Matches in SemOpenAlex for { <https://semopenalex.org/work/W4290792904> ?p ?o ?g. }
- W4290792904 endingPage "115925" @default.
- W4290792904 startingPage "115925" @default.
- W4290792904 abstract "In this paper, we investigate the photon sphere, shadow radius and quasinormal modes of a 4-dimensional black hole with a deficit solid angle and quintessence-like matter. We find that the radii of the photon sphere and shadow decrease with the decreases of the deficit solid angle and density of quintessence-like matter. The quasinormal modes are gotten by the sixth order WKB approximation method and shadow radius, respectively. The values of the real part and imaginary parts of the quasinormal modes increase with the decrease of the values of the deficit solid angle and density of quintessence-like matter when the multipole number is fixed. The quasinormal modes gotten by these two methods are in good agreement, especially when the multipole number is large. It shows the correspondence between the quasinormal modes in the eikonal limit and shadow." @default.
- W4290792904 created "2022-08-09" @default.
- W4290792904 creator A5035008217 @default.
- W4290792904 creator A5039488385 @default.
- W4290792904 creator A5080434242 @default.
- W4290792904 date "2022-10-01" @default.
- W4290792904 modified "2023-10-01" @default.
- W4290792904 title "Quasinormal modes and the correspondence with shadow in black holes with a deficit solid angle and quintessence-like matter" @default.
- W4290792904 cites W1781678779 @default.
- W4290792904 cites W1968369949 @default.
- W4290792904 cites W1968833481 @default.
- W4290792904 cites W1984055616 @default.
- W4290792904 cites W2003968961 @default.
- W4290792904 cites W2004519466 @default.
- W4290792904 cites W2012710252 @default.
- W4290792904 cites W2022318322 @default.
- W4290792904 cites W2032416837 @default.
- W4290792904 cites W2037625321 @default.
- W4290792904 cites W2042402194 @default.
- W4290792904 cites W2045974707 @default.
- W4290792904 cites W2051736254 @default.
- W4290792904 cites W2071886922 @default.
- W4290792904 cites W2073115015 @default.
- W4290792904 cites W2075367341 @default.
- W4290792904 cites W2076572018 @default.
- W4290792904 cites W2080705137 @default.
- W4290792904 cites W2087146931 @default.
- W4290792904 cites W2094060752 @default.
- W4290792904 cites W2097909025 @default.
- W4290792904 cites W2102478229 @default.
- W4290792904 cites W2105585210 @default.
- W4290792904 cites W2107259515 @default.
- W4290792904 cites W2107788712 @default.
- W4290792904 cites W2152589129 @default.
- W4290792904 cites W2160926710 @default.
- W4290792904 cites W2168424351 @default.
- W4290792904 cites W2183584483 @default.
- W4290792904 cites W2273892807 @default.
- W4290792904 cites W2735495081 @default.
- W4290792904 cites W2936095933 @default.
- W4290792904 cites W2936349953 @default.
- W4290792904 cites W2937056002 @default.
- W4290792904 cites W2938000962 @default.
- W4290792904 cites W2997810586 @default.
- W4290792904 cites W3015768614 @default.
- W4290792904 cites W3028159267 @default.
- W4290792904 cites W3042231363 @default.
- W4290792904 cites W3098484659 @default.
- W4290792904 cites W3099270465 @default.
- W4290792904 cites W3099502603 @default.
- W4290792904 cites W3102854195 @default.
- W4290792904 cites W3104902166 @default.
- W4290792904 cites W3106230224 @default.
- W4290792904 cites W3121832579 @default.
- W4290792904 cites W3133596648 @default.
- W4290792904 cites W4226057253 @default.
- W4290792904 cites W4249956767 @default.
- W4290792904 cites W4295932358 @default.
- W4290792904 doi "https://doi.org/10.1016/j.nuclphysb.2022.115925" @default.
- W4290792904 hasPublicationYear "2022" @default.
- W4290792904 type Work @default.
- W4290792904 citedByCount "2" @default.
- W4290792904 countsByYear W42907929042023 @default.
- W4290792904 crossrefType "journal-article" @default.
- W4290792904 hasAuthorship W4290792904A5035008217 @default.
- W4290792904 hasAuthorship W4290792904A5039488385 @default.
- W4290792904 hasAuthorship W4290792904A5080434242 @default.
- W4290792904 hasBestOaLocation W42907929043 @default.
- W4290792904 hasConcept C110521144 @default.
- W4290792904 hasConcept C117797892 @default.
- W4290792904 hasConcept C121332964 @default.
- W4290792904 hasConcept C15744967 @default.
- W4290792904 hasConcept C172790937 @default.
- W4290792904 hasConcept C178635117 @default.
- W4290792904 hasConcept C26405456 @default.
- W4290792904 hasConcept C2780870619 @default.
- W4290792904 hasConcept C3079626 @default.
- W4290792904 hasConcept C36429004 @default.
- W4290792904 hasConcept C37914503 @default.
- W4290792904 hasConcept C38652104 @default.
- W4290792904 hasConcept C41008148 @default.
- W4290792904 hasConcept C44870925 @default.
- W4290792904 hasConcept C52765159 @default.
- W4290792904 hasConcept C542102704 @default.
- W4290792904 hasConcept C62520636 @default.
- W4290792904 hasConcept C88030215 @default.
- W4290792904 hasConceptScore W4290792904C110521144 @default.
- W4290792904 hasConceptScore W4290792904C117797892 @default.
- W4290792904 hasConceptScore W4290792904C121332964 @default.
- W4290792904 hasConceptScore W4290792904C15744967 @default.
- W4290792904 hasConceptScore W4290792904C172790937 @default.
- W4290792904 hasConceptScore W4290792904C178635117 @default.
- W4290792904 hasConceptScore W4290792904C26405456 @default.
- W4290792904 hasConceptScore W4290792904C2780870619 @default.
- W4290792904 hasConceptScore W4290792904C3079626 @default.
- W4290792904 hasConceptScore W4290792904C36429004 @default.
- W4290792904 hasConceptScore W4290792904C37914503 @default.
- W4290792904 hasConceptScore W4290792904C38652104 @default.