On the charge distribution of $d^*(2380)$
Yubing Dong, Fei Huang, Pengnian Shen, and Zongye Zhang

TL;DR
This paper calculates and compares the charge distributions of the $d^*(2380)$ resonance under two different theoretical models, aiming to guide future experimental tests to distinguish these interpretations.
Contribution
It provides a detailed comparison of charge distributions for $d^*(2380)$ in two models, highlighting observable differences for experimental verification.
Findings
Significant differences in charge distributions between the two models.
Future experiments can distinguish between the models based on charge distribution data.
The study offers a theoretical basis for interpreting $d^*(2380)$ structure.
Abstract
We calculate the charge distributions of . Two different interpretations of the are considered for a comparison. One is a compact explanation with coupled two-channel approximation in the chiral constituent quark model. Another is a resonance state of . The remarkable differences of the charge distributions in the two pictures are shown and it is expected that the future experiments may provide a clear test for the different theoretical interpretations.
| Cases | |||
|---|---|---|---|
| A1 | A2 | ||
| 1.09 | 0.78 | 2.39 | |
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On the charge distribution of
Yubing Dong
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
Theoretical Physics Center for Science Facilities (TPCSF), CAS, Beijing 100049, China
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 101408, China
Fei Huang
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 101408, China
Pengnian Shen
College of Physics and Technology, Guangxi Normal University, Guilin 541004, China
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
Theoretical Physics Center for Science Facilities (TPCSF), CAS, Beijing 100049, China
Zongye Zhang
Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
Theoretical Physics Center for Science Facilities (TPCSF), CAS, Beijing 100049, China
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 101408, China
Abstract
We calculate the charge distributions of . Two different interpretations of the are considered for a comparison. One is a compact explanation with coupled two-channel approximation in the chiral constituent quark model. Another is a resonance state of . The remarkable differences of the charge distributions in the two pictures are shown and it is expected that the future experiments may provide a clear test for the different theoretical interpretations.
, Chiral quark model, Charge distributions, ,
pacs:
13.25.Gv, 13.30.Eg, 14.40.Rt, 36.10.Gv
I Introduction
is a new resonance recently observed by CELSIUS/WASA and WASA@COSY Collaborations CELSIUS-WASA ; CELSIUS-WASA1 . It was found in the analysis of double pionic fusion channels and when the ABC effect ABC and the analyzing power of the neutron-proton scattering data were studied. It is argued that the observed structure cannot be simply understood by either the intermediate Roper excitation contribution or by the t-channel process, Refs. CELSIUS-WASA ; CELSIUS-WASA1 proposed an assumption of existing a resonance whose quantum number, mass, and width are , MeV and MeV (see also their recent paper Bashkanov , the averaged mass and width are MeV and MeV, respectively). Since the baryon number of is 2, it would be treated as a dibaryon, and could be explained by either ”an exotic compact particle” or ”a hadronic molecule state” CERN . Moreover, since the observed mass of the is about 80 MeV below the threshold and about above the threshold, the threshold (or cusp) effect may not be so significant as that in the XYZ particles (see the review of XYZ particles Chen:2016qju for example). Thus, understanding the internal structure of would be of great interest.
The existence of such a non-trivial six-quark configuration with (called lately) has triggered a great attention and has intensively been studied in the literature even before the COSY’s discovery Dyson ; Thomas ; Oka ; Wang ; Yuan ; Kukulin . In fact, after the experimental observation of the , there are mainly three types of model explanation for its nature in the market. The first one Wang1 proposed a resonance structure and obtained a binding energy of about 71 MeV (namely MeV) and a width of about MeV. The second one Gal announced a broad resonant structure of for , whose resonant pole is around () +i () MeV. The third one Huang , following our previous prediction Yuan , suggested a dominant hexaquark structure for , with a mass of about MeV and a width of about MeV, respectively Huang ; Dong ; Dong1 ; Dong2017 . From the results of those models, one has three observations: (1) All proposed models can reproduce a right mass of ; (2) Only can last two models provide a total width for which compatible with the observed data; (3) only can the last model give all partial decay widths whose values agree with the observed data quite well. Even more, in terms of the third model (hexaquark dominant model), the predicted decay width of the single pion decay mode of is about ”1 MeV” which is much smaller than the double-pion decay widths Dong2017 . Here, we would particularly mention that this value is much smaller than that with the second scenario of , but agrees with the experimental observation very recently Clement2017 . All the outcomes from the third scenario support the idea that is probably a compact six-quark dominated exotic state due to its large component by Bashkanov, Brodsky and Clement Brodsky . Therefore, the model decay width of the process could be one of the way to justify the structure of , namely the width would be sensitive to the structure of . Although we have this weapon in hand, we are now still facing the problem that there is any additional way to justify different structure models. The general review on the dibaryon studies can be found in Ref. Clement .
It is known that the electromagnetic probe is one of the most useful tools to test the internal structure of a complicated system. For example, the electromagnetic form factors of the nucleon show the charge and magnetron distributions of a nucleon. The slops of the charge and magnetic distributions at original gives the charge and magnetic radii of the system. The precise measurement of the proton charge radius provides a criteria for different model calculations. For the spin-1 particle, like a deuteron or a - meson, the charge, magnetic and quadrupole form factors tell the intrinsic structures as well, like charge and magnetron distributions and the quadrupole deformation of the system. Therefore, the form factors of , for instance the charge distribution, might also be a physical quantity for discriminating the structure of . In this work, the charge distribution of the new resonance will be discussed with two different theoretical scenarios for comparison. One is a system with a single structure or a coupled structure in our chiral constituent quark model. The other one is a resonant system of . Moreover, the is a spin-3 particle, it has form factors. A detailed discussion of all the seven form factors is beyond the scope of this work and will be given elsewhere. Here we only concentrate on its charge distribution and the charge radius of the in the two scenarios.
This paper is organized as follows. In Sect. II, a brief discussion about the electromagnetic form factors of particles with spin-1/2, spin-1, and spin-3 will be shown. An explicit calculation of the charge distribution of with two scenarios is given in Sect. III. Sect. IV is devoted to a short summary.
II Electromagnetic form factors
The study of the electromagnetic form factors of the nucleon (spin-1/2) is of great interest because it can tell us the information about the charge and magnetron distributions of a nucleon. In the one-photon approximation, the electromagnetic current of a nucleon is
[TABLE]
where is nucleon mass, is momentum transfer, , and and are the Dirac and Pauli form factors, respectively. These two form factors relate to the electric and magnetic form factors
[TABLE]
with . The normalization conditions of the two form factors for the proton and neutron are , , , and , respectively.
In the Breit frame, we have , , , and . Then, we obtain Barik
[TABLE]
Clearly, the electric form factor is directly related to the matrix element of .
For a spin-1 particle, like deuteron, it contains three form factors. In the one-photon approximation, the electromagnetic current is
[TABLE]
where and stand for the polarization vectors of the incoming and outgoing deuterons, and are the polarizations of the two deuterons, and
[TABLE]
where . The three form factors relate to the charge , magnetic and quadrupole form factors as Barik
[TABLE]
with and is the deuteron mass. The charge, magnetic and quadrupole form factors are normalized to , , and , respectively. In the Breit frame, one may also see that the charge form factor of the deuteron can be obtained by direct calculating the matrix element .
For the particle, since its spin is 3, it has 2s+1=7 form factors. Its field can be expressed as a rank-3 tensor which is traceless. Clearly, , , and . In the one-photon exchange approximation, the general form of the electromagnetic current of a particle is
[TABLE]
and the matrix element
[TABLE]
where is the mass of , , and are the seven form factors, respectively. The gauge invariant condition
[TABLE]
is fulfilled as well as the time-reversal invariance. The combinations of the above seven form factors can give the physical form factors of such as the charge, magnetic, quadrupole as well as other higher-order multipole form factors. The normalization of all the form factors are unknown except for the charge form factor of . It should be mentioned that the discussion of all the seven form factors is beyond the scope of this paper, and it will appear elsewhere.
In analogy to the spin-1/2 nucleon and spin-1 deuteron cases, we assume that the charge distribution of the spin-3 particle, , is also directly relate to the matrix element of in the Breit frame. For the six-quark system, we just consider the quark-quark-photon current
[TABLE]
Thus, we may calculate the matrix element of and determine the charge distributions of the in the form of
[TABLE]
III Calculations of the charge distribution in two scenarios
III.1 Scenario A: Hexaquark dominant structure
Here, we only concentrate on the charge distribution of . As mentioned in Refs. Huang ; Dong , our model wave function for is obtained by dynamically solving the bound-state RGM equation of the six quark system in the framework of the extended chiral quark model, and then successively projecting the solution onto the inner cluster wave functions of the and CC channels. The resultant wave function of can finally be abbreviated to a form of
[TABLE]
where and are the fractions of the and components in , and denote the inner cluster wave functions of and (color-octet particle) in the coordinate space, and represent the channel wave functions in the and CC channels (in the single channel case, the component is absent), and and stand for the spin-isospin wave functions in the hadronic degrees of freedom in the corresponding channels, respectively Huang . It should be specially mentioned that in such a wave function, two channel wave functions are orthogonal to each other and contain all the totally anti-symmetrization effects implicitly Huang .
Unlike in calculations of the decay processes of , , and where the component does not contribute to the widths, here in the calculation of the charge distribution of the both the and components contribute. Considering that and are antisymmetric then the charge distribution is
[TABLE]
where the superscribe ”A” stands for the scenario A, , , and . Then
[TABLE]
where denote the overlaps of the wave functions of the 3-rd quark (or 6-th quark) which bombarded by photon in and C, and and represent the contributions from the and channel wave functions, respectively. can be calculated by
[TABLE]
Finally, one obtains
[TABLE]
where are the size-parameters of the and systems. As has been discussed explicitly in Ref. Dong , the channel wave function in the channel is written in terms of Gaussian-like wave functions as
[TABLE]
where and can be determined by fitting the channel wave function in this form to our projected model wave function calculated before. The normalization condition of the wave function is . Thus
[TABLE]
For the component, the channel wave function is dominated by the single S-wave Gaussian function
[TABLE]
Similarly, the contribution from the component can be calculated by
[TABLE]
III.2 Scenario B: structure
We can also calculate the wave function of with (I=1, S=2) by using our chiral SU(3) constituent quark model. The obtained mass is about ( is binding energy). It may be very close to the threshold of . Similar to eq. (18), the relative wave function between and can also be expressed as
[TABLE]
where and can be determined by fitting the relative wave function in this form to the resultant wave function of the in our model calculation.
We first calculate the charge distribution of by assuming it as a 6-quark system. The procedure is the same as that for the system shown in Sec. IIIA. The obtained charge distribution can be written in the following form:
[TABLE]
where stands for the third component of the isospin of and
[TABLE]
with
[TABLE]
and
[TABLE]
Now, we calculate the charge distribution of which is assumed to have a structure. What we would like to see is that if such type of structure of has a distinguishable charge distribution compared with the one shown in Sec. IIIA. Since the values of are , the relative motion between and has to be at least P-wave, and in the isospin space should be decomposed as
[TABLE]
The Jacobi momenta of D_{12}$$-\pi system are
[TABLE]
where and are the momenta of and , and stands for the relative momentum between the two systems. From the above equation, one sees that the bombarding effect of photon on the relative momentum is much smaller in the case where is stricken than that in the case where is hit. This is because of the factors of a=m_{\pi}/\Big{(}M_{{}_{D_{12}}}+m_{\pi}\Big{)}\sim 6/100 and b=1-a=M_{{}_{D_{12}}}/\Big{(}M_{{}_{D_{12}}}+m_{\pi}\Big{)}\sim 94/100.
Although the relative wave function between and is not strictly solved, one can still qualitatively see a general character of such a structure by assuming it being a wave function
[TABLE]
where is a so-called solid harmonics with , and denotes the size-parameter for the relative motion between the and . The size-parameter can be adopted in a large range, for instance from , and the real relative wave function could be a combination of such a function with different size-parameters. Then the contribution of the relative wave function between and can be calculated by
[TABLE]
where the subscript and in denote the situations when a photon hits and , respectively. The phenomenological monopole parametrization of the pion charge distribution can be borrowed from Ref. Ame86
[TABLE]
Then, the charge distribution of in the scenario can be written as
[TABLE]
It should be stressed that the pion contributions from the first and the third terms of eq. (27) canceled each other and the one from the second term vanishes since it relates to . Therefore, the charge distribution of in this scenario only comes from the contributions by and the relative motion between . Averaging over the initial states with various magnetic quantum numbers of , one finally obtain the charged distribution of
[TABLE]
where
[TABLE]
III.3 Numerical results in the two scenarios
In our calculations, we take , , , and as inputs. The probabilities in eq. (13) are and . In Fig. 1 we plot the channel wave functions of the in both the single channel (Scenario A1) and coupled channel (Scenario A2) approximations, respectively. In terms of the same chiral SU(3) constituent quark model, the wave functions of the system with can also been obtained by performing a bound state RGM calculation with a set of slightly varied model parameters whose values are still in a reasonable region. It is shown that in such a wave function, the component dominates the state with a fraction of about %, when the system is weakly bound with a binding energy of . The wave function of is displayed in Fig. 1. In terms of the wave functions in the A1, A2, and cases, the root-mean-square radii () of the can be straightforward calculated. The obtained are listed in Table 1.
In Fig. 1 and Table 1, one should notice that the wave function in the coupled channel approximation is normalized to . Clearly, we see that the wave function of is much more extended in radius in comparison with that of does. This is reasonable, because the energy level of this state is fairly close to the threshold, the system is almost broken up, namely and are ”almost free” and the separation between them becomes rather large. The smaller the binding energy is, the larger the size of the system would be. The root-mean-square radius of this component is . This value is consistent with the prediction from Heisenberg uncertainty Clement .
The charge distributions of the can be calculated by Eq. (17) in scenario A. The parameters and in Eq. (18) can be found in Refs. Dong ; Dong1 . The obtained charge distributions from and components are demonstrated in Fig. 2. The charge distribution of the single model (scenario A1) is plotted in Fig. 2 by a pink dotted-dashed curve. The black solid and the red dashed curves denote the contributions from the and components (scenario A2), respectively, and the black dotted curve represents the total contribution by summing over former two curves. These curves tell us that the contribution from component is larger than that from the component, especially, in the larger momentum transfer region, the contribution is dominated by the component. It implies that the quark contents in the component tend to concentrate in a more compact region than that in the component. This physics picture coincides with the radii of two components calculated in our previous paper Huang . Moreover, the curvature of the distribution curve of A1 is larger than that in the coupled channel case. It indicates that quarks here distribute in a larger region than that in the coupled channel case. The size information of can also be seen from the slope of the distribution curve at the origin, because such a slope is closely related to the radius of the system. The larger the slope at origin is, the larger the radius of the system would be. Comparing these slopes with the wave functions shown in Fig. 1, we find that the obtained slopes at the origin here coincide with the radii shown in Fig. 1. One sees that the radius resulted from the single channel wave function (A1) is larger than one from the two coupled-channel approximation (A2). Moreover, the radius contributed by the component is smaller than the one from component.
In order to see the size character of with a structure, the charge distribution of in the scenario B is calculated by Eq. (33). The obtained charge distribution curve, depicted by the blue double-dotted-dashed curve, is also drawn in Fig. 2 as well. It should be specially mentioned that in our numerical calculation, we do not solve the bound state problem for the system, explicitly. However, since the requirement of the conservations of the total spin and parity, the relative motion between and must be at least a P-wave. Therefore, if we ignore the component with higher partial wave, which will be greatly suppressed, the true relative wave function would be a superposition of the P-wave wave functions with different size-parameters . Thus, we calculate the charge distribution curves with a value from to . The result shows that those curves almost overlap with each other, namely this curve is almost insensitive to the size-parameter . This is because that the incoming photon is absorbed by the system, and the induced change of the relative momentum between the and is very small due to the factor of m_{\pi}/\Big{(}M_{{}_{D_{12}}}+m_{\pi}\Big{)}\sim 6/100. Comparing the curve of scenario B with others of scenario A, we see that the curves for the scenario decrease and go to zero much faster than those for the scenario A. A much larger slope at the origin means that the radius of the system is much larger in comparison with those in scenario A.
From our numerical calculation, we find that the ratios of the slopes of the curves at the origin in scenarios A1, A2, and B are
[TABLE]
It should be mentioned that the contributions to from and components in the coupled channel approximation of Scenario A2 are 0.64 and 0.81, respectively. The above obtained ratios tell us that the slop of the charge distribution of the in scenario B at is about 4.8 times larger than the one in Scenario A2, and the corresponding charge radius of scenario B is about 2.2 times larger than the one in scenario A2. This feature is compatable with that discussed in Ref. Gal1 . Finally, the very sharp charge distributions (or large charge radii) of in the scenario B is mainly dominated by the very broad wave function of the obtained . Therefore, we conclude that the two scenarios, A2 and B for the give very different descriptions for its charge distribution and its charge radius.
IV Summary
We have calculated the charge distribution of the in the two scenarios; one is a hexaquark dominant picture and another is a resonant picture. In the first picture, we show the total charge distribution and both contributions from its and components. In order to make a comparison, the result of the single channel is also shown. Comparing the predictions of the two scenarios, we see that the charge distribution from the system is remarkably different from the scenario A2, and consequentially, the charge radius of the the scenario B is obviously larger than that of the scenario A2.
We now expect a series of experiments which may be able to test different interpretations of in future. Although the direct scattering measurement may be hard to carry out, one may consider the form factors in the time-like region. For example, the production of the final pair in the and annihilation processes. It is our hope that the future upgraded BEPC, Belle and Babar and experiment at with high luminosity may provide a test for different theoretical understandings.
Acknowledgements.
We would like to thank Heinz Clement, Qiang Zhao, and Qi-Fang Lü for their useful and constructive discussions. This work is supported by the National Natural Sciences Foundations of China under the grant Nos. 11475192, 11475181, 11521505, 11565007, and 11635009, and by the fund provided to the Sino-German CRC 110 “Symmetries and the Emergence of Structure in QCD” project by NSFC under the grant No.11621131001, the IHEP Innovation Fund under the grant No. Y4545190Y2. F. Huang is grateful for the support of the Youth Innovation Promotion Association of CAS under the grant No. 2015358.
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