Extremal black holes in dynamical Chern–Simons gravity

Robert J. McNees; Robert J. McNees; Leo C. Stein; Nicolás Yunes; Nicolás Yunes

doi:10.1088/0264-9381/33/23/235013

Extremal black holes in dynamical Chern–Simons gravity

Robert J. McNees
, Robert J. McNees
, Leo C. Stein
, Nicolás Yunes
, Nicolás Yunes

Department of Physics

Kavli Institute for Theoretical Physics
California Institute of Technology
Montana State University

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	Classical and Quantum Gravity
Volume	33
Issue number	23
DOIs	https://doi.org/10.1088/0264-9381/33/23/235013
State	Published - Nov 8 2016

Disciplines

Applied Mathematics
Physics

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@article{a4efde0908d9410e8eaba86daf96b264,

title = "Extremal black holes in dynamical Chern–Simons gravity",

author = "McNees, \{Robert J.\} and McNees, \{Robert J.\} and Stein, \{Leo C.\} and Nicol{\'a}s Yunes and Nicol{\'a}s Yunes",

note = "Rapidly rotating black hole (BH) solutions in theories beyond general relativity (GR) play a key role in experimental gravity, as they allow us to compute observables in extreme spacetimes that deviate from the predictions of GR. Such solutions are often difficult to find in beyond-general-relativity theories due to the inclusion of additional fields that couple to the metric nonlinearly and non-minimally.",

year = "2016",

month = nov,

day = "8",

doi = "10.1088/0264-9381/33/23/235013",

language = "American English",

volume = "33",

journal = "Classical and Quantum Gravity",

issn = "1361-6382",

number = "23",

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TY - JOUR

T1 - Extremal black holes in dynamical Chern–Simons gravity

AU - McNees, Robert J.

AU - Stein, Leo C.

AU - Yunes, Nicolás

N1 - Rapidly rotating black hole (BH) solutions in theories beyond general relativity (GR) play a key role in experimental gravity, as they allow us to compute observables in extreme spacetimes that deviate from the predictions of GR. Such solutions are often difficult to find in beyond-general-relativity theories due to the inclusion of additional fields that couple to the metric nonlinearly and non-minimally.

PY - 2016/11/8

Y1 - 2016/11/8

UR - http://ui.adsabs.harvard.edu/abs/2016CQGra..33w5013M/abstract

U2 - 10.1088/0264-9381/33/23/235013

DO - 10.1088/0264-9381/33/23/235013

M3 - Article

SN - 1361-6382

VL - 33

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 23

ER -

Extremal black holes in dynamical Chern–Simons gravity

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