Probing anomalous gauge-Higgs couplings using $Z$ boson polarization at $e^+ e^-$ colliders

TL;DR

This paper investigates how the polarization of the Z boson in the Higgsstrahlung process at future electron-positron colliders can be used to detect and constrain anomalous gauge-Higgs couplings, providing a new method to probe physics beyond the Standard Model.

Contribution

It introduces a novel approach using Z boson polarization and angular asymmetries to constrain anomalous $ZZH$ couplings at future colliders.

Findings

Potential to significantly constrain anomalous couplings at 250 GeV and 500 GeV.

Angular asymmetries effectively relate to Z polarization observables.

Method applicable with various beam polarization configurations.

Abstract

We study possible new physics interactions in the $ZZH$ vertex contributing to the Higgsstrahlung process $e^+ e^- \to ZH$ at proposed future $e^+e^-$ colliders using the polarization of the $Z$ as a probe. We calculate the spin density matrix of the $Z$ for the process and determine the eight independent polarization parameters of the $Z$ boson which have the potential to constrain the anomalous couplings. We study angular asymmetries using the decay leptons from the $Z$ boson which are simply related to the polarization observables. We also estimate the limits that can be placed on the anomalous couplings using measurements of these angular asymmetries at centre of mass energies of 250 GeV and 500 GeV and various combinations of polarized $e^+$ and $e^-$ beams.

Tables

Table 1. Table 1 : Production spin density matrix elements (in fb) of Z 𝑍 Z for the SM and the coefficients of various couplings in each matrix element for unpolarized beams at s = 250 ​  GeV 𝑠 250  GeV \sqrt{s}=250\text{~{}GeV} .

	SM	$\text{Re}{b}_z$	$\text{Im}{b}_z$	$\text{Re}{\tilde{b}}_z$	$\text{Im}{\tilde{b}}_z$
$\sigma (\pm ,\pm )$	$70.32$	$-466.72$	$0$	$0$	$\pm 262.99$
$\sigma (0,0)$	$103.03$	$-466.72$	$0$	$0$	$0$
$\sigma (\pm ,\mp )$	$35.16$	$-233.36$	$0$	$\mp i131.49$	$0$
$\sigma (\pm ,0)$	$10.60$	$-59.21$	$-i11.17$	$\mp i19.83$	$\pm 19.83$
$\sigma (0,\pm )$	$10.60$	$-59.21$	$+i11.17$	$\pm i19.83$	$\pm 19.83$

Table 2. Table 2 : Production spin density matrix elements (in fb) of Z 𝑍 Z for the SM and the coefficients of various couplings in each matrix element for ( P L = − 0.8 , P ¯ L = 0.3 formulae-sequence subscript 𝑃 𝐿 0.8 subscript ¯ 𝑃 𝐿 0.3 P_{L}=-0.8,\bar{P}_{L}=0.3 ) at s = 250 ​  GeV 𝑠 250  GeV \sqrt{s}=250\text{~{}GeV} .

	SM	$\text{Re}{b}_z$	$\text{Im}{b}_z$	$\text{Re}{\tilde{b}}_z$	$\text{Im}{\tilde{b}}_z$
$\sigma (\pm ,\pm )$	$98.76$	$-655.52$	$0$	$0$	$\pm 369.38$
$\sigma (0,0)$	$144.71$	$-655.52$	$0$	$0$	$0$
$\sigma (\pm ,\mp )$	$49.38$	$-327.76$	$0$	$\mp i184.69$	$0$
$\sigma (\pm ,0)$	$91.15$	$-508.93$	$-i96.05$	$\mp i170.45$	$\pm 170.45$
$\sigma (0,\pm )$	$91.15$	$-508.93$	$+i96.05$	$\pm i170.45$	$\pm 170.45$

Table 3. Table 3 : Production spin density matrix elements (in fb) of Z 𝑍 Z for the SM and the coefficients of various couplings in each matrix element for unpolarized beams at s = 500 ​  GeV 𝑠 500  GeV \sqrt{s}=500\text{~{}GeV} .

	SM	$\text{Re}{b}_z$	$\text{Im}{b}_z$	$\text{Re}{\tilde{b}}_z$	$\text{Im}{\tilde{b}}_z$
$\sigma (\pm ,\pm )$	$6.39$	$-186.51$	$0$	$0$	$\pm 172.85$
$\sigma (0,0)$	$45.26$	$-186.51$	$0$	$0$	$0$
$\sigma (\pm ,\mp )$	$3.19$	$-93.26$	$0$	$\mp i86.42$	$0$
$\sigma (\pm ,0)$	$2.12$	$-35.29$	$-i26.56$	$\mp i28.66$	$\pm 28.66$
$\sigma (0,\pm )$	$2.12$	$-35.29$	$+i26.56$	$\pm i28.66$	$\pm 28.66$

Table 4. Table 4 : Production spin density matrix elements (in fb) of Z 𝑍 Z for the SM and the coefficients of various couplings in each matrix element for ( P L = − 0.8 , P ¯ L = 0.3 formulae-sequence subscript 𝑃 𝐿 0.8 subscript ¯ 𝑃 𝐿 0.3 P_{L}=-0.8,\bar{P}_{L}=0.3 ) at s = 500 ​  GeV 𝑠 500  GeV \sqrt{s}=500\text{~{}GeV} .

	SM	$\text{Re}{b}_z$	$\text{Im}{b}_z$	$\text{Re}{\tilde{b}}_z$	$\text{Im}{\tilde{b}}_z$
$\sigma (\pm ,\pm )$	$8.98$	$-261.96$	$0$	$0$	$\pm 369.38$
$\sigma (0,0)$	$63.57$	$-261.96$	$0$	$0$	$0$
$\sigma (\pm ,\mp )$	$4.49$	$-130.98$	$0$	$\mp i121.38$	$0$
$\sigma (\pm ,0)$	$18.21$	$-303.29$	$-i228.25$	$\mp i246.3$	$\pm 246.3$
$\sigma (0,\pm )$	$18.21$	$-303.29$	$+i228.25$	$\pm i246.3$	$\pm 246.3$

Table 5. Table 5 : The total production cross section (in fb) of Z 𝑍 Z and the non-zero angular asymmetries in the SM for unpolarized and polarized beams at s = 250 ​  GeV 𝑠 250  GeV \sqrt{s}=250\text{~{}GeV} .

Observable	$P_L=0{\overline{P}}_L=0$	$P_L=-0.8{\overline{P}}_L=0.3$
$\sigma$ (in fb)	$243.67$	$342.24$
$A_x$	$-0.014$	$-0.085$
$A_{x^2-y^2}$	$0.092$	$0.092$
$A_{zz}$	$-0.05$	$-0.05$

Table 6. Table 6 : The total production cross section (in fb) of Z 𝑍 Z and the non-zero angular asymmetries in the SM for unpolarized and polarized beams at s = 500 ​  GeV 𝑠 500  GeV \sqrt{s}=500\text{~{}GeV} .

Observable	$P_L=0{\overline{P}}_L=0$	$P_L=-0.8\overline{P_L}=0.3$
$\sigma$ (in fb)	$58.04$	$81.56$
$A_x$	$-0.012$	$-0.071$
$A_{x^2-y^2}$	$0.035$	$0.035$
$A_{zz}$	$-0.251$	$-0.251$

Table 7. Table 7 : Anomalous contribution to cross section (in fb) and angular asymmetries for unpolarized and polarized beams at s = 250 ​  GeV 𝑠 250  GeV \sqrt{s}=250\text{~{}GeV} for unit values of the relevant couplings.

Observable	Coupling	$P_L=0{\overline{P}}_L=0$	$P_L=-0.8{\overline{P}}_L=0.3$
$\sigma$ (in fb)	$\text{Re}{b}_z$	$-1400.17$	$-1966.55$
$A_x$	$\text{Re}{b}_z$	$-0.0022$	$-0.014$
$A_y$	$\text{Re}{\tilde{b}}_z$	$-0.026$	$-0.158$
$A_z$	$\text{Im}{\tilde{b}}_z$	$-0.242$	$-0.242$
$A_{xy}$	$\text{Re}{\tilde{b}}_z$	$+0.344$	$+0.344$
$A_{yz}$	$\text{Im}{b}_z$	$+0.041$	$+0.253$
$A_{xz}$	$\text{Im}{\tilde{b}}_z$	$-0.073$	$-0.448$
$A_{x^2-y^2}$	$\text{Re}{b}_z$	$-0.082$	$-0.082$
$A_{zz}$	$\text{Re}{b}_z$	$-0.289$	$-0.289$

Table 8. Table 8 : Anomalous contribution to cross section (in fb) and angular asymmetries for unpolarized and polarized beams at s = 500 ​  GeV 𝑠 500  GeV \sqrt{s}=500\text{~{}GeV} for unit values of the relevant couplings.

Observable	Coupling	$P_L=0{\overline{P}}_L=0$	$P_L=-0.8{\overline{P}}_L=0.3$
$\sigma$ (in fb)	$\text{Re}{b}_z$	$-559.5$	$-785.88$
$A_x$	$\text{Re}{b}_z$	$+0.081$	$+0.497$
$A_y$	$\text{Re}{\tilde{b}}_z$	$-0.157$	$-0.958$
$A_z$	$\text{Im}{\tilde{b}}_z$	$-0.668$	$-0.668$
$A_{xy}$	$\text{Re}{\tilde{b}}_z$	$+0.948$	$+0.948$
$A_{yz}$	$\text{Im}{b}_z$	$+0.412$	$+2.521$
$A_{xz}$	$\text{Im}{\tilde{b}}_z$	$-0.444$	$-2.720$
$A_{x^2-y^2}$	$\text{Re}{b}_z$	$-0.685$	$-0.685$
$A_{zz}$	$\text{Re}{b}_z$	$-2.421$	$-2.421$

Table 9. Table 9 : 1 ​ σ 1 𝜎 1\sigma limit obtained from various leptonic asymmetries for unpolarized and polarized beams at s = 250 ​  GeV 𝑠 250  GeV \sqrt{s}=250\text{~{}GeV} .

		Limit ($\times {10}^{-3}$) for
Observable	Coupling	$P_L=0$	$P_L=-0.8$
		${\overline{P}}_L=0$	${\overline{P}}_L=0.3$
$\sigma$	$\text{Re}{b}_z$	$1.36$	$1.15$
$A_x$	$\text{Re}{b}_z$	$3480$	$478$
$A_y$	$\text{Re}{\tilde{b}}_z$	$303$	$41.7$
$A_z$	$\text{Im}{\tilde{b}}_z$	$32.3$	$27.2$
$A_{xy}$	$\text{Re}{\tilde{b}}_z$	$22.7$	$19.2$
$A_{yz}$	$\text{Im}{b}_z$	$189$	$26.1$
$A_{xz}$	$\text{Im}{\tilde{b}}_z$	$107$	$14.7$
$A_{x^2-y^2}$	$\text{Re}{b}_z$	$94.5$	$80.2$
$A_{zz}$	$\text{Re}{b}_z$	$26.8$	$22.8$

Table 10. Table 10 : 1 ​ σ 1 𝜎 1\sigma limit obtained from various leptonic asymmetries for unpolarized and polarized beams at s = 500 ​  GeV 𝑠 500  GeV \sqrt{s}=500\text{~{}GeV} .

		Limit ($\times {10}^{-3}$) for
Observable	Coupling	$P_L=0$	$P_L=-0.8$
		${\overline{P}}_L=0$	${\overline{P}}_L=0.3$
$\sigma$	$\text{Re}{b}_z$	$3.32$	$2.8$
$A_x$	$\text{Re}{b}_z$	$394$	$54.2$
$A_y$	$\text{Re}{\tilde{b}}_z$	$204$	$28.2$
$A_z$	$\text{Im}{\tilde{b}}_z$	$47.9$	$40.4$
$A_{xy}$	$\text{Re}{\tilde{b}}_z$	$33.7$	$28.5$
$A_{yz}$	$\text{Im}{b}_z$	$77.7$	$10.7$
$A_{xz}$	$\text{Im}{\tilde{b}}_z$	$72.0$	$9.93$
$A_{x^2-y^2}$	$\text{Re}{b}_z$	$46.7$	$39.4$
$A_{zz}$	$\text{Re}{b}_z$	$12.8$	$10.8$

Equations

$${\Gamma }_{\mu \nu }^V=\frac{g}{\cos {\theta }_W}{m}_Z\left[a_Z{g}_{\mu \nu }+\frac{b_Z}{m_Z^2}\left(k_{1\nu }{k}_{2\mu }-g_{\mu \nu }{k}_1.k_2\right)+\frac{{\tilde{b}}_Z}{m_Z^2}{ϵ}_{\mu \nu \alpha \beta }{k}_1^{\alpha }{k}_2^{\beta }\right]$$

$$e^{-}(p_1)+e^{+}(p_2)\to Z^{\alpha }(p)+H(k)$$

$${ϵ}^{\mu }(p,\pm )=\frac{1}{\sqrt{2}}(0,\mp \cos \theta ,-i,\pm \sin \theta ),$$

$${ϵ}^{\mu }(p,0)=\frac{1}{m_Z}(|{\vec{p}}_Z|,E_Z\sin \theta ,0,E_Z\cos \theta ),$$

$$M(-,+,+)$$

$$M(-,+,-)$$

$$M(-,+,0)$$

$$M(+,-,+)$$

$$M(+,-,-)$$

$$M(+,-,0)$$

$$\rho (i,j)={\overline{\sum }}_{\lambda ,{\lambda }^{{}^{\prime }}}M(\lambda ,{\lambda }^{{}^{\prime }},i)M^{\ast }(\lambda ,{\lambda }^{{}^{\prime }},j)$$

$$\rho (\pm ,\pm )$$

$$\rho (0,0)$$

$$\rho (\pm ,\mp )$$

$$\rho (\pm ,0)$$

$$\sigma (\pm ,\pm )$$

$$\sigma (0,0)$$

$$\sigma (\pm ,\mp )$$

$$\sigma (\pm ,0)$$

$$\sigma(i,j)\equiv\sigma\;\left(\begin{array}[]{ccc}\frac{1}{3}+\frac{P_{z}}{2}+\frac{T_{zz}}{\sqrt{6}}&\frac{P_{x}-iP_{y}}{2\sqrt{2}}+\frac{T_{xz}-iT_{yz}}{\sqrt{3}}&\frac{T_{xx}-T_{yy}-2iT_{xy}}{\sqrt{6}}\\ \frac{P_{x}+iP_{y}}{2\sqrt{2}}+\frac{T_{xz}+iT_{yz}}{\sqrt{3}}&\frac{1}{3}-\frac{2T_{zz}}{\sqrt{6}}&\frac{P_{x}-iP_{y}}{2\sqrt{2}}-\frac{T_{xz}-iT_{yz}}{\sqrt{3}}\\ \frac{T_{xx}-T_{yy}+2iT_{xy}}{\sqrt{6}}&\frac{P_{x}+iP_{y}}{2\sqrt{2}}-\frac{T_{xz}+iT_{yz}}{\sqrt{3}}&\frac{1}{3}-\frac{P_{z}}{2}+\frac{T_{zz}}{\sqrt{6}}\end{array}\right)$$

$$\sigma =\sigma (+,+)+\sigma (-,-)+\sigma (0,0).$$

$$P_x$$

$$P_y$$

$$P_z$$

$$T_{xy}$$

$$T_{xz}$$

$$T_{yz}$$

$$T_{xx}-T_{yy}$$

$$T_{zz}$$

$$A_x=\frac{3\alpha P_x}{4}\equiv \frac{\sigma (\cos {\varphi }^{\ast }>0)-\sigma (\cos {\varphi }^{\ast }<0)}{\sigma (\cos {\varphi }^{\ast }>0)+\sigma (\cos {\varphi }^{\ast }<0)}$$

$$A_y=\frac{3\alpha P_y}{4}\equiv \frac{\sigma (\sin {\varphi }^{\ast }>0)-\sigma (\sin {\varphi }^{\ast }<0)}{\sigma (\sin {\varphi }^{\ast }>0)+\sigma (\sin {\varphi }^{\ast }<0)}$$

$$A_z=\frac{3\alpha P_z}{4}\equiv \frac{\sigma (\cos {\theta }^{\ast }>0)-\sigma (\cos {\theta }^{\ast }<0)}{\sigma (\cos {\theta }^{\ast }>0)+\sigma (\cos {\theta }^{\ast }<0)}$$

$$A_{xy}=\frac{2}{\pi }\sqrt{\frac{2}{3}}{T}_{xy}\equiv \frac{\sigma (\sin 2{\varphi }^{\ast }>0)-\sigma (\sin 2{\varphi }^{\ast }<0)}{\sigma (\sin 2{\varphi }^{\ast }>0)+\sigma (\sin 2{\varphi }^{\ast }<0)}$$

$$A_{xz}=\frac{-2}{\pi }\sqrt{\frac{2}{3}}{T}_{xz}\equiv \frac{\sigma (\cos {\theta }^{\ast }\cos {\varphi }^{\ast }<0)-\sigma (\cos {\theta }^{\ast }\cos {\varphi }^{\ast }>0)}{\sigma (\cos {\theta }^{\ast }\cos {\varphi }^{\ast }>0)+\sigma (\cos {\theta }^{\ast }\cos {\varphi }^{\ast }<0)}$$

$$A_{yz}=\frac{2}{\pi }\sqrt{\frac{2}{3}}{T}_{yz}\equiv \frac{\sigma (\cos {\theta }^{\ast }\sin {\varphi }^{\ast }>0)-\sigma (\cos {\theta }^{\ast }\sin {\varphi }^{\ast }<0)}{\sigma (\cos {\theta }^{\ast }\sin {\varphi }^{\ast }>0)+\sigma (\cos {\theta }^{\ast }\sin {\varphi }^{\ast }<0)}$$

$$A_{x^2-y^2}=\frac{1}{\pi }\sqrt{\frac{2}{3}}(T_{xx}-T_{yy})\equiv \frac{\sigma (\cos 2{\varphi }^{\ast }>0)-\sigma (\cos 2{\varphi }^{\ast }<0)}{\sigma (\cos 2{\varphi }^{\ast }>0)+\sigma (\cos 2{\varphi }^{\ast }<0)}$$

$$A_{zz}=\frac{3}{8}\sqrt{\frac{3}{2}}{T}_{zz}\equiv \frac{\sigma (\sin 3{\theta }^{\ast }>0)-\sigma (\sin 3{\theta }^{\ast }<0)}{\sigma ((\sin 3{\theta }^{\ast }>0)+\sigma ((\sin 3{\theta }^{\ast }<0)}$$

$$\alpha =\frac{R_{\ell }^2-L_{\ell }^2}{R_{\ell }^2+L_{\ell }^2}=-\frac{2c_V{c}_A}{c_V^2+c_A^2}$$

$$C_{\mathrm{limit}}=\frac{\sqrt{1-A_{SM}^2}}{|A-A_{SM}|}\frac{1}{\sqrt{{\sigma }_{SM}\mathcal{L}}}$$

Full text

Probing anomalous gauge-Higgs couplings using $Z$ boson polarization at $e^{+}e^{-}$ colliders

Kumar Raoa, Saurabh D. Rindanib and Priyanka Sarmaha

*a**Physics Department, Indian Institute of Technology Bombay,

Powai, Mumbai 400076, India

bTheoretical Physics Division, Physical Research Laboratory,

Navrangpura, Ahmedabad 380009, India*

Abstract

We study possible new physics interactions in the $ZZH$ vertex contributing to the Higgsstrahlung process $e^{+}e^{-}\to ZH$ at proposed future $e^{+}e^{-}$ colliders using the polarization of the $Z$ as a probe. We calculate the spin density matrix of the $Z$ for the process and determine the eight independent polarization parameters of the $Z$ boson which have the potential to constrain the anomalous couplings. We study angular asymmetries using the decay leptons from the $Z$ boson which are simply related to the polarization observables. We also estimate the limits that can be placed on the anomalous couplings using measurements of these angular asymmetries at centre of mass energies of 250 GeV and 500 GeV and various combinations of polarized $e^{+}$ and $e^{-}$ beams.

1 Introduction

The discovery of the Higgs boson ($H$) with mass around 125 GeV at the Large Hadron Collider (LHC) completes the particle spectrum of the Standard Model (SM). However, to confirm that this is indeed the Higgs boson of the SM and uncover the exact mechanism of the breaking of the electroweak symmetry will require precise measurements of the couplings of the Higgs to electroweak gauge bosons ($V=W^{\pm},Z,\gamma$), its Yukawa couplings to the fermions as well as its self couplings. The $VVH$ coupling is of particular importance whose form is fixed by the $SU(2)_{L}\times U(1)_{Y}$ gauge structure of the SM.

Although the present accuracy of experiments at the LHC seems to indicate that the couplings of the Higgs boson are in broad agreement with the SM predictions, given their importance in confirming the symmetry breaking mechanism in the SM, one could be optimistic that future experiments with higher luminosities will either be able to constrain such couplings even further or indicate small deviations from SM predictions. To do that one would need not just the cross section, but more observables. A fit to the differential cross section would be highly demanding requiring large statistics. However, use can be made of expectation values of kinematic variables, or their asymmetries.

A number of scenarios going beyond the SM predict new particles and interactions at the TeV scale and require an enhanced Higgs sector resulting in modified couplings of the Higgs boson to SM particles. Various studies have been carried out on the $VVH$ coupling, at planned $e^{+}e^{-}$ colliders and the LHC, using a most general tensorial form of the coupling and using a variety of observables involving kinematic distributions of the $Z$ and the charged leptons from $Z$ decay, see for example, [1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16, 17]. Anomalous interactions in the $HVV$ vertex have been searched for by the CMS collaboration [19, 18] and although the current data are consistent with the SM predictions, the constraints are still weak (some details follow later) to allow for beyond the SM contributions to the vertex.

An interesting variable which has received attention in recent years is the polarization of the $Z$ boson produced in association with the Higgs. In this work, we study the $ZZH$ coupling using the associated production of the $Z$ with the Higgs at proposed future $e^{+}e^{-}$ colliders. To measure polarization, one needs to look at kinematic distributions of some decay products. In this work we adopt the formalism where we construct appropriate asymmetries from the angular distribution of the decay products of the $Z$, which in turn are related to its polarization parameters [20, 21]. Measurement of these polarization parameters will give insight into the production mechanism and also provide information about the nature of the tensorial structure as well as the strength of anomalous couplings in the $ZZH$ interaction. Such measurements can be used to place stringent limits on the anomalous couplings in the absence of any deviation from the SM prediction.

$Z$ polarization has been studied in the context of new physics at the LHC [20, 22]. Refs. [23, 24] studied anomalous coupling in $ZZ$/$Z\gamma$ production at an $e^{-}e^{+}$ collider. Ref. [8] studied various general $ZZH$ and $Z\gamma H$ couplings using a different set of observables. Analogously, polarization of the $W$ boson produced in association with the Higgs at the LHC has been studied in [25, 22].

In this paper, we are addressing the question how well the form factors for the $ZZH$ interaction can be determined from the polarization observables of the $Z$ boson produced in association with the Higgs boson at an $e^{+}e^{-}$ collider. There have been several proposals for $e^{+}e^{-}$ colliders, especially to be employed as “Higgs factories”, operating around 240-250 GeV centre-of-mass (c.m.) energy. These are the International Linear Collider (ILC) in Japan [26], the Circular Electron Positron Collider (CEPC) in China [27], the Future Circular Collider with $e^{+}e^{-}$ (FCC-ee) at CERN (previously known as TLEP [28]). The Compact Linear Collider (CLIC) at CERN would possibly run at higher c.m. energies [29]. These colliders are planned to collect different integrated luminosities over time, which could be as high as 10 ab*-1* as for example in the case of the FCC-ee. We restrict ourselves to the illustrative case of the ILC operating at 250 GeV collecting 2 ab*-1* and at 500 GeV at a later stage, with 500 fb*-1* of data. It may be borne in mind that the sensitivities that we estimate may be conservative, and may be better at another collider with a larger luminosity.

We include in our discussion unpolarized beams as well as longitudinally polarized beams which are likely to be available at the ILC. Beam polarization has been known to have the advantage of suppressing certain backgrounds and enhancing the sensitivity by appropriate choice of signs of the polarization (see, for example, [30]).

We therefore make predictions for the $Z$ polarization variables, as also certain kinematic asymmetries in leptonic variables, since charged leptonic decay modes of the $Z$ would be ideal for the study of the polarization. It is expected that the ILC would initially run at a c.m. energy of 250 GeV, and that there would be a later run with c.m. energy 500 GeV. We consider both these possibilities. We also estimate the sensitivity of the leptonic asymmetries to possible $ZZH$ anomalous couplings, under ideal experimental conditions.

We consider the process $e^{-}e^{+}\rightarrow ZH$, where the vertex $Z_{\mu}(k_{1})\rightarrow Z_{\nu}(k_{2})H$ has the Lorentz structure

[TABLE]

where $g$ is the $SU(2)_{L}$ coupling and $\theta_{W}$ is the weak mixing angle. The form factors $a_{Z}$, $b_{Z}$ and $\tilde{b}_{Z}$ are in general complex. The first two couplings would correspond to CP-even terms in the interaction, while the third term is odd under CP. In the SM, the coupling $a_{Z}$ is unity at tree level, whereas the other two couplings $b_{Z}$ , $\tilde{b}_{Z}$ vanish at tree level, denoting the deviation from the tree-level SM value. Such anomalous couplings could arise from loop corrections in the SM or in any extension of SM with some new particles. However, we are not concerned with the latter and derive the helicity amplitudes for the process of our interest in a model-independent way, which follows in the next section, where we also evaluate the spin density matrix, which is crucial for a complete description of polarization.

At the LHC, both ATLAS and CMS collaborations have attempted to constrain the $ZZH$ anomalous couplings, though the limits are not very stringent. For example, CMS has put bounds on ratios of the cross section contributions arising from the different $ZZH$ couplings [19] which in our notation translate to $|{\rm Re}b_{Z}/a_{Z}|<0.058$ and $|{\rm Re}\tilde{b}_{Z}/a_{Z}|<0.078$ . Similarly, ATLAS [31] has put bounds on coefficients of an effective Lagrangian, assumed nonzero one at a time, which are related to the anomalous couplings we discuss. The bounds are again of about a few per cent. The possibility of a future Large Hadron electron Collider (LHeC) to probe anomalous $ZZH$ couplings has been studied in [32], where weak limits are found, viz., $-0.21<b_{Z}<0.43$ and $-0.32<\tilde{b}_{Z}<0.32$ for an electron beam energy of 60 GeV and mild improvement for a beam energy of 140 GeV, with proton beam energy of 7 TeV in either case. At $e^{+}e^{-}$ colliders, projections have been made for the measurement of these anomalous couplings in the context of various planned machines. Apart from measurement of the cross section of the dominant process $e^{+}e^{-}\to HZ$, suggestions have been made to include decay distributions as well as results of HL-LHC (see [33] for some relevant references) in a global analysis of various effective Lagrangian parameters. The estimates of sensitivity indicate (see for example [34]) that while HL-LHC would provide limits of the order of order $10^{-1}$ or $10^{-2}$, these would be improved to a per mille level on using angular distributions at electron-positron colliders. Our projections for $HZZ$ couplings are consistent with this general expectation, at the same time, providing a physical understanding through $Z$ polarization parameters.

2 Helicity amplitudes and density matrix

We compute the helicity amplitudes for the process

[TABLE]

in the massless limit of the initial particles, with the $ZZH$ vertex given in Eqn.(1). We will later construct angular asymmetries using the charged muon from $Z$ decay. This process receives a contribution from the “Higgsstrahlung” diagram, mediated by a $s$-channel $Z$. Our results also hold for the $Z$ decaying to taus, to the extent that the mass of the taus can be neglected. We do not consider $Z$ decay to $e^{+}e^{-}$ to avoid interference from the SM vector boson fusion diagram, though these effects are numerically small.

To calculate these amplitudes we adopt the following representations for the transverse and longitudinal polarization vectors of the $Z$:

[TABLE]

[TABLE]

where $E_{Z}$ and $\vec{p}_{Z}$ are the energy and momentum of the $Z$ respectively, with $\theta$ being the polar angle made by the $Z$ with respect to the $e^{-}$ momentum taken to be along the positive $z$ axis.

The helicity amplitudes which are non-zero in the limit of massless initial states are

[TABLE]

Here the first two entries in $M$ denote the signs of the helicities of the electron and positron respectively and the third entry is the $Z$ helicity. $\sqrt{s}$ is the total c.m. energy, and $c_{V}=-\frac{1}{2}+2\sin^{2}\theta_{W}$, $c_{A}=-\frac{1}{2}$ are the vector and axial vector couplings of the $Z$ to charged leptons.

In deriving these helicity amplitudes, we have assummed the SM value $a_{Z}=1$ for $a_{Z}$. However, the $a_{Z}$ dependence can be easily recovered by multiplying the helicity amplitude expressions by $a_{Z}$, and then replacing $b_{Z}$ and $\tilde{b}_{Z}$ by $b_{Z}/a_{Z}$ and $\tilde{b}_{Z}/a_{Z}$, respectively.

The spin-density matrix for $Z$ production expressed in terms of the helicity amplitudes is given by

[TABLE]

the average being over the initial helicities $\lambda$, $\lambda^{{}^{\prime}}$ of the electron and positron respectively and the indices $i,j$ can take values $\pm,0$. The diagonal elements of Eqn.(11) with $i=j$ would give the production probabilities of $Z$ with definite polarization, whose ratios to the total cross section are known as helicity fractions for the corresponding polarizations. Apart from these diagonal elements, it is also necessary to know the off-diagonal elements to include the spin information in a coherent way in the combination of the $Z$ production and decay processes. Then, on integrating over the phase space, the full density matrix Eqn.(11) would lead to the eight independent vector and tensor polarization components, known as the polarization parameters of the $Z$.

The density matrix elements, for unpolarized $e^{+}$ and $e^{-}$ beams, derived from the helicity amplitudes, to linear order in the anomalous couplings $b_{Z}$ and $\tilde{b}_{Z}$ and setting $a_{Z}=1$ are given by

[TABLE]

where $\beta_{Z}=|\vec{p}_{Z}|/E_{Z}$ is the velocity of the $Z$ in the c.m frame. The analytical manipulation software FORM [35] has been used to verify these expressions. We have kept the finite $Z$ width in our numerical calculations later.

The density matrix elements in Eqns. (12)-(15) are computed to leading order in the anomalous couplings, by taking the overlap of the BSM amplitudes with the SM amplitude for which $a_{Z}=1$. Any value of $a_{Z}$ not equal to one would represent BSM physics and thus its overlap with the $b_{Z}$ and $\tilde{b}_{Z}$ pieces would be quadratic in the anomalous couplings, which we neglect, assuming them to be small.

We do not display the somewhat longer expressions for the density matrix elements taking into account the polarizations $P_{L}$ and $\bar{P}_{L}$ of the electron and positron beams, respectively. However, the expressions are more compact on integration over $\cos\theta$, and these are displayed here:

[TABLE]

In the above equations, $P_{L}^{\rm eff}=(P_{L}-\bar{P}_{L})/(1-P_{L}\bar{P}_{L})$.

It is interesting to note that in the density matrix elements, while the SM contributions show the typical dominance of longitudinal polarization as as compared to the transverse polarizations, the contributions linear in $b_{Z}$ do not show this behaviour. The reason for this is the form of the tensor in the $b_{Z}$ vertex in (1), for which the leading contribution from the longitudinal polarization vector of the $Z$ vanishes. In fact, as will be seen later, the longitudinal and transverse contributions to the $b_{Z}$ dependence of the cross section turn out to be numerically equal.

Defining an integral of this density matrix over an appropriate kinematic range as $\sigma(i,j)$, the latter can be parametrized in terms of the linear polarization $\vec{P}$ and the tensor polarization $T$ as follows [36].

[TABLE]

where $\sigma(i,j)$ is the integral of $\rho(i,j)$, and $\sigma$ is the production cross section,

[TABLE]

In the following section, we construct the polarization parameters from the integrated density matrix elements and give relations of these to angular asymmetries of the decay leptons which would serve as measures of the polarization parameters.

3 $Z$ polarization and lepton asymmetries

The eight independent vector and tensor polarization observables can be extracted using appropriate linear combinations of the integrated density matrix elements of Eqn.(20):

[TABLE]

Of these $P_{x}$, $P_{y}$ and $P_{z}$ are the vector polarizations, whereas the $T$’s are the tensor polarizations, with the constraint that the tensor is traceless.

Experimentally, the spin information of the $Z$ is obtained from kinematic distributions of its decay products. Ref. [23] describes the formalism that connects all the spin observables of $Z$ to the angular distribution of the leptons arising from its decay. Ref. [23] also defines various asymmetries in the rest frame of the $Z$ which are simply related to the polarization observables given in Eqs.(22)-(29). These are given by

[TABLE]

[TABLE]

[TABLE]

[TABLE]

[TABLE]

[TABLE]

[TABLE]

[TABLE]

Here, $\alpha$ is the $Z$ boson polarization analyser, given in terms of its left and right handed couplings to charged leptons, $L_{\ell}$ and $R_{\ell}$ respectively, as

[TABLE]

The angles $\theta^{\ast}$ and $\phi^{\ast}$ are polar and azimuthal angles of the lepton in the rest frame of the $Z$. This frame is reached by a boost from the laboratory frame. In the laboratory frame, the initial $e^{-}$ beam defines the $z$ axis, and the production plane of $Z$ is defined as the $xz$. While boosting to the $Z$ rest frame, the $xz$ plane is kept unchanged. Then, the angles $\theta^{\ast}$ and $\phi^{\ast}$ are measured with respect to the would-be momentum of the $Z$.

We have evaluated these asymmetries in the case when initial beams are unpolarized or longitudinally polarized. It is observed that out of eight polarizations asymmetries only three, viz., $A_{x}$, $A_{x^{2}-y^{2}}$ and $A_{zz}$ are non-zero in the SM, which, along with the total cross section, would be proportional to the real part of the anomalous couplings to satisfy CPT theorem. This will be seen in the following section. Also, it can be seen from Eqs. (16)-(19) that only the asymmetries $A_{x}$, $A_{y}$, $A_{xz}$ and $A_{yz}$, which involve $\sigma(\pm,0)$ or $\sigma(0,\pm)$ in their definition through the corresponding polarization parameters have beam polarization dependence. The polarization dependence cancels between numerator and denominator in the remaining asymmetries.

4 Numerical results

Here we present numerical values for the integrated density matrix elements, the corresponding asymmetries and the sensitivities of the asymmetries to the various anomalous couplings. We consider two possibilities for the collider parameters, viz., c.m. energy $\sqrt{s}=250\text{~{}GeV}$, with integrated luminosity $\int\mathcal{L}dt=2$ $\text{ab}^{-1}$ and c.m. energy $500\text{~{}GeV}$ with integrated luminosity $\int\mathcal{L}dt=500$ fb*-1*. We consider longitudinal polarizations of $P_{L}=\pm 0.8$ for the electron beam and $\bar{P_{L}}=\pm 0.3$ for the positron beam, which are expected to be available at the collider. We assume, for simplicity, that the run with polarized beams is for the same luminosity as the run with unpolarized beams. We found that from among combinations with different signs of polarizations, the polarization combination $(P_{L},\bar{P}_{L})=(-0.8,+0.3)$ corresponds to the best sensitivity for given magnitudes of polarizations, and therefore we present results only for this combination, in addition to those for unpolarized beams.

In Tables 1 and 2 we present for c.m. energy 250 GeV the numbers for the integrated production density matrix elements $\sigma(i,j)$, $i,j$ taking values $\pm 1$ and [math], respectively for unpolarized beams and $(P_{L},\bar{P}_{L})=(-0.8,+0.3)$. In each table, the column labelled SM lists the values for the SM, whereas the other columns list the coefficients of the respective couplings in the density matrix element. The corresponding numbers for c.m. energy 500 GeV are given in Tables 3 and 4.

We next evaluate, using equations listed in the previous section, the leptonic asymmetries. For the SM, these are listed in Tables 5 and 6, together with the total cross sections, respectively for $\sqrt{s}=250$ GeV and $\sqrt{s}=500$ GeV. Note that except $A_{x}$, $A_{x^{2}-y^{2}}$ and $A_{zz}$, all other asymmetries vanish in the SM. This is because the asymmetries $A_{x},\,A_{x^{2}-y^{2}}$ and $A_{zz}$ are CP even and T even and they can occur at tree level in the SM. The remaining asymmetries vanish in the SM because they are either CP even and T odd and hence need an absorptive part in the amplitude to be nonzero, or CP odd, and hence proportional to CP violating parameters which are absent in the SM at tree level. With anomalous couplings, the CP even and T even asymmetries which are nonvanishing in the SM will get an additional contribution from $\text{Re}~{}b_{Z}$.

In Tables 7 and 8 we list, respectively for c.m. energies 250 and 500 GeV, the additional contributions to the cross section and various asymmetries for unit values of couplings, the coupling listed in each row being the only one which contributes to the observable in that row.

To obtain the $1\sigma$ limit $C_{\rm{limit}}$ on an anomalous coupling $C$ using these observables we use

[TABLE]

where $\sigma_{SM}$ is the SM cross section for the process $e^{+}e^{-}\to Z^{*}H\to\mu^{+}\mu^{-}H$, $A$ is the asymmetry for unit value of the coupling $C$, and $A_{SM}$ is the corresponding value in the SM. Similarly, the limit from the cross section may be obtained from

[TABLE]

We evaluate the limit considering one coupling to be non-zero at a time and list it in Tables 9 and 10 for the two different values of the c.m. energy and assuming no systematic uncertainty.

It is observed that the limit on the coupling $\text{Re}~{}b_{z}$ can be obtained from the observables $A_{x}$, $A_{zz}$ and $A_{x^{2}-y^{2}}$. However, among these we find that the observable $A_{zz}$ and the total cross section provide the best limits on the coupling $\text{Re}~{}b_{z}$, which becomes more stringent for the combination $(P_{L}=-0.8,\bar{P_{L}}=0.3)$ at $\sqrt{s}=500\text{~{}GeV}$. Also, we note that limits on the same obtained from the remaining observables slightly improves as one increases the c.m. energy especially for the combination where the electron polarization takes the negative sign. Although it seems that the total cross section is enough for probing the coupling $\text{Re}~{}b_{z}$, one will require the other angular asymmetries to explore the couplings which do not appear in the total cross section.

The best limit on $\text{Im}~{}\tilde{b}_{z}$ is $9.93\times 10^{-3}$, which comes from $A_{xz}$ whereas the best limit of $19.2\times 10^{-3}$ on $\text{Re}~{}\tilde{b}_{z}$ can be obtained from the observable $A_{xy}$ for a reduced beam energy of 250 GeV. Similarly the best bound of $10.7\times 10^{-3}$ on the coupling $\text{Im}~{}b_{z}$ can be achieved from the observable $A_{yz}$, which gets improved as one increases the c.m. energy to 500 GeV. As can be seen from the tables, the use of opposite sign beam polarization puts stronger constraints on the anomalous couplings, in some cases upto an order of magnitude better.

To estimate the effect of systematic uncertainties, we have also evaluated the limits taking a systematic error of 1% for the asymmetries and the cross section. We find that limits on couplings from various asymmetries worsen by a factor lying between 1.5 and 3 in the case of c.m. energy of 250 GeV. They are thus in the same ball park as the limits estimated in the absence of systematic uncertainty. However, the change in the limits for the case of c.m energy of 500 GeV is much smaller, only around 5-10%. Similarly, a 1% uncertainty in the measurement of the cross section leads to a change in the limits for the cross sections by 5-7% at 500 GeV, for unpolarized and polarized beams respectively, whereas the corresponding limits worsen by a factor between 1.6 to 1.8 for the case of 250 GeV.

5 Conclusions and discussion

After the discovery of the Higgs boson, it is of utmost importance to have a precise measurement of its couplings with all other SM particles. We propose to measure the form and magnitude of the couplings of the Higgs boson to a pair of $Z$ bosons at an electron-positron collider by making use of the polarization data of the $Z$ boson. We adopt the formalism which connects angular asymmetries of charged leptons from $Z$ decay to the polarization parameters of the $Z$. We take into account possible combinations of longitudinal beam polarizations likely to be available at the collider and have obtained the sensitivities of these polarization observables.

We see that most of the $1\sigma$ limits are of the order of a few times $10^{-3}$. Longitudinal polarization of the beam helps in increasing the sensitivities of certain observables. We find that that oppositely polarized beams provides tighter bounds on the couplings than the same sign polarized and unpolarized beams. Particularly a beam with $80\%$ electron polarization and $30\%$ positron polarization with opposite sign is found to be capable of placing better limits on the anomalous couplings. Limits get slightly improved as one increases the c.m. energy.

We have obtained the $Z$ polarization parameters and the asymmetries using the spin density matrix calculated at production level. However, at a collider these asymmetries will be determined from the angular distribution of the leptons from $Z$ decay and will thus entail acceptance and isolation cuts on the leptons. To get some idea of the cuts, we evaluated the asymmetries and sensitivities considered with generic acceptance cuts at the ILC: a 10 GeV cut on the lepton energy and a $5^{\circ}$ polar angle cut to keep away from the beam pipe. We find that these cuts lead to a less than $1\%$ change in all the observables including the total cross section.

We have also not considered Higgs decays, which do not affect the polarization parameters and asymmetries of the $Z$. The effect of Higgs decay on the sensitivities can be estimated by multiplying the SM cross section by the Higgs branching ratio and detection efficiencies in Eqns (39) and (40). A full scale analysis using an event generator coupled with all appropriate cuts and detection efficiencies relevant to the decay channels of the $Z$ and Higgs with be able to refine the actual sensitivities that we have obtained.

Acknowledgement: KR acknowledges support from IIT Bombay, grant no. 12IRCCSG032. SDR acknowledges support from the Department of Science and Technology, India, under the J.C. Bose National Fellowship programme, Grant No. SR/SB/JCB-42/2009.