Projects per year
Abstract
in the nuclear equation of state at high matter densities. In this paper a first calculation of the role of the d∗(2380) in neutron stars is performed, based on a relativistic mean field description of the nucleonic degrees of freedom supplemented by a free boson gas of d∗(2380). The calculations
indicate that the d∗(2380) would appear at densities around three times normal nuclear matter saturation density, influencing the upper mass limit for a stable neutron star and the neutron and
proton fractions. New possibilities for neutron star cooling mechanisms arising from the d∗(2380)are also predicted.
Original language | English |
---|---|
Pages (from-to) | 112-116 |
Number of pages | 5 |
Journal | Physics Letters B |
Volume | 781 |
Early online date | 23 Mar 2018 |
DOIs | |
Publication status | Published - 10 Jun 2018 |
Bibliographical note
© 2018, The Author(s).Keywords
- EoS
- Hexaquarks
- Neutron stars
Profiles
Projects
- 2 Finished
-
Nuclear Physics Consolidated Grant
Jenkins, D. (Principal investigator), Andreyev, A. (Co-investigator), Bentley, M. (Co-investigator), Diget, C. A. (Co-investigator), Dobaczewski, J. J. (Co-investigator), Fulton, B. R. (Co-investigator), Laird, A. M. (Co-investigator), Paschalis, S. (Co-investigator), Pastore, A. (Co-investigator), Petri, M. (Co-investigator) & Wadsworth, R. (Co-investigator)
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL (STFC)
1/10/17 → 30/09/22
Project: Research project (funded) › Research
-
Nuclear Physics Theory
Dobaczewski, J. J. (Principal investigator) & Pastore, A. (Principal investigator)
SCIENCE AND TECHNOLOGY FACILITIES COUNCIL (STFC)
1/06/15 → 31/03/20
Project: Research project (funded) › Research