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Hexaquarks under the microscope
Mikhail Bashkanov
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Baryon-Baryon molecule Meson-Baryon molecule
Possible particles Tetraquark Meson-Meson molecule Hexaquark Baryon-Baryon molecule Pentaquark Meson-Baryon molecule 𝑓 0 / 𝑎 0 (980) deuteron 𝑍 + (4430) Λ(1405) d ∗ (2380) 𝑃 𝑐 + (4450) Mikhail Bashkanov "Dibaryons"
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𝑑 ∗ (2380) hexaquark I(Jp) = 0(3+) Δ Δ 𝚪 𝒅 ∗ =𝟕𝟎 𝐌𝐞𝐕≪ 𝚪 𝚫𝚫 =𝟐𝟒𝟎 𝑴𝒆𝑽
𝚪 𝒅 ∗ =𝟕𝟎 𝐌𝐞𝐕≪ 𝚪 𝚫𝚫 =𝟐𝟒𝟎 𝑴𝒆𝑽 u u u d d d Threshold I(Jp) = 0(3+) 80 MeV d* Δ Δ 𝑴 𝒅 ∗ =𝟐.𝟑𝟖 𝑮𝒆𝑽≈𝟐 𝑴 𝚫 −𝟖𝟎 𝑴𝒆𝑽
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Total cross section pn d00
d*(2380) dibaryon 70 MeV P. Adlarson et. al Phys. Rev. Lett. 106:242302, 2011
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Dibaryon: hadronic decays
PRL 106 (2011) PLB 721 (2013) 229 WASA data 𝑑 𝜋 0 𝜋 0 𝑑 𝜋 + 𝜋 − pn d*(2380) 𝑝𝑛 𝑝𝑝 𝜋 − 𝜋 0 𝑝𝑛 𝜋 0 𝜋 0 𝑝𝑛 𝜋 + 𝜋 − PRL 112 (2014) PRC 90, (2014) d* PRC 88 (2013) PLB 743 (2015) 325 d* d*
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deuteron to d*(2380) transitions
0.15% 5% Deuteron: |6𝑞 |𝑝 𝑛 𝑆−𝑤𝑎𝑣𝑒 |𝑝 𝑛 𝐷−𝑤𝑎𝑣𝑒 𝜸 𝜸 𝑑 ∗ (2380): |6𝑞 |Δ Δ 𝑆−𝑤𝑎𝑣𝑒 |Δ Δ 𝐷−𝑤𝑎𝑣𝑒 66% 30% 2% d E2, ( 𝟐 + ) 𝜸 d*(2380) d M3, ( 𝟑 + ) 𝜸 𝐸 𝛾 ~570 𝑀𝑒𝑉 d E4, ( 𝟒 + ) 𝜸 deuteron
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d*(2380) in photoproduction?
𝜋 0 p 𝜋 0 d* d* d d d n 𝛾𝑑→𝑑 𝜋 0 𝜋 0 𝛾𝑑→𝑑 𝜋 0 𝜋 0 Conventional Background M. Egorov, A. Fix, Nucl.Phys. A933 (2015) 𝑑 ∗ M. Guenther, Hadron 2017 T. Ishikawa et al. Phys.Lett. B772 (2017) 398
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𝛾𝑑→ 𝑑 ∗ →𝑝𝑛
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Beam asymmetry Σ fit 𝜎 1 = 𝜎 ⊥ − 𝜎 ∥ =Σ𝜎 ~ 𝐽=2 𝐵 𝐽 𝑃 2 𝐽 (𝑐𝑜𝑠Θ)
𝜎 1 = 𝜎 ⊥ − 𝜎 ∥ =Σ𝜎 ~ 𝐽=2 𝐵 𝐽 𝑃 2 𝐽 (𝑐𝑜𝑠Θ) 𝜎 ⊥ − 𝜎 ∥ 𝜎 ⊥ + 𝜎 ∥ = 𝑃 𝛾 𝚺𝑐𝑜𝑠2𝜙 Σ Θ 𝜎 Θ 𝜎 0 ~ 𝐽=2 𝐵 𝐽 𝑃 2 𝐽 (𝑐𝑜𝑠Θ) 𝐵 𝐽 =𝑓(𝐸) – smooth function +BW for the d* Phys. Lett B789, (2019), 7-12
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Deuteron photodisintegration: beam asymmetry Σ
Σ Θ 𝜎 Θ 𝜎 0 ~ 𝐽=2 𝐵 𝐽 𝑃 𝐽 2 (𝑐𝑜𝑠Θ) 𝑑 ∗ M3 transition seems to be preferable
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𝑑 ∗ (2380) multipole expansion
𝑀3 𝐸2 ~ Ω d→ 𝑑 ∗ 𝑄 d→ 𝑑 ∗ ~ 𝑄 d→ 𝑑 ∗ 𝜇 d→ 𝑑 ∗ 𝑄 d→ 𝑑 ∗ ~ 𝑀 𝑑 𝜔 𝛾 2 𝜇 d→ 𝑑 ∗ If 𝜇 d→ 𝑑 ∗ is large the 𝑑→𝑑 ∗ M3 transition might be dominant 𝜇 𝑑 ∗ ∼7.6 𝜇 𝑁 Yubing Dong, Pengnian Shen, Zongye Zhang Phys.Rev. D 97, (2018), no.11,
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The benchmark measurement
d* p 𝛾 d n Measure polarization of both proton and neutron ! Mikhail Bashkanov "Dibaryons"
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Experiment 𝛾 𝑑→𝑝 𝑛 Target 𝜸 p 𝒏 Θ,𝜙,𝐸 p 𝚯 ′ ,𝝓′ Polarimeter
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Recoil polarization at 90 degree
Conventional background, Kang et al
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Recoil polarization at 90 degree
proton Conventional background, Kang et al H. Ikeda et al., Phys. Rev. Lett. 42, May 1979, 1321
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Recoil polarization at 90 degree
proton background+ d* Conventional background, Kang et al H. Ikeda et al., Phys. Rev. Lett. 42, May 1979, 1321
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Recoil polarization at 90 degree
neutron proton background+ d* Conventional background, Kang et al H. Ikeda et al., Phys. Rev. Lett. 42, May 1979, 1321
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Recoil polarization 𝑃(Θ) ~ 𝐽=1 𝐵 𝐽 𝑃 1 𝐽 (𝑐𝑜𝑠Θ)
𝑃(Θ) ~ 𝐽=1 𝐵 𝐽 𝑃 1 𝐽 (𝑐𝑜𝑠Θ) 𝑑 ∗ :𝐽=3 → 𝑃 1 3 (𝑐𝑜𝑠Θ)
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𝑑 ∗ size d*(2380) Transition form factor Charge distribution
* d*(2380) d Transition form factor Charge distribution Internal structure
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Nuclear matter at high density
p d* n Mikhail Bashkanov "Dibaryons"
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The d*(2380) in neutron stars a new degree of freedom?
I. Vidaña, M. Bashkanov, D.P. Watts, A. Pastore Phys.Lett. B781 (2018)
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Conclusion The very first hexaquark d*(2380) is established
Mass, Width, Quantum numbers Main decay branches Structure: Hexaquark vs Molecule? d*(2380) electro-magnetic coupling Size, 𝜇, 𝑄,Ω Neutron Stars? ( 𝑑 ∗ in medium)
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* * 𝑑 ∗ (2380) Thank you
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Recoil polarization at 90 degree
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d*(2380) in photoproduction?
R. Gilman and F. Gross nucl-th/ (2001) d* p T. Kamae, T. Fujita Phys. Rev. Lett. 38, Feb 1977, 471 d n H. Ikeda et al., Phys. Rev. Lett. 42, May 1979, 1321 I(Jp) = 0(3+) 𝐌=𝟐.𝟑𝟖 𝐆𝐞𝐕
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𝑑 ∗ and beam asymmetry Σ 𝟑 𝑫 𝟑 & 𝟑 𝑮 𝟑 𝑑 ∗
E2 transition ( 𝟐 + ) M3 transition ( 𝟑 + ) E4 transition ( 𝟒 + ) p 𝑑 ∗ 𝟑 𝑫 𝟑 & 𝟑 𝑮 𝟑 d n 90% 10% 𝜎 ⊥ − 𝜎 ∥ 𝜎 ⊥ + 𝜎 ∥ = 𝑃 𝛾 𝚺𝑐𝑜𝑠2𝜙 H. Arenhoevel, M. Sanzone “Photodisintegration of the deuteron”
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Beam asymmetry Σ 𝜎 ⊥ − 𝜎 ∥ 𝜎 ⊥ + 𝜎 ∥ = 𝑃 𝛾 𝚺𝑐𝑜𝑠2𝜙 Δ 𝜋
M1 transition ( 𝟏 + ) or E2 transition ( 𝟐 + ) p N 𝜎 ⊥ − 𝜎 ∥ 𝜎 ⊥ + 𝜎 ∥ = 𝑃 𝛾 𝚺𝑐𝑜𝑠2𝜙 E2/M1 ratio for the 𝛾𝑁→Δ 𝐸2 𝑀1 = 1 2 𝑘 𝑀 𝑁 𝑄 𝑧𝑧 𝑁Δ 𝜇 𝑁Δ T. Watabe et al. hep-ph R. Beck et al. (MAMI-A2) Phys.Rev. C61 (2000) Analysis of beam asymmetry 𝐸2 𝑀1 =2.5%
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Recoil polarization
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