Dynamically generated momentum space shell structure of quarkyonic matter via an excluded volume model
Journal Article
·
· Physical Review C
- Asia Pacific Center for Theoretical Physics, Pohang (Korea); Univ. of Washington, Seattle, WA (United States); OSTI
- Univ. of Washington, Seattle, WA (United States)
The phase-space structure of zero-temperature quarkyonic matter is a Fermi sphere of quark matter surrounded by a shell of nucleonic matter. Here, we construct a quasiparticle model of quarkyonic matter based on the constituent quark model, where the quark and nucleon masses are related by $$m_Q = m_N/N_c$$, and $$N_c$$ is the number of quark colors. The region of occupied states is for quarks $$k_Q < k_F/N_c$$ and for nucleons $$k_F < k_N < k_F + Δ$$. We first consider the general problem of quarkyonic matter with hard-core nucleon interactions. We then specialize to a quasiparticle model where the hard-core nucleon interactions are accounted for by an excluded volume. In this model, we show that the nucleonic shell forms past some critical density related to the hard-core size and for large densities becomes a thin shell. We explore the basic features of such a model and argue this model has the semiquantitative behavior needed to describe neutron stars.
- Research Organization:
- Univ. of Washington, Seattle, WA (United States)
- Sponsoring Organization:
- Ministry of Science, ICT and Future Planning (MSIT); National Research Foundation of Korea (NRF); Simons Foundation; USDOE; USDOE Office of Science (SC)
- Grant/Contract Number:
- FG02-00ER41132
- OSTI ID:
- 1799977
- Alternate ID(s):
- OSTI ID: 1603198
- Journal Information:
- Physical Review C, Journal Name: Physical Review C Journal Issue: 3 Vol. 101; ISSN 2469-9985
- Publisher:
- American Physical Society (APS)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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