Matches in SemOpenAlex for { <https://semopenalex.org/work/W2024078140> ?p ?o ?g. }
- W2024078140 abstract "By assuming that only gravitation exists between dark matter (DM) and normal matter (NM), we study the effects of fermionic DM on the properties of neutron stars using the two-fluid Tolman-Oppenheimer-Volkoff formalism. It is found that the mass-radius relationship of the DM admixed neutron stars (DANSs) depends sensitively on the mass of DM candidates, the amount of DM, and interactions among DM candidates. The existence of DM in DANSs results in a spread of mass-radius relationships that cannot be interpreted with a unique equilibrium sequence. In some cases, the DM distribution can surpass the NM distribution to form DM halo. In particular, it is favorable to form an explicit DM halo, provided the repulsion of DM exists. It is interesting to find that the difference in particle number density distributions in DANSs and consequently in star radii caused by various density dependencies of nuclear symmetry energy tends to disappear as long as the repulsion of accumulated DM is sufficient. These phenomena indicate that the admixture of DM in neutron stars can significantly affect the astrophysical extraction of nuclear equation of state by virtue of neutron star measurements. In addition, the effect of the DM admixture on the star maximum mass is also investigated." @default.
- W2024078140 created "2016-06-24" @default.
- W2024078140 creator A5012831301 @default.
- W2024078140 creator A5030090528 @default.
- W2024078140 creator A5037090715 @default.
- W2024078140 creator A5083692659 @default.
- W2024078140 date "2014-02-13" @default.
- W2024078140 modified "2023-10-16" @default.
- W2024078140 title "Effects of fermionic dark matter on properties of neutron stars" @default.
- W2024078140 cites W1565680558 @default.
- W2024078140 cites W1969081735 @default.
- W2024078140 cites W1976036290 @default.
- W2024078140 cites W1977900177 @default.
- W2024078140 cites W1981514350 @default.
- W2024078140 cites W1983680550 @default.
- W2024078140 cites W1983770670 @default.
- W2024078140 cites W1984829288 @default.
- W2024078140 cites W1985363012 @default.
- W2024078140 cites W1987692311 @default.
- W2024078140 cites W2000291798 @default.
- W2024078140 cites W2016106149 @default.
- W2024078140 cites W2016400599 @default.
- W2024078140 cites W2016515266 @default.
- W2024078140 cites W2021717060 @default.
- W2024078140 cites W2027574739 @default.
- W2024078140 cites W2031831197 @default.
- W2024078140 cites W2034554023 @default.
- W2024078140 cites W2053222792 @default.
- W2024078140 cites W2054400164 @default.
- W2024078140 cites W2065553584 @default.
- W2024078140 cites W2071655161 @default.
- W2024078140 cites W2074288952 @default.
- W2024078140 cites W2076752847 @default.
- W2024078140 cites W2083034637 @default.
- W2024078140 cites W2084329918 @default.
- W2024078140 cites W2090896155 @default.
- W2024078140 cites W2091474967 @default.
- W2024078140 cites W2092350553 @default.
- W2024078140 cites W2097820102 @default.
- W2024078140 cites W2106558292 @default.
- W2024078140 cites W2109089400 @default.
- W2024078140 cites W2110352019 @default.
- W2024078140 cites W2133224752 @default.
- W2024078140 cites W2137338726 @default.
- W2024078140 cites W2138374709 @default.
- W2024078140 cites W2144622771 @default.
- W2024078140 cites W2145860733 @default.
- W2024078140 cites W2151085036 @default.
- W2024078140 cites W2156712718 @default.
- W2024078140 cites W2159751525 @default.
- W2024078140 cites W2162076236 @default.
- W2024078140 cites W2167572849 @default.
- W2024078140 cites W3099247730 @default.
- W2024078140 cites W3101311590 @default.
- W2024078140 cites W3104159254 @default.
- W2024078140 cites W3105880739 @default.
- W2024078140 cites W3126023968 @default.
- W2024078140 doi "https://doi.org/10.1103/physrevc.89.025803" @default.
- W2024078140 hasPublicationYear "2014" @default.
- W2024078140 type Work @default.
- W2024078140 sameAs 2024078140 @default.
- W2024078140 citedByCount "53" @default.
- W2024078140 countsByYear W20240781402015 @default.
- W2024078140 countsByYear W20240781402016 @default.
- W2024078140 countsByYear W20240781402017 @default.
- W2024078140 countsByYear W20240781402018 @default.
- W2024078140 countsByYear W20240781402019 @default.
- W2024078140 countsByYear W20240781402020 @default.
- W2024078140 countsByYear W20240781402021 @default.
- W2024078140 countsByYear W20240781402022 @default.
- W2024078140 countsByYear W20240781402023 @default.
- W2024078140 crossrefType "journal-article" @default.
- W2024078140 hasAuthorship W2024078140A5012831301 @default.
- W2024078140 hasAuthorship W2024078140A5030090528 @default.
- W2024078140 hasAuthorship W2024078140A5037090715 @default.
- W2024078140 hasAuthorship W2024078140A5083692659 @default.
- W2024078140 hasBestOaLocation W20240781402 @default.
- W2024078140 hasConcept C121332964 @default.
- W2024078140 hasConcept C134222618 @default.
- W2024078140 hasConcept C142362112 @default.
- W2024078140 hasConcept C150846664 @default.
- W2024078140 hasConcept C152568617 @default.
- W2024078140 hasConcept C153349607 @default.
- W2024078140 hasConcept C159249277 @default.
- W2024078140 hasConcept C165410206 @default.
- W2024078140 hasConcept C172695262 @default.
- W2024078140 hasConcept C178635117 @default.
- W2024078140 hasConcept C184665706 @default.
- W2024078140 hasConcept C185544564 @default.
- W2024078140 hasConcept C192887742 @default.
- W2024078140 hasConcept C38652104 @default.
- W2024078140 hasConcept C41008148 @default.
- W2024078140 hasConcept C44870925 @default.
- W2024078140 hasConcept C53810900 @default.
- W2024078140 hasConcept C558565934 @default.
- W2024078140 hasConcept C62520636 @default.
- W2024078140 hasConcept C73301696 @default.
- W2024078140 hasConcept C98444146 @default.
- W2024078140 hasConceptScore W2024078140C121332964 @default.
- W2024078140 hasConceptScore W2024078140C134222618 @default.