Effects of modified dispersion relations on free Fermi gas: equations of state and applications in astrophysics
Autor: | Guilherme Grams, Franciele M. da Silva, L. C. N. Santos, Clésio E. Mota, Iarley P. Lobo |
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Přispěvatelé: | Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS) |
Rok vydání: | 2021 |
Předmět: |
Physics
Nuclear and High Energy Physics Fermi gas 010308 nuclear & particles physics QC1-999 Structure (category theory) Relativistic stars FOS: Physical sciences Relativistic star 01 natural sciences [PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph] Classical mechanics Physics - General Physics General Physics (physics.gen-ph) Simple (abstract algebra) Dispersion relation 0103 physical sciences 010306 general physics Nucleon Relations |
Zdroj: | Physics Letters B, Vol 822, Iss, Pp 136684-(2021) Physics Letters Phys.Lett.B Phys.Lett.B, 2021, 822, pp.136684. ⟨10.1016/j.physletb.2021.136684⟩ |
DOI: | 10.48550/arxiv.2110.00371 |
Popis: | International audience; Deformed dispersion relations are considered in the study of equations of state of Fermi gas with applications to compact objects. Different choices of deformed energy relations are used in the formulation of our model. As a first test, we consider a relativistic star with a simple internal structure. The mass-radius diagrams obtained suggest a positive influence of deformed Fermi gas, depending of the functions employed. In addition, we comment on how realistic equations of state, in which interactions between nucleons are taken into account, can be addressed. |
Databáze: | OpenAIRE |
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