Litcius/Paper detail

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi mathvariant="normal">Ξ</mml:mi></mml:math> hypernuclei <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:mi mathvariant="normal">Ξ</mml:mi><mml:mn>15</mml:mn></mml:mmultiscripts></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:mi mathvariant="normal">Ξ</mml:mi><mml:mn>12</mml:mn></mml:mmultiscripts></mml:math>, and the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi mathvariant="normal">Ξ</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:math> two-body interaction

Yusuke Tanimura, H. Sagawa, T. Sun, Emiko Hiyama

2022Physical review. C11 citationsDOIOpen Access PDF

Abstract

We study the energy spectra of $\mathrm{\ensuremath{\Xi}}$ hypernuclei $_{\mathrm{\ensuremath{\Xi}}}^{15}\mathrm{C}$ and $_{\mathrm{\ensuremath{\Xi}}}^{12}\mathrm{Be}$ with a relativistic mean field (RMF) model with meson exchange $\mathrm{\ensuremath{\Xi}}N$ interactions. The RMF parameters are optimized to reproduce the average energy of KINKA and IRRAWADDY events for the ground state and also the average energy of KISO and IBUKI events for the excited state in $_{\mathrm{\ensuremath{\Xi}}}^{15}\mathrm{C}$. The potential depth of the average $\mathrm{\ensuremath{\Xi}}N$ mean field potential is found to be about $\ensuremath{-}12$ MeV in the nuclear matter limit. We further introduce the two-body $s$- and $p$-wave interactions between valence nucleons and $\mathrm{\ensuremath{\Xi}}$ particle. We found that the $s$-wave interaction deduced from the HAL lattice QCD results is rather weak to obtain the energy difference between IRRAWADDY and KINKA events. The $p$-wave interaction is added and fitted to reproduce the energy difference. The resulting interaction together with the $s$-wave one gives a reasonable energy simultaneously for IBUKI event as an excited ${\mathrm{\ensuremath{\Xi}}}_{p}$ state. The model is further applied to predict the energy spectrum of $_{\mathrm{\ensuremath{\Xi}}}^{12}\mathrm{Be}$.

Topics & Concepts

Excited statePhysicsEnergy (signal processing)NucleonGround stateAtomic physicsQuantum mechanicsQuantum Chromodynamics and Particle InteractionsNuclear physics research studiesHigh-Energy Particle Collisions Research
<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi mathvariant="normal">Ξ</mml:mi></mml:math> hypernuclei <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi mathvariant="normal">C</mml:mi><mml:mprescripts/><mml:mi mathvariant="normal">Ξ</mml:mi><mml:mn>15</mml:mn></mml:mmultiscripts></mml:math> and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:mi mathvariant="normal">Ξ</mml:mi><mml:mn>12</mml:mn></mml:mmultiscripts></mml:math>, and the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi mathvariant="normal">Ξ</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:math> two-body interaction | Litcius