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Effects of strange molecular partners of PcP_{c} states in γpKΣ\gamma p\to K\Sigma reactions

Jian-Cheng Suo suojiancheng@itp.ac.cn CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics,
Chinese Academy of Sciences, Beijing 100190, China
School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China
   Di Ben bendi20@mails.ucas.ac.cn School of Nuclear Science and Technology, University of Chinese Academy of Sciences, Beijing 101408, China CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics,
Chinese Academy of Sciences, Beijing 100190, China
   Bing-Song Zou Department of Physics, Tsinghua University, Beijing 100084, China
(October 1, 2025)
Abstract

Our previous studies revealed evidence of the strange molecular partners of PcP_{c} states, N(2080)3/2N(2080)3/2^{-} and N(2270)3/2N(2270)3/2^{-}, in the γpK+Σ0/K0Σ+\gamma p\to K^{*+}\Sigma^{0}/K^{*0}\Sigma^{+} and γpϕp\gamma p\to\phi p reactions. Motivated by the differential cross-section data for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} from CLAS 2010, which exhibits some bump structures at WW\approx 1875, 2080 and 2270 MeV, we extend our previous analysis by investigating the effects of N(1535)1/2N(1535)1/2^{-}, N(1875)3/2N(1875)3/2^{-}, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-} and N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-}, as strange partners of PcP_{c} molecular states, in the reactions γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. The theoretical model employed in this study utilizes an effective Lagrangian approach in the tree-level Born approximation. It contains the contributions from ss-channel with exchanges of NN, Δ\Delta, NN^{*} (including the hadronic molecules with hidden strangeness), and Δ\Delta^{*}; tt-channel; uu-channel; and the generalized contact term. The results corresponding to the final fitted parameters are in good agreement with all available experimental data of both cross-sections and polarization observables for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. Notably, the ss-channel exchanges of molecules significantly contribute to the bump structures in cross-sections for γpKΣ\gamma p\to K\Sigma at WW\approx 1900, 2080 and 2270 MeV, and show considerable coherence with contributions from ss-channel exchanges of general resonances to construct the overall structures of cross-sections. More abundant experiments, particularly for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, are necessary to further strengthen the constraints on the theoretical models.

I INTRODUCTION

The several PcP_{c} states observed by the LHCb experiment in 2015 and later Aaij et al. (2015, 2019) are the most convincing multiquark candidates, prompting significant interest in investigating their nature Chen et al. (2016); Guo et al. (2018); Liu et al. (2019a). In the hadronic molecular picture, the Pc(4312)P_{c}(4312) can be interpreted as a narrow D¯Σc\overline{D}\Sigma_{c} bound state with spin-parity JP=1/2J^{P}=1/2^{-}, while the Pc(4440)P_{c}(4440) and Pc(4457)P_{c}(4457) can be interpreted as two degenerate narrow D¯Σc\overline{D}^{*}\Sigma_{c} bound states with JP=1/2& 3/2J^{P}=1/2^{-}\&\ 3/2^{-}, respectively He and Chen (2019); Chen et al. (2019); Liu et al. (2021). Moreover, a D¯Σc\overline{D}\Sigma_{c}^{*} bound state with JP=3/2J^{P}=3/2^{-} referred to as Pc(4380)P_{c}(4380), which is different from the broad one reported by LHCb in 2015, and three D¯Σc\overline{D}^{*}\Sigma_{c}^{*} bound states with JP=1/2,3/2& 5/2J^{P}=1/2^{-},3/2^{-}\&\ 5/2^{-} are also expected to exist, based on heavy quark spin symmetry Du et al. (2020, 2021); Liu et al. (2019b); Yalikun et al. (2021). The successful interpretation of these hidden-charm PcP_{c} states as the hadronic molecules inspires us to investigate their strange partners.

In the strange sector, S-wave KΣK\Sigma^{*} molecule N(1875)3/2N(1875)3/2^{-}, S-wave KΣK^{*}\Sigma molecules N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-} and S-wave KΣK^{*}\Sigma^{*} molecules N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-} are proposed as the strange partners of PcP_{c} molecular states He (2017); Zou and Dai (2018); Lin et al. (2018); Ben et al. (2023); Wu et al. (2023); Ben and Wu (2024). In Refs. Lin et al. (2018); Ben and Wu (2024), their decay patterns have been calculated using an effective Lagrangian approach. Notably, in the most recent Particle Data Group(PDG) review Navas et al. (2024), the two-star N(2080)N(2080) listed before the 2012 review has been split into two three-star states: N(1875)N(1875) and N(2120)N(2120). For consistency with our previous work, we retain the designation N(2080)3/2N(2080)3/2^{-} for the possible KΣK^{*}\Sigma molecule, which is not necessarily identified with the N(2120)N(2120) resonance in the PDG review. Furthermore, the contentious state N(1535)1/2N(1535)1/2^{-} can also be interpreted as a bound state of KΛ,KΣK\Lambda,K\Sigma within the molecular picture Zou and Dai (2018); Kaiser et al. (1995); Bruns et al. (2011); Li et al. (2024); Molina et al. (2024).

We have conducted several studies to investigate the effects of these hidden-strange molecules in photoproduction reactions. In Refs. Ben et al. (2023); Wu et al. (2023), the N(2080)3/2N(2080)3/2^{-} and N(2270)3/2N(2270)3/2^{-} are introduced in s-channel as the primary contributors to the γpK+Σ0/K0Σ+\gamma p\to K^{*+}\Sigma^{0}/K^{*0}\Sigma^{+} and γpϕp\gamma p\to\phi p reactions. The theoretical models constructed based on this fit well with the available experimental data for these reactions. Following this, we observe that the differential cross-section data for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} from CLAS 2010 Dey et al. (2010) exhibits bump structures near the center-of-mass energies WW = 1875, 2080 and 2270 MeV, as shown in Fig. 3, corresponding to the Breit-Wigner masses of N(1875)3/2N(1875)3/2^{-}, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-} and N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-}. Additionally, the KΣK\Sigma channel is essential in the molecular picture of N(1535)1/2N(1535)1/2^{-} Molina et al. (2024). These prompt us to focus on the γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+} reactions to test the effects of these seven hidden-strange molecules mentioned above.

The KΣK\Sigma photoproduction reactions have garnered significant attention both experimentally and theoretically over the past few years, contributing to the study of the light baryon resonance spectrum. In the experimental aspect, various collaborations such as CLAS, SAPHIR, LEPS have contributed large and diverse sets of experimental data on both cross-sections and polarization observables for the reaction γpK+Σ0\gamma p\to K^{+}\Sigma^{0} Glander et al. (2004); Kohri et al. (2006); Bradford et al. (2006); Dey et al. (2010); Schmieden (2014); Shiu et al. (2018); Jude et al. (2021); Lleres et al. (2007); Paterson et al. (2016); Shiu et al. (2018); Bradford et al. (2007). With the exception of some older measurements, these data generally show no significant discrepancies. For the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, several collaborations such as SAPHIR, CBELSA, A2 have also provided the experimental data Lawall et al. (2005); Castelijns et al. (2008); Aguar-Bartolome et al. (2013); Ewald et al. (2012); Nepali et al. (2013); Clark et al. (2024), including the latest data of polarization observables from the CLAS Collaboration Clark et al. (2024). However, in comparison to γpK+Σ0\gamma p\to K^{+}\Sigma^{0}, the amount of experimental data available for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} remains relatively sparse.

Many theoretical works have already been devoted to analyzing the data for KΣK\Sigma photoproduction, based on the effective Lagrangian approaches, isobar models, Regge-plus-resonance models, and so on Wei et al. (2022, 2023); Rönchen et al. (2022); Mart and Kholili (2019); Clymton and Mart (2021); Maxwell (2016); Sarantsev et al. (2005); Steininger and Meissner (1997); Mai et al. (2009); Kaiser et al. (1997); Borasoy et al. (2007); Golli and Širca (2016); Luthfiyah and Mart (2021); Egorov (2020); Lee et al. (2001); Tiator (2018); Corthals et al. (2007). In Refs. Mart and Kholili (2019); Clymton and Mart (2021) and Ref. Rönchen et al. (2022), photoproduction data for KΣK\Sigma have been simultaneously analyzed and effectively described using an isobar model and the Jülich-Bonn dynamical coupled-channel approach, respectively. And the work in Refs. Wei et al. (2022, 2023) provides a comprehensive analysis of the available data for γnK+Σ\gamma n\to K^{+}\Sigma^{-} and γnK0Σ0\gamma n\to K^{0}\Sigma^{0} reactions, based on an effective Lagrangian approach in the tree-level Born approximation.

In this work, we employ the methodology used in Refs. Wei et al. (2022, 2023) to simultaneously analyze data for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+} reactions. Our theoretical model incorporates contributions from ss-channel exchanges of NN, Δ\Delta, NN^{*}(including the hadronic molecules with hidden strangeness), and Δ\Delta^{*}; tt-channel exchanges of KK, K(892)K^{*}(892), and K1(1270)K_{1}(1270); uu-channel exchange of Σ\Sigma; and the generalized contact term. We utilize this model to investigate the reaction mechanisms and test the effects of hidden-strange molecules in γpKΣ\gamma p\to K\Sigma reactions.

The article is organized as follows. In Sec. II, we briefly introduce the framework of our theoretical model. Sec. III presents the details of our fitting settings. In Sec. IV, we show the results of our theoretical model along with some discussions. Finally, Sec. V provides the summary and conclusions.

II FORMALISM

As shown in Fig. 1, the gauge-invariant amplitude of KΣK\Sigma photoproduction reactions in the tree-level effective Lagrangian approach can be expressed as Wei et al. (2022, 2023)

M=Ms+Mt+Mu+Mint,\displaystyle M=M_{s}+M_{t}+M_{u}+M_{int}, (1)

where the terms MsM_{s}, MtM_{t}, MuM_{u} and MintM_{int} stand for the amplitudes calculated from the ss-channel mechanism, tt-channel mechanism, uu-channel mechanism and the interaction current, respectively.

Refer to caption
(a) ss-channel
Refer to caption
(b) tt-channel
Refer to caption
(c) uu-channel
Refer to caption
(d) Interaction current
Figure 1: Generic structure of the amplitude for γNKΣ\gamma N\to K\Sigma. Time proceeds from left to right.

Fig. 1(a) presents the ss-channel with exchanges of NN, Δ\Delta, NN^{*}, and Δ\Delta^{*}. The corresponding resonances are discussed in detail below. First, to investigate the effects of hidden-strange molecular states in KΣK\Sigma photoproduction, we introduce the seven molecules: N(1535)1/2N(1535)1/2^{-}, N(1875)3/2N(1875)3/2^{-}, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-} and N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-}. Second, in Ref. Wei et al. (2023), contributions from the N(1710)1/2+N(1710)1/2^{+}, N(1880)1/2+N(1880)1/2^{+}, N(1900)3/2+N(1900)3/2^{+}, N(1895)1/2N(1895)1/2^{-}, N(2060)5/2N(2060)5/2^{-}, Δ(1910)1/2+\Delta(1910)1/2^{+} and Δ(1920)3/2+\Delta(1920)3/2^{+} resonances have been taken into account to reproduce the available data for both γnK0Σ0\gamma n\to K^{0}\Sigma^{0} and γnK+Σ\gamma n\to K^{+}\Sigma^{-} reactions. Apart from the N(1710)1/2+N(1710)1/2^{+} which is marked as ”seen” in its decay branching ratio to the KΣK\Sigma channel, all the other considered resonances have sizable branching ratios in PDG Navas et al. (2024). In this work, we disregard the N(1895)1/2N(1895)1/2^{-} and N(2060)5/2N(2060)5/2^{-}, as their contributions are negligible when considering molecules, and we retain the other five resonances: N(1710)1/2+N(1710)1/2^{+}, N(1880)1/2+N(1880)1/2^{+}, N(1900)3/2+N(1900)3/2^{+}, Δ(1910)1/2+\Delta(1910)1/2^{+} and Δ(1920)3/2+\Delta(1920)3/2^{+}. Third, to achieve satisfactory numerical results, we refer to the analyses in Refs. Mart and Kholili (2019); Clymton and Mart (2021) and add seven additional resonances that may have significant contributions: N(1675)5/2N(1675)5/2^{-}, N(1720)3/2+N(1720)3/2^{+}, Δ(1600)3/2+\Delta(1600)3/2^{+}, Δ(1700)3/2\Delta(1700)3/2^{-}, Δ(1900)1/2\Delta(1900)1/2^{-}, Δ(1930)5/2\Delta(1930)5/2^{-} and Δ(1940)3/2\Delta(1940)3/2^{-}. In summary, besides the ground states NN and Δ\Delta, there are seven molecules, five general NN^{*} resonances and seven Δ\Delta^{*} resonances considered in ss-channel of our theoretical model, which are listed in Table 2.

Fig. 1(b) illustrates the tt-channel, which includes exchanges of KK and K(892)K^{*}(892) as considered in Refs. Wei et al. (2022, 2023), along with the K1(1270)K_{1}(1270), which may also contribute. Fig. 1(c) depicts the uu-channel with only the exchange of the bound state Σ\Sigma. As noted in Ref. Maxwell (2016), adding more resonances in the uu-channel did not materially improve the result. Therefore, we neglect other baryon exchanges in the uu-channel to reduce the number of fit parameters in our theoretical model, providing a cleaner background for testing the effects of molecules. Additionally, Fig. 1(d) presents the interaction current, which is modeled by a generalized contact current to ensure the gauge invariance of the full photoproduction amplitudes Wei et al. (2023).

Most parts of the formalism, including the Lagrangians, propagators, form factors attached to hadronic vertices, the gauge-invariance preserving term, and the interaction coupling constants, are detailed in Refs. Wei et al. (2022, 2023). For brevity, we do not repeat them here but present only the additional content relevant to the theoretical model in this work.

First, this work focuses on the γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+} reactions, so the coupling constant gγK0K0=0.631g_{\gamma K^{0}K^{*0}}=-0.631 referred to Ref. Wang et al. (2018), and different isospin factors will be used in the specific calculations. Second, the Lagrangians Maxwell (2016) and the propagator used for K1(1270)K_{1}(1270) are presented below:

γKK1=egγKK1MK((μAν)K(νK1μ)(νAμ)K(νK1μ)),\displaystyle\mathcal{L}_{\gamma KK_{1}}=-e\frac{g_{\gamma KK_{1}}}{M_{K}}\left(\left(\partial_{\mu}A^{\nu}\right)K\left(\partial_{\nu}K_{1}^{\mu}\right)-\left(\partial^{\nu}A_{\mu}\right)K\left(\partial_{\nu}K_{1}^{\mu}\right)\right), (2)
ΣNK1=Σ¯[(gΣNK1(1)γμgΣNK1(2)2MNσμνν)K1μγ5]N+H.c.,\displaystyle\mathcal{L}_{\Sigma NK_{1}}=-\overline{\Sigma}\left[\left(g_{\Sigma NK_{1}}^{(1)}\gamma^{\mu}-\frac{g_{\Sigma NK_{1}}^{(2)}}{2M_{N}}\sigma^{\mu\nu}\partial_{\nu}\right)K_{1\mu}\gamma_{5}\right]N+H.c., (3)
SK1(p)=iMK1+iΓK1/2(pμpνMK12gμν).\displaystyle S_{K_{1}}\left(p\right)=\frac{i}{\not{p}-M_{K_{1}}+i\Gamma_{K_{1}}/2}\left(\frac{p^{\mu}p^{\nu}}{M_{K_{1}}^{2}}-g^{\mu\nu}\right). (4)

Here, MKM_{K} and MNM_{N} denote the masses of KK and NN. The gγKK1g_{\gamma KK_{1}}, gΣNK1(1)g_{\Sigma NK_{1}}^{(1)} and gΣNK1(2)g_{\Sigma NK_{1}}^{(2)} are the electromagnetic and hadronic coupling constants treated as fit parameters. MK1M_{K_{1}} and ΓK1\Gamma_{K_{1}} are the mass and width for K1(1270)K_{1}(1270) with four-momentum pp.

Refer to caption
Refer to caption
Figure 2: Electromagnetic and hadronic couplings of N(2080)3/2N(2080)3/2^{-} as KΣK^{*}\Sigma molecule.

Finally, we briefly explain the treatment of the molecules in the ss-channel. Take N(2080)3/2N(2080)3/2^{-} as an example, which is assumed to be a pure SS-wave molecular state of KK^{*} and Σ\Sigma. In principle, in the hadronic molecular picture, both the electromagnetic and hadronic couplings of it are dedicated by the loop diagrams illustrated in Fig. 2 Lin et al. (2018). Here for simplicity, we just follow Ref. Ben et al. (2023) to calculate the tree-level approximation by introducing the effective Lagrangians Wei et al. (2022) of NN^{*} with spin-parity JP=3/2J^{P}=3/2^{-} for N(2080)3/2N(2080)3/2^{-}:

γNR3/2=iegγNR(1)2MNR¯μγνFμνN+egγNR(2)(2MN)2R¯μFμννN+H.c.,\displaystyle\mathcal{L}_{\gamma NR}^{3/2^{-}}=-ie\frac{g_{\gamma NR}^{(1)}}{2M_{N}}\overline{R}_{\mu}\gamma_{\nu}F^{\mu\nu}N+e\frac{g_{\gamma NR}^{(2)}}{(2M_{N})^{2}}\overline{R}_{\mu}F^{\mu\nu}\partial_{\nu}N+H.c., (5)
KΣR3/2=gKΣRMKΣ¯γ5(μK)Rμ+H.c..\displaystyle\mathcal{L}_{K\Sigma R}^{3/2^{-}}=-\frac{g_{K\Sigma R}}{M_{K}}\overline{\Sigma}\gamma_{5}\left(\partial_{\mu}K\right)R^{\mu}+H.c.. (6)

In addition, we attach a phase factor Exp[iϕRi\phi_{R}] in front of the tree-level amplitude, to partially mimic the loop contributions as illustrated in Fig. 2. Similarly, all the other hidden-strange molecules are treated in the same manner, and the Lagrangians introduced for them are referred to Ref. Wei et al. (2022), corresponding via the spin-parity. The masses of N(1535)1/2N(1535)1/2^{-}, N(1875)3/2N(1875)3/2^{-}, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-}, N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-} are taken as 1535, 1875, 2080 and 2270 MeV, respectively. Furthermore, the width ΓR\Gamma_{R} and coupling constants gγNR(1)g_{\gamma NR}^{(1)}, gγNR(2)g_{\gamma NR}^{(2)} and gKΣRg_{K\Sigma R}—which depend on the choice of cutoff parameters in Refs. Lin et al. (2018); Ben and Wu (2024)—along with the phase ϕR\phi_{R} of molecules, are treated as fit parameters.

III FITTING SETTINGS

The fit parameters of this theoretical model are adjusted to match the experimental data in a χ2\chi^{2} minimization using MINUIT James and Roos (1975); Dembinski and et al. (2020). Below, we present our selected settings for the experimental data and fit parameters.

III.1 Data base

Table 1: Experimental data used in the fit. The detailed information of the data presented in the table includes the reactions, observables, experimental collaborations, number, references, and additional weights applied in the fit.
Reaction Observable Collaboration Number Ref. Weight
γpK+Σ0\gamma p\to K^{+}\Sigma^{0} dσ/dcosθd\sigma/dcos\theta SAPHIR 2004 660 Glander et al. (2004) 1
LEPS 2006 54 Kohri et al. (2006)
CLAS 2006 1010 Bradford et al. (2006)
CLAS 2010 1288 Dey et al. (2010)
Crystal Ball 2014 1115 Schmieden (2014)
LEPS 2017 44 Shiu et al. (2018)
BGOOD 2021 22 Jude et al. (2021)
PP SAPHIR 2004 16 Glander et al. (2004) 1
GRAAL 2007 8 Lleres et al. (2007)
CLAS 2010 280 Dey et al. (2010)
Σ\Sigma LEPS 2006 30 Kohri et al. (2006) 1
GRAAL 2007 42 Lleres et al. (2007)
CLAS 2016 127 Paterson et al. (2016)
LEPS 2017 12 Shiu et al. (2018)
TT CLAS 2016 127 Paterson et al. (2016) 2
CxC_{x} CLAS 2007 70 Bradford et al. (2007) 3
CzC_{z} CLAS 2007 63 Bradford et al. (2007) 3
OxO_{x} CLAS 2016 127 Paterson et al. (2016) 3
OzO_{z} CLAS 2016 127 Paterson et al. (2016) 2
γpK0Σ+\gamma p\to K^{0}\Sigma^{+} dσ/dcosθd\sigma/dcos\theta SAPHIR 2005 120 Lawall et al. (2005) 7
CBELSA 2008 72 Castelijns et al. (2008)
A2 2013 50 Aguar-Bartolome et al. (2013)
CBELSA 2012 72 Ewald et al. (2012)
PP SAPHIR 2005 10 Lawall et al. (2005) 2
CBELSA 2008 23 Castelijns et al. (2008)
CLAS 2013 78 Nepali et al. (2013)
A2 2013 32 Aguar-Bartolome et al. (2013)
CLAS 2024 21 Clark et al. (2024)
Σ\Sigma CLAS 2024 21 Clark et al. (2024) 5
TT CLAS 2024 21 Clark et al. (2024) 5
OxO_{x} CLAS 2024 21 Clark et al. (2024) 5
OzO_{z} CLAS 2024 21 Clark et al. (2024) 5
In total 5784

The experimental data used in our fit are listed in Table 1. We have compiled nearly all available experimental data for the γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+} reactions. However, we exclude certain datasets, including the differential cross-section data for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} from the A2 2019 Akondi et al. (2019), the photon beam asymmetry data for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} from the CBELSA 2014 Schmieden (2014), and some older data, due to issues such as inconsistencies with others, sparsity or larger errors. To concentrate on the regions with potential contributions from exchanges of the molecules, we select the experimental data within the center-of-mass energy range from the KΣK\Sigma threshold up to 2400 MeV. The new polarization observables for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} from CLAS 2024 Clark et al. (2024) have also been included, and the definitions of the polarization observables are detailed in Refs. Dey et al. (2011); Sandorfi et al. (2011).

From Table 1, we can observe significant variations in the number of available data points across different reaction channels and observables, which may result in the fit ignoring some observable data due to their limited quantity. To address this issue, there is a standard weighting procedure commonly used in the field for this type of analyses, detailed in Refs. Rönchen et al. (2022); Clymton and Mart (2021). We also implement this method, adjusting the weights based on the number and fit quality of different observables. The final weights applied in our present study are also provided in Table 1.

III.2 Fit parameters

Here, we introduce the fit parameters of our theoretical model, which are listed in Table 2 and Table 3. First, the electromagnetic and hadronic coupling constants of the K1(1270)K_{1}(1270), molecules, general NN^{*} and Δ\Delta^{*} resonances, are treated as free parameters that need to be fitted. Since the reaction amplitudes are only sensitive to the products of electromagnetic and hadronic coupling constants, we make the products as the fit parameters instead of individual coupling constants, which are shown in Table 2. It is necessary to note that for the specific calculations of the reactions γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, the products gγNRgKΣRg_{\gamma NR}g_{K\Sigma R} should be multiplied by the corresponding isospin factor τ\tau.

Second, to reduce the number of fit parameters, we implement the following settings for the masses MRM_{R}, widths ΓR\Gamma_{R}, and phases ϕR\phi_{R} of molecules and general resonances. For molecules, the widths and phases are treated as fit parameters, while the masses are fixed, as mentioned in Sec. II. For four-star general resonances, only the masses of Δ(1910)\Delta(1910) and the widths of N(1720)N(1720), N(1900)N(1900), Δ(1910)\Delta(1910) are treated as fit parameters due to their large ranges recorded in PDG and relatively significant effects on fitted results. The masses and widths of other four-star general resonances are fixed according to PDG. For three-star and two-star general resonances, all masses and widths are treated as fit parameters.

Lastly, the cutoff parameters Λ\Lambda in the phenomenological form factors attached in each hadronic vertex are also treated as fit parameters. We merge some of them to reduce the number of fit parameters. Specifically, we use the same cutoff parameter Λt\Lambda_{t} for the tt-channel KK and K(892)K^{*}(892) exchanges, and the same cutoff parameter Λs\Lambda_{s} for the ss-channel ground states NN and Δ\Delta exchanges. Additionally, we merge the cutoff parameters of the molecules and general resonances located below the KΣK\Sigma threshold. For the molecules and general resonances above the threshold, the cutoff parameters are divided into ten groups based on their category and spin-parity, which are shown in Table 3.

In summary, our theoretical model contains a total of 77 fit parameters, which is a relatively streamlined number, that need to be adjusted to match the experimental data through the fitting program.

IV RESULTS AND DISCUSSION

IV.1 Fitted results

We construct χweight2\chi^{2}_{weight} with weights shown in Table 1, then determine the fitted values of the model’s free parameters by minimizing χweight2\chi^{2}_{weight} with MINUIT. Due to the large number of fit parameters and the sparsity of experimental data for some observables, the fitting process yields a few different convergence results. We have selected the most representative set of results as our final fitted results. The results of all 77 fit parameters are listed in Table 2 and Table 3, and the corresponding values of χ2\chi^{2} are listed in Table 4.

Table 2: Specific values of molecular and resonant parameters. The fitted values of free parameters are presented with uncertainties, while the values of the other parameters are fixed. The values in the brackets below general resonances’ masses and widths are corresponding values advocated by PDG Navas et al. (2024).
Molecule MR[MeV]M_{R}[MeV] ΓR[MeV]\Gamma_{R}[MeV] gγNR(1)gKΣRg_{\gamma NR}^{(1)}g_{K\Sigma R} gγNR(2)gKΣRg_{\gamma NR}^{(2)}g_{K\Sigma R} ϕR\phi_{R}
N(1535)1/2N(1535)1/2^{-} 1535 450450 0.157±0.004-0.157\pm 0.004 0.190±0.021-0.190\pm 0.021
N(1875)3/2N(1875)3/2^{-} 1875 450450 10.900±0.190-10.900\pm 0.190 12.230±0.22012.230\pm 0.220 2.473±0.017-2.473\pm 0.017
N(2080)1/2N(2080)1/2^{-} 2080 203±9203\pm 9 0.050±0.003-0.050\pm 0.003 2.756±0.0312.756\pm 0.031
N(2080)3/2N(2080)3/2^{-} 2080 144±7144\pm 7 0.630±0.0400.630\pm 0.040 0.880±0.040-0.880\pm 0.040 0.069±0.0340.069\pm 0.034
N(2270)1/2N(2270)1/2^{-} 2270 261±10261\pm 10 0.040±0.003-0.040\pm 0.003 3.685±0.0323.685\pm 0.032
N(2270)3/2N(2270)3/2^{-} 2270 450450 2.013±0.0342.013\pm 0.034 2.320±0.040-2.320\pm 0.040 11.203±0.026-11.203\pm 0.026
N(2270)5/2N(2270)5/2^{-} 2270 450450 0.574±0.013-0.574\pm 0.013 0.610±0.040-0.610\pm 0.040 0.998±0.0210.998\pm 0.021
Resonance MR[MeV]M_{R}[MeV] ΓR[MeV]\Gamma_{R}[MeV] gγNR(1)gKΣRg_{\gamma NR}^{(1)}g_{K\Sigma R} gγNR(2)gKΣRg_{\gamma NR}^{(2)}g_{K\Sigma R}
N(1675) 5/2N(1675)\ 5/2^{-} 1675 145145 0.492±0.0350.492\pm 0.035 2.630±0.1202.630\pm 0.120
**** [16651680][1665\sim 1680] [130160][130\sim 160]
N(1710) 1/2+N(1710)\ 1/2^{+} 1710 140140 0.193±0.0150.193\pm 0.015
**** [16801740][1680\sim 1740] [80200][80\sim 200]
N(1720) 3/2+N(1720)\ 3/2^{+} 1720 414±13414\pm 13 0.859±0.0330.859\pm 0.033 0.480±0.050-0.480\pm 0.050
**** [16801750][1680\sim 1750] [150400][150\sim 400]
N(1880) 1/2+N(1880)\ 1/2^{+} 1858±71858\pm 7 404±16404\pm 16 0.567±0.0260.567\pm 0.026
*** [18301930][1830\sim 1930] [200400][200\sim 400]
N(1900) 3/2+N(1900)\ 3/2^{+} 1920 155±3155\pm 3 0.189±0.0050.189\pm 0.005 0.360±0.014-0.360\pm 0.014
**** [18901950][1890\sim 1950] [100320][100\sim 320]
Δ(1600) 3/2+\Delta(1600)\ 3/2^{+} 1570 250250 1.804±0.020-1.804\pm 0.020 2.719±0.0402.719\pm 0.040
**** [15001640][1500\sim 1640] [200300][200\sim 300]
Δ(1700) 3/2\Delta(1700)\ 3/2^{-} 1710 300300 0.727±0.144-0.727\pm 0.144 0.012±0.162-0.012\pm 0.162
**** [16901730][1690\sim 1730] [220380][220\sim 380]
Δ(1900) 1/2\Delta(1900)\ 1/2^{-} 1853±21853\pm 2 161±8161\pm 8 0.053±0.0030.053\pm 0.003
*** [18401920][1840\sim 1920] [180320][180\sim 320]
Δ(1910) 1/2+\Delta(1910)\ 1/2^{+} 1950±11950\pm 1 400400 0.953±0.009-0.953\pm 0.009
**** [18501950][1850\sim 1950] [200400][200\sim 400]
Δ(1920) 3/2+\Delta(1920)\ 3/2^{+} 1913±21913\pm 2 178±8178\pm 8 0.111±0.0060.111\pm 0.006 0.040±0.0230.040\pm 0.023
*** [18701970][1870\sim 1970] [240360][240\sim 360]
Δ(1930) 5/2\Delta(1930)\ 5/2^{-} 1937±21937\pm 2 286±14286\pm 14 1.080±0.069-1.080\pm 0.069 0.647±0.1440.647\pm 0.144
*** [19002000][1900\sim 2000] [200400][200\sim 400]
Δ(1940) 3/2\Delta(1940)\ 3/2^{-} 1940±11940\pm 1 500500 7.280±0.092-7.280\pm 0.092 9.671±0.1159.671\pm 0.115
** [19402060][1940\sim 2060] [300500][300\sim 500]
MK1[MeV]M_{K_{1}}[MeV] ΓK1[MeV]\Gamma_{K_{1}}[MeV] gγK+K1+gΣ0pK1+(1)g_{\gamma K^{+}K_{1}^{+}}g_{\Sigma^{0}pK_{1}^{+}}^{(1)} gγK+K1+gΣ0pK1+(2)g_{\gamma K^{+}K_{1}^{+}}g_{\Sigma^{0}pK_{1}^{+}}^{(2)} gγK0K10gΣ+pK10(1)g_{\gamma K^{0}K_{1}^{0}}g_{\Sigma^{+}pK_{1}^{0}}^{(1)}
K1(1270) 1+K_{1}(1270)\ 1^{+} 1253 9090 1.060±0.1501.060\pm 0.150 1.876±0.166-1.876\pm 0.166 0.082±0.022-0.082\pm 0.022
Table 3: Fitted values of cutoff parameters (in MeV). The exchanged particles listed below share the same cutoff value.
Λt\Lambda_{t} ΛK1\Lambda_{K_{1}} Λu\Lambda_{u} Λs\Lambda_{s} Λ1\Lambda_{1}
K,K(892)K,K^{*}(892) K1(1270)K_{1}(1270) Σ\Sigma N,ΔN,\Delta N(2080)1/2,N(2270)1/2N(2080)1/2^{-},N(2270)1/2^{-}
667±1667\pm 1 767±21767\pm 21 700±1700\pm 1 985±3985\pm 3 2200±602200\pm 60
Λ2\Lambda_{2} Λ3\Lambda_{3} Λ4\Lambda_{4} Λ5\Lambda_{5} Λ6\Lambda_{6}
N(1710),N(1880)N(1710),N(1880) N(1720),N(1900)N(1720),N(1900) N(1875)3/2,N(2080)3/2N(1875)3/2^{-},N(2080)3/2^{-} N(2270)5/2N(2270)5/2^{-} Δ(1900)\Delta(1900)
N(2270)3/2N(2270)3/2^{-}
2000±32000\pm 3 1395±241395\pm 24 837±6837\pm 6 1150±41150\pm 4 1750±701750\pm 70
Λ7\Lambda_{7} Λ8\Lambda_{8} Λ9\Lambda_{9} Λ10\Lambda_{10} Λ11\Lambda_{11}
Δ(1910)\Delta(1910) Δ(1920)\Delta(1920) Δ(1700),Δ(1940)\Delta(1700),\Delta(1940) Δ(1930)\Delta(1930) N(1535)1/2,N(1675),Δ(1600)N(1535)1/2^{-},N(1675),\Delta(1600)
2000±72000\pm 7 873±15873\pm 15 1281±61281\pm 6 750±1750\pm 1 1700±11700\pm 1

Table 2 and Table 3 present the specific values of 77 fit parameters and some other fixed parameters in our theoretical model. It should be noted that that during the fitting process, we observed that the widths of N(1535)1/2N(1535)1/2^{-}, N(1875)3/2N(1875)3/2^{-}, N(2270)3/2& 5/2N(2270)3/2^{-}\&\ 5/2^{-}, Δ(1910)1/2+\Delta(1910)1/2^{+} and Δ(1940)3/2\Delta(1940)3/2^{-} tend to be larger; however, they have no significant impact on the fitted results. Consequently, the widths of N(1535)1/2N(1535)1/2^{-}, N(1875)3/2N(1875)3/2^{-}, N(2270)3/2& 5/2N(2270)3/2^{-}\&\ 5/2^{-} are set at 450 MeV, while the widths of Δ(1910)1/2+\Delta(1910)1/2^{+} and Δ(1940)3/2\Delta(1940)3/2^{-} are set at the upper limits of the width ranges recorded in PDG. Apart from these parameters, the other fit parameters have convergent fitted values with associated errors.

For the molecules, as calculated in Refs. Lin et al. (2018); Ben and Wu (2024), the widths exhibit a significant dependence on the cutoff parameters, and the range of widths for the molecules can cover the possible width range of the general nucleon excited states. Thus, it is difficult for us to provide accurate predictions for both the total width and the coupling constants of the molecules. The fitted values of them listed in Table 2 are deemed consistent with the calculations in Refs. Lin et al. (2018); Ben and Wu (2024) and regarded as reference.

For the general resonances in the ss-channel, Table 2 lists the fitted values of their fit parameters along with their basic information. Besides the coupling constants, some widths and masses are treated as fit parameters, with fitted values basically falling within the range recorded in the PDG. For K1(1270)K_{1}(1270), only three products of coupling constants serve as independent free parameters, and their fitted values are also presented in Table 2.

Table 3 presents the fitted values of the free cutoff parameters, with the exchanged particles listed below sharing the same cutoff value, as noted in Sec. III.2.

Table 4: The χ2\chi^{2} values for the reactions γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and K0Σ+K^{0}\Sigma^{+}. The χ2/Ndata\chi^{2}/N_{data} for each individual observable, as well as the χ2/(NdataNpar.)\chi^{2}/(N_{data}-N_{par.}) for the total data, are presented, where NdataN_{data} and Npar.N_{par.} denote the number of experimental data points and fit parameters, respectively.
Reaction Observable  (NdataN_{data}) χ2/Ndata\chi^{2}/N_{data}
γpK+Σ0\gamma p\to K^{+}\Sigma^{0} dσ/dcosθd\sigma/dcos\theta  (4193) 1.055
PP  (304) 1.852
Σ\Sigma  (211) 5.376
TT  (127) 1.748
CxC_{x}  (70) 1.881
CzC_{z}  (63) 1.801
OxO_{x}  (127) 2.501
OzO_{z}  (127) 1.754
In total  (5222) 1.365
γpK0Σ+\gamma p\to K^{0}\Sigma^{+} dσ/dcosθd\sigma/dcos\theta  (314) 1.519
PP  (164) 1.861
Σ\Sigma  (21) 1.360
TT  (21) 1.684
OxO_{x}  (21) 2.110
OzO_{z}  (21) 0.787
In total  (562) 1.614
In total  (5784) χ2/(NdataNpar.)=\chi^{2}/(N_{data}-N_{par.})= 1.408

Table 4 clearly illustrates the fit quality of the final fitted results. Here, χ2\chi^{2} presents an unweighted chi-squared statistic, while NdataN_{data} and Npar.N_{par.} indicate the number of experimental data points and free parameters, respectively. Nearly all the χ2/Ndata\chi^{2}/N_{data} values of the observables in the two reactions are around or below 2, indicating a high fitting quality for each observable. The only exception is the Σ\Sigma of the reaction γpK+Σ0\gamma p\to K^{+}\Sigma^{0}, where the χ2/Ndata\chi^{2}/N_{data} is relatively high. However, this is primarily due to the rather small error bars in the data points, while the fitting quality remains good, as shown in Fig. 8. Furthermore, the total χ2/(NdataNpar.)\chi^{2}/(N_{data}-N_{par.}) is 1.408, demonstrating the overall high quality of the fitted results. In conclusion, both in terms of individual observables and the overall picture, the quality of our fitted results is satisfactory. Achieving this is challenging for coupled-channel fits that involve two different reactions and data sets from various measurements, demonstrating the effectiveness of our theoretical model.

Table 5: The convergent fitted values for the masses of the molecules above the KΣK\Sigma threshold. These error-inclusive values come from the further fitting with the fitted results presented above as initial values.
MN(1875)3/2M_{N(1875)3/2^{-}} MN(2080)1/2M_{N(2080)1/2^{-}} MN(2080)3/2M_{N(2080)3/2^{-}} MN(2270)1/2M_{N(2270)1/2^{-}} MN(2270)3/2M_{N(2270)3/2^{-}} MN(2270)5/2M_{N(2270)5/2^{-}}
1896±41896\pm 4 2047±52047\pm 5 2005±52005\pm 5 2408±52408\pm 5 2258±32258\pm 3 2216±42216\pm 4

Moreover, as mentioned in Sec. II, the masses of the molecules are fixed in our theoretical model. To verify the stability of the fitted results with fixed molecular masses presented above, we further use this set of fitted values as initial values to perform the fitting with the molecular masses above the KΣK\Sigma threshold released. The convergent fitted values for the masses of N(1875)3/2N(1875)3/2^{-}, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-}, N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-} are listed in Table 5. The variation range for most of these masses is within 100 MeV. Notably, for N(2270)3/2N(2270)3/2^{-}, its mass varies by only 12 MeV, indicating a particularly strong tendency for N(2270)3/2N(2270)3/2^{-} to contribute in this region. In contrast, the variation in the mass of N(2270)1/2N(2270)1/2^{-} is relatively larger, and as shown in the following Fig. 5(b), its contribution is also comparatively small, suggesting that the experimental data does not strongly favor it.

IV.2 Cross-sections

Fig. 3 and Fig. 4 present the theoretical and experimental results for the differential cross-sections of γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, respectively. Our theoretical numerical results, corresponding to the parameters listed in Table 2, are compared with nearly all available experimental data. Additionally, the individual contributions from ss-channel molecule exchanges, ss-channel general resonance exchanges, and all the other terms—collectively referred to as the background—are displayed to facilitate the analysis of the reaction mechanisms.

Fig. 5 and Fig. 6 present the theoretical and experimental results for the total cross-sections of these two reactions, along with the individual contributions from single particle exchanges displayed below. The experimental data for the total cross-sections shown in the figures were not used in the fitting database, and are just compared with our theoretical predicted results. In addition, the calculated results of the HFF-P3 model in Ref. Clymton and Mart (2021) are included for further comparison. The work in Ref. Clymton and Mart (2021) provides a comprehensive analysis of nearly all available data for the four possible isospin channels of KΣK\Sigma photoproduction using a covariant isobar model. It is highly representative; according to Ref. Clymton and Mart (2021), among the three models, “the model HFF-P3 shows the best agreement with the experimental data (lowest χ2\chi^{2}) from all but the γnK0Σ0\gamma n\to K^{0}\Sigma^{0} channel.” Therefore, the calculated results of the HFF-P3 model are particularly valuable for comparison with our results.

Overall, the experimental data for both the differential and total cross-sections of the two reactions are well described. As shown in Table 4, the χ2/Ndata\chi^{2}/N_{data} values of the differential cross-sections are 1.055 for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and 1.519 for γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, indicating excellent agreement. Considering the differences in the amount of experimental data for the two reactions, this is a challenging yet satisfactory outcome, demonstrating the effectiveness of our theoretical model and the settings of weights. Additionally, from Fig. 3 to Fig. 6, we can also see that contributions from the ss-channel molecule exchanges are essential, indicating that the effects of the molecules are potentially significant in the γpKΣ\gamma p\to K\Sigma reactions. Moreover, we will discuss several other important features of the results below.

For the reaction γpK+Σ0\gamma p\to K^{+}\Sigma^{0}, contributions from the ss-channel Δ\Delta^{*} resonance exchanges are dominant, as illustrated in detail in Fig. 5(d). In fact, this is a reasonable expectation, which we will analyze in detail later by comparing the cross-sections and isospin factors of the two reactions. Regarding the background, as shown in Fig. 5(e), ss-channel proton exchange, tt-channel KK exchange, uu-channel Σ\Sigma exchange and the interaction current have little contributions. The ground state Δ\Delta exchange has a relatively significant contribution, similar to other Δ\Delta^{*} resonances. And the tt-channel K(892)K^{*}(892) and K1(1270)K_{1}(1270) exchanges provide considerable contributions of differential cross-sections at the forward angles in the high energy regions, as shown in Fig. 3.

As for the ss-channel molecule exchanges, as shown in Fig. 5(b), the N(1875)3/2N(1875)3/2^{-} exchange provides the largest contributions among molecules. Alongside N(1535)1/2N(1535)1/2^{-}, exchanges of these two molecules contribute across a wide energy range due to their relatively large widths. Together with contributions from ss-channel general resonance exchanges, they help construct the overall structure of the cross-sections, particularly the peak at W1900W\approx 1900 MeV. In addition, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-} and N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-} exchanges are mainly responsible for the peak structures around WW = 2080 and 2270 MeV, respectively, observable at both the backward and forward angular regions of the differential cross-sections in Fig. 3, as well as in the total cross-section shown in Fig. 5. The contributions from these molecules with different spins are roughly comparable, as illustrated in Fig. 5(b), showing no obvious preference for any particular spin.

In Fig. 5, we compare the total cross-section result from our theoretical model (red thick solid line) with that from the HFF-P3 model (blue thick dashed line) in Ref. Clymton and Mart (2021). Our result exhibits distinct peaks around WW = 2080 and 2270 MeV, while the HFF-P3 result appears smoother. This discrepancy indicates the significant effects of molecules within our model. In Sec. I, we have mentioned that the bump structures near WW = 1875, 2080 and 2270 MeV in differential cross-sections for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}, serve as one of the motivations for investigating the effects of the molecules in γpK+Σ0/K0Σ+\gamma p\to K^{+}\Sigma^{0}/K^{0}\Sigma^{+} reactions. The final fitted results indicate that these peak structures do contain significant contributions from the molecules.

From γpK+Σ0\gamma p\to K^{+}\Sigma^{0} to γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, the isospin factor τ\tau of gKΣΔg_{K\Sigma\Delta} changes from 2\sqrt{2} to 11, while the τ\tau of gKΣNg_{K\Sigma N} changes from 1-1 to 2\sqrt{2}. This is inclined to suggest that contributions from the ss-channel Δ\Delta^{*} resonance exchanges are more substantial for the reaction γpK+Σ0\gamma p\to K^{+}\Sigma^{0}, based on a simple comparison of the magnitudes of cross-sections for the two reactions shown in Fig. 5 and Fig. 6, respectively. Meanwhile, the contributions from NN^{*} and Δ\Delta^{*} resonance exchanges have become comparable for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, as depicted in Fig. 6(b) through Fig. 6(d), due to the variation of the isospin factor τ\tau. Therefore, if we want to investigate NN^{*} resonances, the K0Σ+K^{0}\Sigma^{+} reaction seems to be more important due to the amplified effects on isospin factors.

For the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, in terms of background, as shown in Fig. 6(e), the contribution from K1(1270)K_{1}(1270) exchange becomes negligible, while the contribution from K(892)K^{*}(892) exchange increases a lot for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} compared to γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Furthermore, the effects of the molecules are more pronounced. Fig. 4 illustrates the substantial interference effects between the contributions from ss-channel general resonance exchanges and molecule exchanges. The interference effects arise not only from isospin factors but also from the phase factors considered in the calculation of molecules, and these are one of the important reasons for the significant differences in the magnitudes of the cross-sections for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. Aside from these, most of the contribution characteristics of cross-sections for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} are similar to those for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. In Fig. 6, we also compare the total cross-section result from our theoretical model with that from the HFF-P3 model, which is provided up to 2150 MeV in Ref. Clymton and Mart (2021). And our result exhibits the additional variability around WW = 2080 MeV, due to the effects of the molecules.

However, it is clear that the experimental data for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+} are much sparser compared to these for the reaction γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. We improved the fitted results for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} by adjusting the weights during the fitting procedure, but we hope to obtain more experimental data for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} in the future to strengthen the constraints on the theoretical models.

Refer to caption
Figure 3: Differential cross-sections for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} as a function of the total center-of-mass energy WW. The collaborations of the experimental data are listed in the legend, and the detailed information can be found in Table 1. The red solid line represents our theoretical numerical result corresponding to the parameters listed in Table 2 and Table 3. And other three dashed lines represent the contributions from all the ss-channel molecule exchanges, ss-channel general resonance exchanges and the background (all the other terms).
Refer to caption
Figure 4: Differential cross-sections for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} as a function of the total center-of-mass energy WW. Except for A2 2019 Akondi et al. (2019) not used in the fitting database due to some inconsistencies, other experimental data can be found in Table 1. Notation for the theoretical numerical results is as in Fig. 3.
Refer to caption
(a) The total cross-section for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Except for SAPHIR 1998 Tran et al. (1998) and ABBHHM 1969 Erbe et al. (1969), other collaborations of experimental data can be found in Table 1. The blue thick dashed line represents calculated result of the HFF-P3 model in Ref. Clymton and Mart (2021). Notation for our theoretical numerical results is as in Fig. 3. Note that all data of the total cross-section shown in this figure were not used in the fitting database.
Refer to caption
(b) Molecules
Refer to caption
(c) General NN^{*} resonances
Refer to caption
(d) Δ\Delta^{*} resonances
Refer to caption
(e) Background
Figure 5: The total cross-section for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}, along with the individual contributions from single particle exchanges labeled on the right.
Refer to caption
(a) The total cross-section for γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. Except for CLAS 2005 Klein (2005), other collaborations of experimental data can be found in Table 1. Notation for numerical results of our theory and the HFF-P3 model is as in Fig. 5. For K0Σ+K^{0}\Sigma^{+}, the upper limit of the HFF-P3 model’s result presented in Ref. Clymton and Mart (2021) is 2150 MeV(marked with a black dashed line). Note that all data of the total cross-section shown in this figure were not used in the fitting database.
Refer to caption
(b) Molecules
Refer to caption
(c) General NN^{*} resonances
Refer to caption
(d) Δ\Delta^{*} resonances
Refer to caption
(e) Background
Figure 6: The total cross-section for γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, along with the individual contributions from single particle exchanges labeled on the right.

IV.3 Polarization observables

Fig. 7 to Fig. 15 display the polarization observables for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+} obtained in our theoretical calculations corresponding to the parameters listed in Table 2 and Table 3. Almost all of the available experimental data shown in these figures can be well described, which is truly encouraging and demonstrates the effectiveness of our theoretical model. We also present predictions for some regions currently lacking experimental data, which can be compared with future experimental results. There are two points that need further explanation below.

First, as mentioned in Sec. IV.1, the χ2/Ndata\chi^{2}/N_{data} of Σ\Sigma for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} is relatively high, primarily due to the rather small error bars associated with the data points. In Fig. 8, we can see that our theoretical results are in good agreement with the experimental data in most regions. However, due to the quite small error bars in the experimental data from CLAS 2016 Paterson et al. (2016), even slight deviations can lead to a significant increase in the value of χ2\chi^{2}. So we do not adjust the weight of it to improve its χ2\chi^{2}.

Second, the amount of experimental data for the polarization observables is still relatively limited, particularly for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, and the precision of some available experimental data is also insufficient. These result in the experimental data still not being adequately constraining for our model parameters. We just provide a potential theoretical result based on the currently available experimental data for the reactions γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. However, more abundant and high-precision experimental data, particularly for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, are necessary to further strengthen the constraints on the theoretical models.

Refer to caption
Figure 7: Recoil polarization PP for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} obtained in our theoretical calculations corresponding to the parameters listed in Tab. 2 and Tab. 3, compared with the experimental data shown in Tab. 1.
Refer to caption
Figure 8: Photon beam asymmetry Σ\Sigma for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Notation for the theoretical and experimental results is shown in the legend.
Refer to caption
Figure 9: Target asymmetry TT for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Notation for the theoretical and experimental results is shown in the legend.
Refer to caption
Figure 10: Beam-recoil double polarization CxC_{x} for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Notation for the theoretical and experimental results is shown in the legend.
Refer to caption
Figure 11: Beam-recoil double polarization CzC_{z} for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Notation for the theoretical and experimental results is shown in the legend.
Refer to caption
Figure 12: Beam-recoil double polarization OxO_{x} for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Notation for the theoretical and experimental results is shown in the legend.
Refer to caption
Figure 13: Beam-recoil double polarization OzO_{z} for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. Notation for the theoretical and experimental results is shown in the legend.
Refer to caption
Figure 14: Recoil polarization PP for γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. Notation for the theoretical and experimental results is shown in the legend.
Refer to caption
Figure 15: Recoil polarization PP, Photon beam asymmetry Σ\Sigma, Target asymmetry TT, Beam-recoil double polarizations OxO_{x} and OzO_{z} as functions of the cosθK0c.m.cos\theta_{K^{0}}^{c.m.}. All the experimental data are sourced from the CLAS 2024 Clark et al. (2024).

.

V SUMMARY AND CONCLUSION

Our previous studies revealed evidence of the strange molecular partners of PcP_{c} states, N(2080)3/2N(2080)3/2^{-} and N(2270)3/2N(2270)3/2^{-}, in the γpK+Σ0/K0Σ+\gamma p\to K^{*+}\Sigma^{0}/K^{*0}\Sigma^{+} and γpϕp\gamma p\to\phi p reactions Ben et al. (2023); Wu et al. (2023). Inspired by the experimental data of differential cross-sections for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} from CLAS 2010 Dey et al. (2010), which reveal some bump structures around WW = 1875, 2080 and 2270 MeV—corresponding to the Breit-Wigner masses of N(1875)3/2N(1875)3/2^{-}, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-}, N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-}—we decided to extend our previous work by investigating the effects of these six molecules, along with N(1535)1/2N(1535)1/2^{-}, as strange partners of PcP_{c} molecular states in the reactions γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. Our theoretical model is based on an effective Lagrangian approach in the tree-level Born approximation Wei et al. (2022, 2023), and contains the contributions from ss-channel with exchanges of NN, Δ\Delta, NN^{*}(including the hadronic molecules with hidden strangeness), and Δ\Delta^{*}; tt-channel; uu-channel; and the generalized contact term. Through some simplification settings in Sec. III.2, there are a total of 77 free parameters in the model listed in Table 2 and Table 3, which represents a relatively streamlined number of fit parameters. We then construct χweight2\chi^{2}_{weight} through our theoretical model, incorporating nearly all available experimental data and associated weights listed in Table 1. The fitted values of the free parameters are determined by minimizing the χweight2\chi^{2}_{weight} with MINUIT.

The theoretical results corresponding to the final fitted parameter values listed in Table 2 and Table 3 are in good agreement with all the available experimental data of both cross-sections and polarization observables for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+} reactions, which is directly reflected in the very low χ2/Ndata\chi^{2}/N_{data} values listed in Table 4. Achieving this is challenging for coupled-channel fits that involve two different reactions and data sets from various measurements, demonstrating the effectiveness of our theoretical model.

In the results of cross-sections, contributions from the ss-channel Δ\Delta^{*} resonance exchanges are more substantial for the reaction γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. In contrast, for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, the contributions from NN^{*} and Δ\Delta^{*} resonance exchanges become comparable. This difference is attributed to the variation in the isospin factor τ\tau. Regarding the background, ss-channel proton exchange, tt-channel KK exchange, uu-channel Σ\Sigma exchange and the interaction current have little contribution. The ground state Δ\Delta exchange has a relatively significant contribution, similar to other Δ\Delta^{*} resonances. In the reaction γpK+Σ0\gamma p\to K^{+}\Sigma^{0}, the tt-channel K(892)K^{*}(892) and K1(1270)K_{1}(1270) exchanges provide considerable contributions of differential cross-sections at the forward angles in the high energy regions. Conversely, for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, the contribution from K1(1270)K_{1}(1270) exchange becomes negligible, while the contribution from K(892)K^{*}(892) exchange increases a lot.

As for the molecules, the N(1875)3/2N(1875)3/2^{-} exchange provides the largest contributions among molecules. Alongside N(1535)1/2N(1535)1/2^{-}, exchanges of these two molecules contribute across a wide energy range due to their relatively large widths. Together with contributions from ss-channel general resonance exchanges, they help construct the overall structure of the cross-sections, particularly the peak at W1900W\approx 1900 MeV. Notably, the substantial interference effects between the contributions from ss-channel general resonance exchanges and molecule exchanges, are one of the important reasons for the significant differences in the magnitudes of the cross-sections for γpK+Σ0\gamma p\to K^{+}\Sigma^{0} and γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. In addition, N(2080)1/2& 3/2N(2080)1/2^{-}\&\ 3/2^{-} and N(2270)1/2,3/2& 5/2N(2270)1/2^{-},3/2^{-}\&\ 5/2^{-} exchanges are mainly responsible for the peak structures around WW = 2080 and 2270 MeV, respectively. And the contributions from these molecules with different spins are roughly comparable, showing no obvious preference for any particular spin. Moreover, compared with the HFF-P3 model in Ref. Clymton and Mart (2021), our results of total cross-sections exhibit distinct peaks around WW = 2080 and 2270 MeV, indicating the significant effects of molecules.

For the results of polarization observables, all experimental data are well described. The predictions for some regions currently lacking experimental data are also presented, which can be compared with future experimental results. However, the amount of experimental data for the polarization observables is still relatively limited, particularly for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}. Meanwhile, the cross-section data for γpK0Σ+\gamma p\to K^{0}\Sigma^{+} are also much sparser compared to those for γpK+Σ0\gamma p\to K^{+}\Sigma^{0}. These result in the experimental data still not being adequately constraining for our model parameters.

Furthermore, to verify the stability of these fitted results with the molecular masses fixed, we use this set of fitted values as initial values to perform the fitting with the molecular masses above the KΣK\Sigma threshold released. The convergent fitted values for most of the molecular masses fall within a variation range of 100 MeV. Notably, the mass of N(2270)3/2N(2270)3/2^{-} remains almost unchanged, indicating a particularly strong tendency for N(2270)3/2N(2270)3/2^{-} to contribute in this region.

More abundant experiments are necessary to further strengthen the constraints on the theoretical models, particularly for the reaction γpK0Σ+\gamma p\to K^{0}\Sigma^{+}, due to the effects of isospin factors and the unbalanced datasets. Hopefully further experiments can distinguish various models.

VI ACKNOWLEDGMENTS

We thank Feng-Kun Guo, Jia-Jun Wu, Shu-Ming Wu, Zhen-Hua Zhang and Chao Tang for their useful discussions and valuable comments. This work is supported by the NSFC and the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through the funds provided to the Sino-German Collaborative Research Center TRR110 “Symmetries and the Emergence of Structure in QCD” (NSFC Grant No. 12070131001, DFG Project-ID 196253076-TRR 110), by the NSFC Grant No. 12047503, and by the Chinese Academy of Sciences (CAS) under Grant No. XDB34030000.

References