PaperPanorama

Nuclear Theory·nucl-th

Monday·January 14, 2019

6 papers4 primary·2 cross-listed

  1. 05

    [Submitted on 9 Jan 2019] (cross-list from cond-mat.quant-gas)

    Bose polaron in spherically symmetric trap potentials: Ground states with zero and lower angular momenta

    Kano Watanabe · Eiji Nakano · Hiroyuki Yabu

    Single-atomic impurities immersed in a dilute Bose gas in the spherically symmetric harmonic trap potentials are studied at zero temperature. In order to find the ground state of the polarons, we present a conditional variational method with fixed expectation values of the total angular momentum operators, and , of the system, using a cranking gauge-transformation for bosons to move them in the frame co-rotating with the impurity. In the formulation, the expectation value is shown to be shared in impurity and bosons, but the value is carried by the impurity due to the rotational symmetry. We also analyze the ground-state properties numerically obtained in this variational method for the system of the attractive impurity-boson interaction, and find that excited boson distributions around the impurity overlap largely with impurity's wave function in their quantum-number spaces and also in the real space because of the attractive interaction employed.

    Comments:
    31 pages, 6 figures. Some comments, references, and new figures in Fig.3 have been added
    Subjects:
    Quantum Gases (cond-mat.quant-gas); Nuclear Theory (nucl-th)
    arXiv:
    1901.02847 [pdf]
    PRA(2019)·3 citations
  2. 06

    [Submitted on 3 Jan 2019] (cross-list from gr-qc)

    Effect of Scalar Boson on Fermionic Dark Star

    A. B. Wahidin🇮🇩 · A. Rahmansyah🇮🇩 · A. Sulaksono🇮🇩

    The role of scalar boson exchange as a mediator of the fermionic dark particle interaction and the mass of dark particle on the bulk properties of fermionic dark stars including their moment of inertia and tidal deformability are studied. We have found that the role of the attractive nature of the scalar boson exchange and the fermionic dark particle mass can control the stiffness of the fermionic dark star equation of state. By increasing the strength of scalar boson coupling, the fermionic dark star becomes more compact. As a consequence, if scalar boson exchange contribution is included the compactness of a dark star can exceed =0.22. We also compare the fermionic dark stars moment of inertia and tidal deformability to those of neutron stars (with and without hyperons in neutron star core) predicted by relativistic mean field model. It is evidence that the properties of both types of stars are quite different. We also have found that the universal I-Love relation in fermionic dark stars is not affected by scalar boson exchange contribution and the fermionic dark particle mass. Possible observations of fermionic dark stars are also discussed.

    Comments:
    27 pages,11 figures, accepted for publication in IJMPD
    Subjects:
    General Relativity and Quantum Cosmology (gr-qc); Solar and Stellar Astrophysics (astro-ph.SR); High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    1901.03390 [pdf]
    Int.J.Mod.Phys.D(2019)·5 citations

Affiliations

first authorsco-authorsvia INSPIRE