Testing the black hole 'no-hair' hypothesis

Research output: Contribution to journal › Journal article › Research › peer-review

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Testing the black hole 'no-hair' hypothesis. / Cardoso, Vitor; Gualtieri, Leonardo.

In: Classical and Quantum Gravity, Vol. 33, No. 17, 174001, 08.09.2016.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Cardoso, V & Gualtieri, L 2016, 'Testing the black hole 'no-hair' hypothesis', Classical and Quantum Gravity, vol. 33, no. 17, 174001. https://doi.org/10.1088/0264-9381/33/17/174001

APA

Cardoso, V., & Gualtieri, L. (2016). Testing the black hole 'no-hair' hypothesis. Classical and Quantum Gravity, 33(17), [174001]. https://doi.org/10.1088/0264-9381/33/17/174001

Vancouver

Cardoso V, Gualtieri L. Testing the black hole 'no-hair' hypothesis. Classical and Quantum Gravity. 2016 Sep 8;33(17). 174001. https://doi.org/10.1088/0264-9381/33/17/174001

Author

Cardoso, Vitor ; Gualtieri, Leonardo. / Testing the black hole 'no-hair' hypothesis. In: Classical and Quantum Gravity. 2016 ; Vol. 33, No. 17.

Bibtex

@article{fd53912514ef4a80ade455c8c8aba029,
title = "Testing the black hole 'no-hair' hypothesis",
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 gravitational window, and what it can possibly tell us about our Universe.",
keywords = "black holes, general relativity, observations of black holes, gravitational waves, tests of general relativity, GENERAL-RELATIVISTIC MODELS, MULTIPOLE MOMENTS, GRAVITATIONAL-WAVES, GALACTIC-CENTER, BARYON NUMBER, MASS, KERR, SCALAR, FIELD, NONMEASURABILITY",
author = "Vitor Cardoso and Leonardo Gualtieri",
year = "2016",
month = sep,
day = "8",
doi = "10.1088/0264-9381/33/17/174001",
language = "English",
volume = "33",
journal = "Classical and Quantum Gravity",
issn = "0264-9381",
publisher = "Institute of Physics Publishing Ltd",
number = "17",

}

RIS

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