on cooling of neutron stars with a stiff equation of state including hyperons
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ID: 248807
2018
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Abstract
Exploiting a stiff equation of state of the relativistic mean-field model MKVORH ϕ with σ -scaled hadron effective masses and couplings, including hyperons, we demonstrate that the existing neutron-star cooling data can be appropriately described within “the nuclear medium cooling scenario” under the assumption that different sources have different masses.
| Reference Key |
grigorian2018universeon
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|---|---|
| Authors | ;Hovik Grigorian;Evgeni E. Kolomeitsev;Konstantin A. Maslov;Dmitry N. Voskresensky |
| Journal | smart innovation, systems and technologies |
| Year | 2018 |
| DOI |
10.3390/universe4020029
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| URL | |
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