On Cooling of Neutron Stars with a Stiff Equation of State Including Hyperons
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...
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2018-02-01
|
| Series: | Universe |
| Subjects: | |
| Online Access: | http://www.mdpi.com/2218-1997/4/2/29 |