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  On the minimum mass of neutron stars

Suwa, Y., Yoshida, T., Shibata, M., Umeda, H., & Takahashi, K. (2018). On the minimum mass of neutron stars. Monthly Notices of the Royal Astronomical Society, 481(3), 3305-3312. doi:10.1093/mnras/sty2460.

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Item Permalink: https://hdl.handle.net/21.11116/0000-0002-58D4-C Version Permalink: https://hdl.handle.net/21.11116/0000-0002-FA30-E
Genre: Journal Article

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 Creators:
Suwa, Yudai1, Author
Yoshida, Takashi, Author
Shibata, Masaru2, Author           
Umeda, Hideyuki, Author
Takahashi, Koh, Author
Affiliations:
1YITP, Kyoto Univ. and Kyoto Sangyo Univ., ou_persistent22              
2Computational Relativistic Astrophysics, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_2541714              

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Free keywords: Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE, Astrophysics, Solar and Stellar Astrophysics, astro-ph.SR
 Abstract: We investigate the remnant neutron star mass, in particular the minimum mass.
We perform advanced stellar evolution calculations and neutrino-radiation
hydrodynamics simulations for core-collapse supernova explosions based on the
standard astrophysical scenarios. We find that from low-mass carbon-oxygen
cores which form sufficiently massive iron cores that eventually collapse, the
remnant neutron stars after supernova explosion are as light as 1.17 $M_\odot$,
which is compatible with the lowest mass of the neutron star precisely measured
in a binary system of PSR J0453+1559.

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 Dates: 2018-08-072018
 Publication Status: Issued
 Pages: 8 pages, 5 figures
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 Rev. Type: -
 Identifiers: arXiv: 1808.02328
DOI: 10.1093/mnras/sty2460
URI: http://arxiv.org/abs/1808.02328
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Title: Monthly Notices of the Royal Astronomical Society
Source Genre: Journal
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Pages: - Volume / Issue: 481 (3) Sequence Number: - Start / End Page: 3305 - 3312 Identifier: -