Strong Gravity News & Events
Tübingen Einstein Seminar
C. Herdeiro was the invited speaker of the Tübingen Einstein seminar on April 16 2021.
Probing light axion-like particles with neutron star inspirals
Gravitational-wave imprints of non-integrable extreme-mass-ratio inspirals
Abstract: The detection of gravitational waves from extreme-mass-ratio inspirals (EMRIs) with upcoming space-borne detectors will allow for unprecedented tests of general relativity in the strong-field regime. Aside from assessing whether black holes are unequivocally described by the Kerr metric, they may place constraints on the degree of spacetime symmetry.
Black hole (de)scalarization in compact binaries
Discussion of the paper "An analytic representation for the quasi-normal modes of Kerr black holes" by E. W. Leaver
An analytic representation for the quasi-normal modes of Kerr black holes
E. W. Leaver
Proc. Roy. Soc. Lond. A 402 (1985) 285-298
Discussion of the paper "Thermodynamics of Black Holes in Anti-de Sitter Space" by S. W. Hawking and D. N. Page
Thermodynamics of Black Holes in Anti-de Sitter Space
S. W. Hawking and D. N. Page
Commun. Math. Phys. 87 (1983) 577-588
One year Post-Doctoral Grant in High Energy Physics
A call for a 1 year postdoctoral grant in High Energy Physics, within the research grant “From Higgs phenomenology to the unification of fundamental interactions", PTDC / FIS-PAR / 31000/2017, is open from the 19th of April to the 14th of May 2021. See the eracareers announcement (in Portuguese and English) here.
A Nobel Prize for Black Holes
Celebrating the 2020 Physics Nobel Prize for Black Holes, here is an outreach article published in Gazeta de Física (published by the Portuguese Physics Society) by C. Herdeiro. The article pdf can be found in attachment.
Quasinormal modes and their connection to black hole shadow
In this talk I will first review a few intriguing properties of black hole quasinormal modes in the eikonal limit or in the near extremal limit (for the black hole). After that I will show how to relate quasinormal modes to the black hole shadows, and how to formulate a test for such relation.
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