Recent development of hadron-hadron interactions: Case of...

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Takayasu SEKIHARA (Kyoto Prefectural Univ.) in collaboration with Yuki KAMIYA (Institute of Theoretical Physics, CAS) and Tetsuo HYODO (Tokyo Metropolitan Univ.) On-line seminar @ Yonsei Univ. (Sep. 21, 2020) Recent development of hadron-hadron interactions: Case of NΩ [1] T. S. , Y. Kamiya and T. Hyodo, Phys. Rev. C98 (2018) 015205. [2] T. S. , Y. Kamiya and T. Hyodo, in preparation.

Transcript of Recent development of hadron-hadron interactions: Case of...

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Takayasu SEKIHARA (Kyoto Prefectural Univ.) in collaboration with

Yuki KAMIYA (Institute of Theoretical Physics, CAS) and Tetsuo HYODO (Tokyo Metropolitan Univ.)

On-line seminar @ Yonsei Univ. (Sep. 21, 2020)

Recent development of hadron-hadron interactions:

Case of NΩ

[1] T. S. , Y. Kamiya and T. Hyodo, Phys. Rev. C98 (2018) 015205. [2] T. S. , Y. Kamiya and T. Hyodo, in preparation.

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On-line seminar @ Yonsei Univ. (Sep. 21, 2020)

1. Introduction

2. Model for the NΩ interaction, version 2018

3. Model for the NΩ interaction, version 202X (Under construction, conception only)

4. Summary

Contents

2

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On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 3

1. Introduction

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++ Nuclear physics ++ ■ Motivation for nuclear physics (in a broad sense) is to understand all the phenomena related to the strong interaction in terms of the underlying theory, quantum chromodynamics (QCD). - In terms of quark-gluon dynamics. ・ Quark confinement. ・ Chiral symmetry breaking. ・ Quark-gluon plasma. ・ Atomic nuclei and nuclear force. ・ Nucleosynthesis. ・ Neutron stars. ・ ...

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 4

1. Introduction

HIGGSTAN.

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++ Hadron-hadron interaction ++ ■ Because of the non-perturbative nature of QCD, we cannot directly solve QCD at low energies. □ The hadron-hadron interaction - the main subject in this talk - belongs to low-energy phenomena as well.

□ Traditional approaches to hadron-hadron interaction: - Perform hadron-hadron scattering experiments. - Construct phenomenological models.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 5

1. Introduction

e.g., nuclear force.HAL QCD.

n

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++ Nuclear force ++ ■ For example, the nuclear force has been investigated as:

- They are constructed phenomenologically so as to reproduce the experimental NN data.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 6

1. Introduction

Ishii, Aoki, and Hatsuda, Phys. Rev. Lett. 99 (2007) 022001.

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++ Recent breakthrough 1 ++ ■ A way to calculate hadron-hadron interactions directly in lattice QCD simulation by the HAL QCD collaboration.

□ Measuring the correlation function of two-hadrons, they obtained hadron-hadron interactions from QCD.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 7

1. Introduction

HAL QCD.

Aoki, Hatsuda, and Ishii, Prog. Theor. Phys. 123 (2010) 89.

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++ Recent breakthrough 1 ++ ■ A way to calculate hadron-hadron interactions directly in lattice QCD simulation by the HAL QCD collaboration.

□ Measuring the correlation function of two-hadrons, they obtained hadron-hadron interactions from QCD.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 8

1. Introduction

HAL QCD.

Aoki, Hatsuda, and Ishii, Prog. Theor. Phys. 123 (2010) 89.

Nuclear force.

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++ Recent breakthrough 1 ++ ■ A way to calculate hadron-hadron interactions directly in lattice QCD simulation by the HAL QCD collaboration.

□ Nowadays they performed simulations near the physical point, i.e., near the physical quark masses, mπ = 146 MeV and mK = 525 MeV, with large volume = (8.1 fm)3.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 9

1. Introduction

HAL QCD.

K computer.

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++ Recent breakthrough 1 ++ ■ A way to calculate hadron-hadron interactions directly in lattice QCD simulation by the HAL QCD collaboration.

□ In lattice QCD simulations, they obtain better signal to noise ratio as the number of strange quarks increases.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 10

1. Introduction

Talk by Hatsuda-san in QNP2018.

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++ Recent breakthrough 1 ++ ■ A way to calculate hadron-hadron interactions directly in lattice QCD simulation by the HAL QCD collaboration. □ ΩΩ system. - mΩ = 1712 MeV.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 11

1. Introduction

Gongyo et al. [HAL QCD], Phys. Rev. Lett. 120 (2018) 212001.

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++ Recent breakthrough 1 ++ ■ A way to calculate hadron-hadron interactions directly in lattice QCD simulation by the HAL QCD collaboration. □ NΩ system. - mΩ = 1712 MeV.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 12

1. Introduction

Iritani et al. [HAL QCD], Phys. Lett. B792 (2019) 284.

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++ Recent breakthrough 1 ++ ■ A way to calculate hadron-hadron interactions directly in lattice QCD simulation by the HAL QCD collaboration. □ ΛΛ-NΞ system. - (mN, mΛ, mΞ) = (956, 1140, 1355) MeV.

- Virtual pole in NΞ(11S0).

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 13

1. Introduction

Sasaki et al. [HAL QCD], Nucl. Phys. 998 (2020) 121737.

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++ Recent breakthrough 2 ++ ■ Hadron-hadron interactions can be confirmed by relativistic pp (not heavy ion, sorry) collisions (7 - 13 TeV). - 246,000 Λb -> J/ψ p K- !

□ Pc(4457) and other “exotic” states exist near D̅Σc thresholds. -> D̅Σc molecular states ?

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 14

1. Introduction

LHCb, Phys. Rev. Lett. 122 (2019) 222001.

American Physical Society.

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++ Recent breakthrough 2 ++ ■ Hadron-hadron interactions can be confirmed by relativistic pp (not heavy ion, sorry) collisions (7 - 13 TeV). □ So many theoretical calculations on the Pc states ... Here I quote only:

- Heavy quark spin symmetry + tensor force in OPEP. Good system to study hadron- hadron interaction.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 15

1. Introduction

Talk by Hosaka-san in 1st CENuM workshop for Hadron Physics, Inha Univ. (2019); Yamaguchi et al., Phys. Rev. D96 (2017) 114031; Liu et al., Phys. Rev. Lett. 122 (2019) 242001.

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++ Recent breakthrough 2 ++ ■ Hadron-hadron interactions can be confirmed by relativistic pp (not heavy ion, sorry) collisions (7 - 13 TeV). □ Hadron-hadron correlation provides information on the hadron-hadron interaction.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 16

1. Introduction

Theory: Morita et al., Phys. Rev. C91 (2015) 024916 (ΛΛ); Ohnishi et al., Nucl. Phys. A954 (2016) 294 (ΛΛ, K-p); Morita et al. Phys. Rev. C94 (2016) 031901 (pΩ); ExHIC, Prog. Part. Nucl. Phys. 95 (2017) 279 (ΛΛ, K-p); Hatsuda et al., Nucl. Phys. A967 (2017) 856 (pΞ-); Morita et al.,Phys. Rev. C101 (2020) 015201 (pΩ, ΩΩ); Kamiya et al. Phys. Rev. Lett. 124 (2020) 132501 (K-p).

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++ Recent breakthrough 2 ++ ■ Hadron-hadron interactions can be confirmed by relativistic pp (not heavy ion, sorry) collisions (7 - 13 TeV). □ Hadron-hadron correlation provides information on the hadron-hadron interaction.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 17

1. Introduction

Experiments: STAR, Phys. Rev. Lett. 114 (2015) 022301 (ΛΛ); ALICE, Phys. Rev. C99 (2019) 024001 (ΛΛ); STAR, Phys. Lett. B790 (2019) 490 (pΩ); ALICE, arXiv:2005.11495, submitted to Nature (pΩ, pΞ-); ALICE, Phys. Rev. Lett. 123 (2019) 112002 (pΞ-); ALICE, Phys. Rev. Lett. 124 (2020) 092301 (K-p).

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++ Recent breakthrough 2 ++ ■ Hadron-hadron correlations in the pp collisions.

□ Correlation depends on the source size and interaction. - The size can be fixed in another way.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 18

1. Introduction

ALICE, arXiv:2005.11495 (submitted to Nature).

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++ Recent breakthrough 2 ++ ■ Hadron-hadron correlations in the pp collisions.

- Exp. data are consistent with the HAL QCD potentials !

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 19

1. Introduction

ALICE, arXiv:2005.11495.

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++ Stimulation ++ ■ These breakthroughs stimulated further theoretical studies on the hadron-hadron interactions. □ For the NΩ system: - Chiral effective field theory, leading order & non-rel.

- Our meson exchange model.

□ In this talk, I would like to explain our model in detail.On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 20

1. Introduction

Haidenbauer et al., Eur. Phys. J. C77 (2017) 760.

T.S., Y. Kamiya and T. Hyodo, Phys. Rev. C98 (2018) 015205.

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2. Model for the NΩ interaction, version 2018

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++ Why NΩ system ? ++ ■ Expected feature of the NΩ interaction. □ Combination of N(uud / udd) [octet] + Ω(sss) [decuplet]. No same flavor. -> No repulsive core !?

□ Calculations in quark models. Goldman et al., Phys. Rev. Lett. 59 (1987) 627; Oka, Phys. Rev. D38 (1988) 298; Li and Shen, Eur. Phys. J. A8 (2000) 417; Pang, Ping, Wang, Goldman and Zhao, Phys. Rev. C69 (2004) 065207; Zhu, Huang, Ping and F. Wang, Phys. Rev. C92 (2015) 035210; Huang, Ping and Wang, Phys. Rev. C92 (2015) 065202; ...

- Although the details are different, these calculations indicate the existence of the NΩ bound state.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 22

2. Model for NΩ, ver.2018

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++ The NΩ system from lattice QCD ++ ■ The S-wave NΩ interaction (JP = 2+) in HAL QCD analysis of lattice QCD data (up to 2018).

□ No repulsive core !

□ Implying NΩ is bound.On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 23

Etminan et al. [HAL QCD], Nucl. Phys. A928 (2014) 89.

2. Model for NΩ, ver.2018

Doi et al. [HAL QCD], EPJ Web of Conf. 175 (2018) 05009.

□ mπ = 875 MeV.

□ Bound: BE ~ 19 MeV. □ mπ = 146 MeV.

□ Bound, but almost in the unitary limit.

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++ Motivation ++ ■ We want to understand the NΩ (5S2) interaction. □ What is the origin of the attraction ? - Physics behind it.

□ Extrapolate quark masses: mπ = 146 MeV to 138 MeV.

□ Discuss decay modes.

■ We construct baryon-baryon interaction model with meson exchanges.

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2. Model for NΩ, ver.2018

Doi et al. [HAL QCD], EPJ Web of Conf. 175 (2018) 05009.

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++ NΩ and coupled channels ++ ■ Consider the NΩ (5S2, JP = 2+) coupled-channels. □ Baryon-baryon systems in S = -3 & I = 1/2:

□ Decay channels: ΛΞ, ΣΞ - Couple to the NΩ (5S2) state in D wave.

□ Closed channel: ΛΞ* = ΛΞ(1530) (the nearest). On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 25

( 2S+1 L J )

2. Model for NΩ, ver.2018

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++ Elastic NΩ interaction ++ ■ Possible mediating mesons in the elastic NΩ interaction: □ Pseudoscalar: the η meson.

□ Scalar: the “σ” meson, which should be treated as as the correlated two pseudoscalar mesons (cf. nuclear force). - We employ the dispersion relation approach.

□ Vector: NO light vector mesons owing to the OZI rule.

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2. Model for NΩ, ver.2018

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++ Further terms of NΩ interaction ++ ■ We may consider further contributions at short ranges: □ Exchanges of heavier mesons.

□ Interactions at the quark-gluon level such as color magnetic interactions.

□ ...

-> We treat them as a contact term.

■ Box diagrams with K meson exchange give the inelastic channel contributions. □ ΛΞ, ΣΞ and ΛΞ*.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 27

2. Model for NΩ, ver.2018

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++ Summary of the NΩ interaction ++

■ Evaluate the NΩ (5S2) Int. with the above four diagrams.

□ Non-local interaction.

□ Energy dependence from the box terms.

□ Each vertex by effective Lagrangians. - Free parameter only in the contact interaction. (Cut-off is fixed as a typical hadron scale Λ = 1 GeV)

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2. Model for NΩ, ver.2018

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++ Model parameter ++ ■ The contact coupling constant c is fixed by information from the HAL QCD analysis (up to 2018).

- We could use potential V(r), but it is not observable in general (off-shell quantity). The potential may be non-local or change under the field redefinitions. -> It is safer to employ observable to fix coupling constant.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020)

2. Model for NΩ, ver.2018

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Doi et al. [HAL QCD], EPJ Web of Conf. 175 (2018) 05009.

e.g., Epelbaum et al. Rev. Mod. Phys. 81 (2009) 1773.

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++ Model parameter ++ ■ The contact coupling constant c is fixed by information from the HAL QCD analysis (up to 2018).

■ We reproduce the Scatt. length of the HAL QCD analysis on NΩ.

□ HAL QCD provides the nearly physical quark masses on the lattice. -> We fix c = - 22.1 GeV-2 to reproduce a = 7.4 fm with these lattice masses.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020)

2. Model for NΩ, ver.2018

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Scattering length a = 7.4 ± 1.6 fm at t = 11.

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++ Elastic NΩ interaction ++ ■ First, we show the NΩ (5S2) interaction in elastic channels:

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 31

VA [ GeV-2 ] - η exchange. VB [ GeV-2 ] - “σ” exchange.

2. Model for NΩ, ver.2018

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++ Elastic NΩ interaction ++ ■ First, we show the NΩ (5S2) interaction in elastic channels:

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 32

VA [ GeV-2 ] - η exchange. VB [ GeV-2 ] - “σ” exchange.

2. Model for NΩ, ver.2018

VC [ GeV-2 ] - contact.

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++ Elastic NΩ interaction ++ ■ Calculate V with p’ = p : V = V( p’ = p, p ).

□ The contact term is dominant.

□ The η and “σ” exchanges are moderate. - Small ηNN and “σ” ΩΩ couplings.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 33

2. Model for NΩ, ver.2018

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++ Inelastic NΩ interaction ++ ■ Next, we show the NΩ (5S2) Int. from inelastic channels:

- Calculate Vbox with p’ = p and E = mN + mΩ: V = Vbox( mN+mΩ; p’ = p, p ).

□ ΛΞ is the largest among the box terms owing to the large K̅NΛ coupling.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 34

2. Model for NΩ, ver.2018

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++ Inelastic NΩ interaction ++ ■ Next, we show the NΩ (5S2) Int. from inelastic channels:

- Calculate Vbox with p’ = p and E = mN + mΩ: V = Vbox( mN+mΩ; p’ = p, p ).

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 35

2. Model for NΩ, ver.2018

cf. Elastic V.

□ The attraction by inelastic channels is similar strength to the η / “σ” exchange.

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++ NΩ (5S2) scattering amplitude ++ ■ Scatt. amplitude fS as a function of relative momentum k:

■ Threshold parameters of the NΩ (5S2) scattering: □ Scattering length a:

--- Complex due to decay channels.

--- Positive real part implies existence of a bound state.

□ Effective range reff:

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 36

2. Model for NΩ, ver.2018

- Almost real.

NΩ (5S2)

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++ NΩ (5S2) quasi-bound state ++ ■ The NΩ (5S2) Scatt. amplitude contains a resonance pole which corresponds to the NΩ (5S2) quasi-bound state !

■ Epole = 2611.3 - 0.7 i MeV. -> BE = 0.1 MeV, Γ = 1.5 MeV.

■ We can extract the bound-state wave function ψNΩ from the residue of the resonance pole.

■ Coulomb assist for pΩ-: On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 37

2. Model for NΩ, ver.2018

| T(E) | [ GeV-2 ].

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On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 38

3. Model for the NΩ interaction, version 202X

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++ Update the NΩ interaction ++ ■ We have constructed the NΩ (5S2) interaction in 2018, but it is not so satisfactory today. Mainly because:

1. Experimental data from ALICE as well as the final version of the HAL QCD NΩ potential are available.

2. Contact term was not interpreted.

3. Potential shape of HAL QCD vs. our model.

4. Only 5S2.

-> Update is necessary !

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 39

3. Model for NΩ, ver.202X

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++ The latest data ++ ■ The latest data from ALICD and HAL QCD will help us to construct more reliable interaction.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 40

3. Model for NΩ, ver.202X

Iritani et al. [HAL QCD], Phys. Lett. B792 (2019) 284.

ALICE, arXiv:2005.11495.

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++ The latest data ++ ■ The latest data from ALICD and HAL QCD will help us to construct more reliable interaction.

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3. Model for NΩ, ver.202X

ALICE, arXiv:2005.11495.

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++ The latest data ++ ■ The latest data from ALICD and HAL QCD will help us to construct more reliable interaction.

□ We can fix our model parameter (coupling constant) with the Exp. correlation function. - In Exp., NΩ is a mixed state of various partial waves. -> We need 3S1 as well.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 42

3. Model for NΩ, ver.202X

ALICE, arXiv:2005.11495.

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++ Short-range part ++ ■ We have introduced a phenomenological contact term which contributes at short range.

□ What is the origin of the contact term ?

□ Interaction at the quark-gluon level is expected to be dominant.

-> We can calculate the contact term by quark exchange.

■ In calculating this, the approach by Yonsei group will be helpful.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 43

3. Model for NΩ, ver.202X

Park et al., Eur. Phys. J. A56 (2020) 93.

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++ Equivalent local potential ++ ■ Our NΩ (5S2) interaction is non-local. -> Construct a local potential as the sum of Yukawa form:

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 44

3. Model for NΩ, ver.202X

Coordinate space.

Fit function VC [ GeV-2 ]

Fitted.

Parameter listed in T.S., Y. Kamiya and T. Hyodo, Phys. Rev. C98 (2018) 015205.

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++ Comparison with the HAL QCD potential ++ ■ We compare our local NΩ (5S2) potential with the HAL QCD potential (mπ = 146 MeV). □ Behavior is qualitatively consistent with the HAL QCD.

□ However, the shape is different. - Cannot reproduce the long-range tail.

- Two-fold potential ?

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 45

3. Model for NΩ, ver.202X

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++ Comparison with the HAL QCD potential ++ ■ Mechanism to generate long-range tail of the potential ? □ We have checked that the η and “σ” exchanges give only moderate attraction because of small ηNN and “σ” ΩΩ couplings..

- Moderate attraction.

□ The K exchange to inelastic channels might help more. - Exchanged K carries energy (neglected in ver.2018) and hence it becomes closer to its on mass shell.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 46

3. Model for NΩ, ver.202X

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++ Comparison with the HAL QCD potential ++ ■ Nevertheless, we may not consider seriously the shape difference between the HAL QCD potential and ours. □ HAL QCD potential is based on the approach with the Nambu-Bethe-Salpeter wave function:

- We expect that the underlying theory is fine.

□ The potential is not observable in general (off-shell quantity), so it may change under the field redefinitions or may be non-local.

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 47

3. Model for NΩ, ver.202X

HAL QCD, Prog. Theor. Exp. Phys. 2012 01A105.

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++ Comparison with the HAL QCD potential ++ ■ Nevertheless, we may not consider seriously the shape difference between the HAL QCD potential and ours. □ Non-locality might take place (???) to generate long-range interaction. - ΞN, NΩ and ΩΩ give the same range of interactions. ΞN: π exchange, NΩ: NO π exchange, ΩΩ: NO π exchange. <- Why the same range ?

On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 48

3. Model for NΩ, ver.202X

Haidenbauer et al., Eur. Phys. J. A55 (2019) 70.

Comparison of HAL QCD potentials.

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4. Summary

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++ Summary ++ ■ We constructed the NΩ (5S2) interaction according to:

□ The conventional exchanges of the η, “σ”, and K (as boxes) mesons do not provide sufficient attraction.

□ Most of the attraction indicated in recent HAL QCD analysis is attributed to the short-range contact term.

■ Fitting parameter (contact coupling constant only) to scattering length in HAL QCD, we obtain the NΩ (5S2) quasi-bound state at Epole = 2611.3 - 0.7 i MeV. - BE = 0.1 MeV, Γ = 1.5 MeV.

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4. Summary

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++ Outlook ++ ■ We have to update our NΩ interaction. - In particular, Exp. data from ALICE as well as the final version of the HAL QCD NΩ potential are available.

■ NΩ (5S2) quasi-bound state, exists or not ?On-line seminar @ Yonsei Univ. (Sep. 21, 2020) 51

4. Summary

ALICE, arXiv:2005.11495.Iritani et al. [HAL QCD], Phys. Lett. B792 (2019) 284.?

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Thank you very much for your kind attention !