2020
DOI: 10.48550/arxiv.2005.10794
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Where is Love? Tidal deformability in the black hole compactness limit

Cecilia Chirenti,
Camilo Posada,
Victor Guedes

Abstract: One of the macroscopically measurable effects of gravity is the tidal deformability of astrophysical objects, which can be quantified by their tidal Love numbers. For planets and stars, these numbers measure the resistance of their material against the tidal forces, and the resulting contribution to their gravitational multipole moments. According to general relativity, deformed black holes, instead, show no addition to their gravitational multipole moments, and all of their Love numbers are zero. In this pape… Show more

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Cited by 4 publications
(14 citation statements)
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“…In this paper, we will review the main results of the tidal deformability of ultracompact Schwarzschild stars presented by Chirenti et al (2020). As an addition to those results, we will show that the tidal Love number k 2 for ultracompact Schwarzschild stars do not follow the 1/ log ξ proposed by (Cardoso et al, 2017), instead, we found that k 2 decays exponentially as a function of the compactness.…”
Section: Introductionmentioning
confidence: 72%
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“…In this paper, we will review the main results of the tidal deformability of ultracompact Schwarzschild stars presented by Chirenti et al (2020). As an addition to those results, we will show that the tidal Love number k 2 for ultracompact Schwarzschild stars do not follow the 1/ log ξ proposed by (Cardoso et al, 2017), instead, we found that k 2 decays exponentially as a function of the compactness.…”
Section: Introductionmentioning
confidence: 72%
“…The tidal Love number for constant-density stars, or Schwarzschild stars, was studied by (Damour and Nagar, 2009;Postnikov et al, 2010;Chan et al, 2015) and more recently by (Chirenti et al, 2020). The details of the computation were discussed in these papers so we refer the reader to those works.…”
Section: Schwarzschild Starsmentioning
confidence: 99%
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