Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Wasif Husain"'
Publikováno v:
Universe, Vol 9, Iss 7, p 307 (2023)
Inspired by the well-known anomaly in the lifetime of the neutron, we investigated its consequences inside neutron stars. We first assessed the viability of the neutron decay hypothesis suggested by Fornal and Grinstein within neutron stars, in terms
Externí odkaz:
https://doaj.org/article/f5ceb30134ba42c880ee6149c94b561e
Publikováno v:
Universe; Volume 9; Issue 7; Pages: 307
Inspired by the well-known anomaly in the lifetime of the neutron, we investigated its consequences inside neutron stars. We first assessed the viability of the neutron decay hypothesis suggested by Fornal and Grinstein within neutron stars, in terms
Autor:
Wasif Husain, Anthony Thomas
We explore the suggestion that the neutron lifetime puzzle might be resolved by neutrons decaying into dark matter through the process, n \rightarrow \chi\chi\chi, with \chi having a mass one third of that of the neutron. In particular, we examine th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::765039975d5dc4b810e9b1903c5723a0
Autor:
Anthony W. Thomas, Wasif Husain
{We present a study of neutron star models that contain dark matter (DM) in the core. The DM is assumed to have a particle nature and to be self-interacting. Using constraints on the mass and radius of neutron stars, we investigate the allowed proper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7bf1fa666988384f2573836cb897ae04
Autor:
Wasif Husain, Anthony W. Thomas
We have constructed and compared models of rotating neutron stars and strange stars, within the Hartle framework. The significance of the low energy density region and crust region inside the neutron star has been studied, along with how much the exi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a61db097dcf901146dfac081f4f590b
http://arxiv.org/abs/2101.00951
http://arxiv.org/abs/2101.00951
Autor:
Wasif Husain, Anthony W. Thomas
We consider the possibility of having hybrid stars with a phase transition from hadrons into strange matter at the core of a neutron star in b equilibrium. For the hadron phase equation of state (EoS) the quark-meson coupling model is used, while the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bcf8442cf2cf1a5d9d5f82148020386b