PIRSA:15030115

Kerr black holes with scalar hair

APA

Herdeiro, C. (2015). Kerr black holes with scalar hair. Perimeter Institute for Theoretical Physics. https://pirsa.org/15030115

MLA

Herdeiro, Carlos. Kerr black holes with scalar hair. Perimeter Institute for Theoretical Physics, Mar. 05, 2015, https://pirsa.org/15030115

BibTex

          @misc{ scivideos_PIRSA:15030115,
            doi = {10.48660/15030115},
            url = {https://pirsa.org/15030115},
            author = {Herdeiro, Carlos},
            keywords = {Strong Gravity},
            language = {en},
            title = {Kerr black holes with scalar hair},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2015},
            month = {mar},
            note = {PIRSA:15030115 see, \url{https://scivideos.org/pirsa/15030115}}
          }
          

Carlos Herdeiro Universidad de Aveiro

Talk numberPIRSA:15030115
Source RepositoryPIRSA
Collection

Abstract

The Kerr metric of vacuum general relativity is expected to describe astrophysical black holes. Boson stars, on the other hand, are one of the simplest gravitating solitons, suggested as astrophysical compact objects, black holes mimickers and as dark matter candidates. Kerr black holes with scalar hair, found in [1], continuously interpolate between these two types of, per se, physically interesting solutions. I will describe the construction of these solutions and discuss theoretical, astrophysical and high energy physics aspects and challenges for Kerr black holes with scalar hair.

References:

[1] Kerr black holes with scalar hair, Carlos A. R. Herdeiro, Eugen Radu, Phys. Rev. Lett. 112 (2014) 221101; e-Print: arXiv:1403.2757

[2] A new spin on black hole hair, C. Herdeiro, E. Radu, International Journal of Modern Physics D 23 (2014) 1442014; e-Print: arXiv: 1405.3696;

[3] Construction and physical properties of Kerr black holes with scalar hair, C. Herdeiro and E. Radu, arXiv:1501.04319 [gr-qc]; Focus Issue on "Black holes and fundamental fields" to appear in Classical and Quantum Gravity