Superfluid Fermi atomic gas as a quantum simulator for the study of the neutron-star equation of state in the low-density region

Pieter Van Wyk, Hiroyuki Tajima, Daisuke Inotani, Akira Ohnishi, Yoji Ohashi

Research output: Contribution to journalArticle

12 Citations (Scopus)

Abstract

We propose a theoretical idea to use an ultracold Fermi gas as a quantum simulator for the study of the low-density region of a neutron-star interior. Our idea is different from the standard quantum simulator that heads for perfect replication of another system, such as the Hubbard model discussed in high-Tc cuprates. Instead, we use the similarity between two systems and theoretically make up for the difference between them. That is, (1) we first show that the strong-coupling theory developed by Nozières and Schmitt-Rink (NSR) can quantitatively explain the recent experiment on the equation of state (EoS) in a Li6 superfluid Fermi gas in the BCS (Bardeen-Cooper-Schrieffer) unitary limit far below the superfluid phase-transition temperature Tc. This region is considered to be very similar to the low-density region (crust regime) of a neutron star (where a nearly unitary s-wave neutron superfluid is expected). (2) We then theoretically compensate the difference that, while the effective range reff is negligibly small in a superfluid Li6 Fermi gas, it cannot be ignored (reff=2.7 fm) in a neutron star, by extending the NSR theory to include effects of reff. The calculated EoS when reff=2.7 fm is shown to agree well with the previous neutron-star EoS in the low-density region predicted in nuclear physics. Our idea indicates that an ultracold atomic gas may more flexibly be used as a quantum simulator for the study of other complicated quantum many-body systems, when we use not only the experimental high tunability, but also the recent theoretical development in this field. Since it is difficult to directly observe a neutron-star interior, our idea would provide a useful approach to the exploration for this mysterious astronomical object.

Original languageEnglish
Article number013601
JournalPhysical Review A
Volume97
Issue number1
DOIs
Publication statusPublished - 2018 Jan 3

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monatomic gases
neutron stars
simulators
equations of state
gases
nuclear physics
cuprates
crusts
transition temperature
neutrons

ASJC Scopus subject areas

  • Atomic and Molecular Physics, and Optics

Cite this

Superfluid Fermi atomic gas as a quantum simulator for the study of the neutron-star equation of state in the low-density region. / Van Wyk, Pieter; Tajima, Hiroyuki; Inotani, Daisuke; Ohnishi, Akira; Ohashi, Yoji.

In: Physical Review A, Vol. 97, No. 1, 013601, 03.01.2018.

Research output: Contribution to journalArticle

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