Nonlinear interactions between black holes and Proca fields

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Standard

Nonlinear interactions between black holes and Proca fields. / Zilhao, Miguel; Witek, Helvi; Cardoso, Vitor.

I: Classical and Quantum Gravity, Bind 32, Nr. 23, 234003, 02.12.2015.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Zilhao, M, Witek, H & Cardoso, V 2015, 'Nonlinear interactions between black holes and Proca fields', Classical and Quantum Gravity, bind 32, nr. 23, 234003. https://doi.org/10.1088/0264-9381/32/23/234003

APA

Zilhao, M., Witek, H., & Cardoso, V. (2015). Nonlinear interactions between black holes and Proca fields. Classical and Quantum Gravity, 32(23), [234003]. https://doi.org/10.1088/0264-9381/32/23/234003

Vancouver

Zilhao M, Witek H, Cardoso V. Nonlinear interactions between black holes and Proca fields. Classical and Quantum Gravity. 2015 dec. 2;32(23). 234003. https://doi.org/10.1088/0264-9381/32/23/234003

Author

Zilhao, Miguel ; Witek, Helvi ; Cardoso, Vitor. / Nonlinear interactions between black holes and Proca fields. I: Classical and Quantum Gravity. 2015 ; Bind 32, Nr. 23.

Bibtex

@article{67a08d0ddb08496ea57e46cdf6f97b2c,
title = "Nonlinear interactions between black holes and Proca fields",
abstract = "Physics beyond the standard model is an important candidate for dark matter, and an interesting testing ground for strong-field gravity: the equivalence principle 'forces' all forms of matter to fall in the same way, and it is therefore natural to look for imprints of these fields in regions with strong gravitational fields, such as compact stars or black holes (BHs). Here we study general relativity minimally coupled to a massive vector field, and how BHs in this theory lose 'hair'. Our results indicate that BHs can sustain Proca field condensates for extremely long time-scales.",
keywords = "black holes, (nonlinear) stability, numerical relativity, KLEIN-GORDON EQUATION, BARYON NUMBER, INITIAL DATA, ENERGY, NONEXISTENCE, EVOLUTION",
author = "Miguel Zilhao and Helvi Witek and Vitor Cardoso",
year = "2015",
month = dec,
day = "2",
doi = "10.1088/0264-9381/32/23/234003",
language = "English",
volume = "32",
journal = "Classical and Quantum Gravity",
issn = "0264-9381",
publisher = "Institute of Physics Publishing Ltd",
number = "23",

}

RIS

TY - JOUR

T1 - Nonlinear interactions between black holes and Proca fields

AU - Zilhao, Miguel

AU - Witek, Helvi

AU - Cardoso, Vitor

PY - 2015/12/2

Y1 - 2015/12/2

N2 - Physics beyond the standard model is an important candidate for dark matter, and an interesting testing ground for strong-field gravity: the equivalence principle 'forces' all forms of matter to fall in the same way, and it is therefore natural to look for imprints of these fields in regions with strong gravitational fields, such as compact stars or black holes (BHs). Here we study general relativity minimally coupled to a massive vector field, and how BHs in this theory lose 'hair'. Our results indicate that BHs can sustain Proca field condensates for extremely long time-scales.

AB - Physics beyond the standard model is an important candidate for dark matter, and an interesting testing ground for strong-field gravity: the equivalence principle 'forces' all forms of matter to fall in the same way, and it is therefore natural to look for imprints of these fields in regions with strong gravitational fields, such as compact stars or black holes (BHs). Here we study general relativity minimally coupled to a massive vector field, and how BHs in this theory lose 'hair'. Our results indicate that BHs can sustain Proca field condensates for extremely long time-scales.

KW - black holes

KW - (nonlinear) stability

KW - numerical relativity

KW - KLEIN-GORDON EQUATION

KW - BARYON NUMBER

KW - INITIAL DATA

KW - ENERGY

KW - NONEXISTENCE

KW - EVOLUTION

U2 - 10.1088/0264-9381/32/23/234003

DO - 10.1088/0264-9381/32/23/234003

M3 - Journal article

VL - 32

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

SN - 0264-9381

IS - 23

M1 - 234003

ER -

ID: 300071916