Black holes (BHs) in general relativity (GR) are very simple objects. This property, that goes under the name of ‘no-hair’, has been refined in the last few decades and admits several versions. The simplicity of BHs makes them ideal testbeds of fundamental physics and of GR itself. Here we discuss the no-hair property of BHs, how it can be measured in the electromagnetic or gravita- tional window, and what it can possibly tell us about our Universe.
Testing the black hole 'no-hair' hypothesis / Cardoso, Vitor; Gualtieri, Leonardo. - In: CLASSICAL AND QUANTUM GRAVITY. - ISSN 0264-9381. - STAMPA. - 33:17(2016), p. 174001. [10.1088/0264-9381/33/17/174001]
Testing the black hole 'no-hair' hypothesis
GUALTIERI, Leonardo
2016
Abstract
Black holes (BHs) in general relativity (GR) are very simple objects. This property, that goes under the name of ‘no-hair’, has been refined in the last few decades and admits several versions. The simplicity of BHs makes them ideal testbeds of fundamental physics and of GR itself. Here we discuss the no-hair property of BHs, how it can be measured in the electromagnetic or gravita- tional window, and what it can possibly tell us about our Universe.| File | Dimensione | Formato | |
|---|---|---|---|
|
Cardoso_Testing the black hole_2016.pdf
solo gestori archivio
Tipologia:
Versione editoriale (versione pubblicata con il layout dell'editore)
Licenza:
Tutti i diritti riservati (All rights reserved)
Dimensione
3.98 MB
Formato
Adobe PDF
|
3.98 MB | Adobe PDF | Contatta l'autore |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
