Testing the black hole 'no-hair' hypothesis
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Testing the black hole 'no-hair' hypothesis. / Cardoso, Vitor; Gualtieri, Leonardo.
I: Classical and Quantum Gravity, Bind 33, Nr. 17, 174001, 08.09.2016.Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt
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TY - JOUR
T1 - Testing the black hole 'no-hair' hypothesis
AU - Cardoso, Vitor
AU - Gualtieri, Leonardo
PY - 2016/9/8
Y1 - 2016/9/8
N2 - 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 gravitational window, and what it can possibly tell us about our Universe.
AB - 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 gravitational window, and what it can possibly tell us about our Universe.
KW - black holes
KW - general relativity
KW - observations of black holes
KW - gravitational waves
KW - tests of general relativity
KW - GENERAL-RELATIVISTIC MODELS
KW - MULTIPOLE MOMENTS
KW - GRAVITATIONAL-WAVES
KW - GALACTIC-CENTER
KW - BARYON NUMBER
KW - MASS
KW - KERR
KW - SCALAR
KW - FIELD
KW - NONMEASURABILITY
U2 - 10.1088/0264-9381/33/17/174001
DO - 10.1088/0264-9381/33/17/174001
M3 - Journal article
VL - 33
JO - Classical and Quantum Gravity
JF - Classical and Quantum Gravity
SN - 0264-9381
IS - 17
M1 - 174001
ER -
ID: 299821726