$ spectra, after determining $T_{0}$ and $\beta_{T}$ for each $p_{T}$ spectrum, the correlation between $T_{0}$ and $\beta_{T}$ is possibly positive or negative, which depends on the choices of flow profile function and $p_{T}$ coverage. If the correlation is negative, one may increase $T_{0}$ and decrease $\beta_{T}$ by changing the flow profile function and $p_{T}$ coverage, and obtain possibly positive correlation. If the correlation is positive, one may decrease $T_{0}$ and increase $\beta_{T}$ by changing the flow profile function and $p_{T}$ coverage, and obtain possibly negative correlation. Unlike experimental papers, where one finds a single $T_{0}$ and a common $\beta_{T}$ by fitting the blast-wave model to the bulk part of the $p_{T}$ spectra (in a very narrow coverage which is particle dependent and much less than 3 GeV/$c$) by performing a simultaneous fitting to the identified particle spectra using a changeable $n_{0}$ (from 0 to 4.3) [57], here we have considered a differential freeze-out scenario and have restricted uniformly the fitting up to 3 GeV/$c$ for different particles and have used always $n_{0}=2$. The value of $T_{0}$ ($\beta_{T}$) in positive correlation is larger (less) than that in negative correlation. Positive correlation means high excitation and quick expansion, while negative correlation means longer lifetime (lower excitation) and quicker expansion. In our opinion, although both positive and negative correlations are available, one needs other method to check which one is suitable. In fact, positive correlation in Fig. 16 is in agreement with the alternative method used in our previous works [36, 37].

We would rather like to use $\langle p_{T}\rangle$ directly in the determination of kinetic freeze-out temperature and transverse flow velocity. For example, the contribution of one participant in each binary collision in the Erlang distribution is $\langle p_{T}\rangle/2$ which is regarded as effective temperature [58] contributed by the thermal motion and flow effect. We could assume the contribution fraction of the thermal motion to be $k_{0}$. Then, the kinetic freeze-out temperature is $k_{0}\langle p_{T}\rangle/2$, and the transverse flow velocity is $(1-k_{0})\langle p_{T}\rangle/2m_{0}\overline{\gamma}$, where $\overline{\gamma}$ is the mean Lorentz factor of the considered particles in the rest frame of emission source. If we take $k_{0}\approx 0.3$ and at large $\theta$, the obtained kinetic freeze-out temperature (0.05 GeV for pion emission and 0.10 GeV for proton emission) are in agreement with those from the blast-wave model [34, 35], and transverse flow velocity ($0.2c$ for pion emission and $0.1c$ for proton emission) are qualitatively in agreement with those from the blast-wave model [34, 35] and the afterburner model [50]. The treatment of $\langle p_{T}\rangle/2$ is also model dependent and in agreement with hydrodynamic type behavior. In addition, larger $\langle p_{T}\rangle/2$ results in larger $T_{0}$ and $\beta_{T}$, which shows positive correlation between $T_{0}$ and $\beta_{T}$. The positive correlation in Fig. 16 is also in agreement with the treatment of $\langle p_{T}\rangle/2$.

Before the summary and conclusions, we would like to point out that the kinetic freeze-out temperature and transverse flow velocity obtained in this paper are mass dependent, which renders a scenario for multiple kinetic freeze-out (differential freeze-out) [59]. The afterburner model [56] uses a mass independent flow velocity, which renders a scenario for single kinetic freeze-out. There are arguments on the kinetic freeze-out scenario, which is beyond the focus of this paper, so we shall not discuss it anymore. In addition, it should be noted that in the absence of required number of experimental data points, the fittings using the current model in few cases yield negative $\chi^{2}$/ndof, making the description unphysical, though the corresponding curves could be used as eye guiding only.

4 Summary and conclusions

We summarize here our main observations and conclusions.

(a) The momentum spectra of $\pi^{+}$, $\pi^{-}$, $K^{+}$, $K^{-}$, and $p$ produced in $p$-C collisions at 31 GeV/$c$ are analyzed in the framework of multisource thermal model by using the Boltzmann distribution and Monte Carlo method. The results are approximately in agreement with the experimental data in various emission angle, $\theta$, ranges and longitudinal positions, $z$, measured by the NA61/SHINE Collaboration at the SPS.

(b) The effective temperature $T$ and rapidity shifts $\Delta y$ from the spectra under given experimental conditions which limit various $\theta$ and $z$ ranges are obtained. For $\pi^{\pm}$ and $K^{\pm}$, $T$ and $\Delta y$ decrease slightly with the increase of $\theta$, and do not change obviously with the increase of $z$. The situation for $p$ is more complex due to the effect of leading protons. There is no obvious change in $T$ and $\Delta y$ when $z$ increases due to not too large energy loss in a not too long graphite target. Both $T$ and $\Delta y$ depend on models. In particular, $T$ contains the contribution of flow effect, which is not ideal to describe the excitation degree of emission source.

(c) The fraction $k$ ($1-k$) of non-leading (leading) protons in total protons from the spectra in various $\theta$ and $z$ ranges are obtained. There is no obvious change in the dependence of $k$ ($1-k$) on $\theta$, but some statistical fluctuations. There is a slight increase (decrease) in the dependence of $k$ ($1-k$) on $z$ with the increase of $z$ due to more energy loss of the beam protons in the target at larger $z$. The effect of leading protons cannot be neglected at the SPS energies. It is expected that $k$ ($1-k$) will be larger (smaller) at both lower ($\leq$ several GeV) and higher energies ($\geq$ dozens of GeV).

(d) The average transverse momentum $\langle p_{T}\rangle$ and initial quasi-temperature $T_{i}$ from the spectra in various $\theta$ and $z$ ranges are obtained. For $\pi^{\pm}$ and $K^{\pm}$, there are increases in $\langle p_{T}\rangle$ and $T_{i}$ when $\theta$ increases. The situation for $p$ is complex due to the effect of leading protons. There is no obvious change in $\langle p_{T}\rangle$ and $T_{i}$ when $z$ increases due to not too large energy loss in a not too long graphite target. Both $\langle p_{T}\rangle$ and $T_{i}$ are model dependent due to the fact that they are obtained from the model which fits the data.

(e) The behaviors of effective temperature, rapidity shifts, fraction of non-leading (leading) protons, average transverse momentum, and initial quasi-temperature obtained from the fits of multisource thermal model to the NA61/SHINE data can be explained in terms of cascade collisions in the target, stopping power of the target, energy loss of the beam protons in the target, and so on. This paper provides a new evidence for the effectiveness of the multisource thermal model, though there is no connection with a possible formation of a Quark-Gluon Plasma due to small system being considered.

Data Availability

The data used to support the findings of this study are included within the article and are cited at relevant places within the text as references.

Compliance with Ethical Standards

The authors declare that they are in compliance with ethical standards regarding the content of this paper.

Conflict of Interest

The authors declare that there are no conflicts of interest regarding the publication of this paper.

Acknowledgments

Communications from Debasish Das are highly acknowledged. Authors P.P.Y., M.Y.D., and F.H.L. acknowledge the financial supports from the National Natural Science Foundation of China under Grant Nos. 11575103 and 11847311, the Shanxi Provincial Innovative Foundation for Graduate Education Grant No. 2019SY053, the Scientific and Technological Innovation Programs of Higher Education Institutions in Shanxi (STIP) under Grant No. 201802017, the Shanxi Provincial Natural Science Foundation under Grant No. 201701D121005, and the Fund for Shanxi “1331 Project” Key Subjects Construction. Author R.S. acknowledges the financial supports from ALICE Project No. SR/MF/PS-01/2014-IITI(G) of Department of Science & Technology, Government of India. The funding agencies have no role in the design of the study; in the collection, analysis, or interpretation of the data; in the writing of the manuscript, or in the decision to publish the results.