Gravitational Tidal Deformations of Rotating Black Holes.
Black holes are influenced by external gravitational fields in the universe, which are generated by other astrophysical objects in their surroundings. Because of this gravitational interaction, they experience tidal deformations of their event horizons. To quantify this effect, we compute the so-cal...
| Publicado en: | Journal of the Utah Academy of Sciences, Arts & Letters Vol. 102; p. 379 |
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| Autores principales: | , , , , , |
| Formato: | Artículo |
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Utah Academy of Sciences, Arts & Letters
2025
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| Materias: | |
| Acceso en línea: | Ver este registro en EBSCOhost |
| fields | @attributes: recordID: 1 pdfLink: plink: https://search.ebscohost.com/login.aspx?direct=true&db=ssf&AN=193377505&site=ehost-live header: @attributes: shortDbName: ssf uiTerm: 193377505 longDbName: Social Sciences Full Text (H.W. Wilson) uiTag: AN controlInfo: bkinfo: jinfo: jid: B0JA jtl: Journal of the Utah Academy of Sciences, Arts & Letters maglogo: N pubinfo: dt: 2025 vid: 102 pid: 59066 pub: Utah Academy of Sciences, Arts & Letters artinfo: ui: 193377505 ppf: 379 ppct: 0 formats: fmt: @attributes: type: P size: 269KB tig: atl: Gravitational Tidal Deformations of Rotating Black Holes. aug: au: Glazer, Daniel Joyce, Austin Rodriguez, Maria J. Santoni, Luca Solomon, Adam R. Temoche, Luis Fernando affil: Utah State University. su: Black holes Kerr black holes Physical constants Spacetime sug: subj: Black holes Kerr black holes Physical constants Spacetime ab: Black holes are influenced by external gravitational fields in the universe, which are generated by other astrophysical objects in their surroundings. Because of this gravitational interaction, they experience tidal deformations of their event horizons. To quantify this effect, we compute the so-called Love numbers, which measure the deformability of the event horizon. Theoretical results from several authors have shown that Love numbers vanish for black hole solutions in four-dimensional spacetime. But does this behavior persist for black hole solutions in higher-dimensional spacetimes? In our presentation, we aim to address this question by demonstrating that, unlike their lower-dimensional counterparts, higher-dimensional rotating black holes exhibit nonvanishing Love numbers. pubtype: Academic Journal doctype: Article src: R language: English refInfo: copyright: @attributes: flag: N holdings: @attributes: islocal: N |
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