Built on

H. Motohashi and M. Minamitsuji, “Exact black hole solutions in shift-symmetric quadratic degenerate higher-order scalar-tensor theories,” Phys. Rev. D 99
Original
1901
Earlier work this paper cites.
C. Charmousis, M. Crisostomi, R. Gregory, and N. Stergioulas, “Rotating Black Holes in Higher Order Gravity,” Phys. Rev. D100
Original
1903
Earlier work this paper cites.
K. Takahashi, H. Motohashi, and M. Minamitsuji, “Linear stability analysis of hairy black holes in quadratic degenerate higher-order scalar-tensor theories: Odd-parity perturbations,” Phys. Rev. D 100
Original
1904
Earlier work this paper cites.
M. Minamitsuji and J. Edholm, “Black hole solutions in shift-symmetric degenerate higher-order scalar-tensor theories,” Phys. Rev. D 100
Original
1907
Earlier work this paper cites.
C. Charmousis, M. Crisostomi, D. Langlois, and K. Noui, “Perturbations of a rotating black hole in DHOST theories,” Class. Quant. Grav. 36
Original
1907
Earlier work this paper cites.
C. de Rham and J. Zhang, “Perturbations of stealth black holes in degenerate higher-order scalar-tensor theories,” Phys. Rev. D 100
Original
1907
Earlier work this paper cites.
J. Ben Achour, H. Liu, and S. Mukohyama, “Hairy black holes in DHOST theories: Exploring disformal transformation as a solution-generating method,” JCAP 02
Original
1910
Earlier work this paper cites.
K. Van Aelst, E. Gourgoulhon, P. Grandcl/’ement, and C. Charmousis, “Hairy rotating black holes in cubic Galileon theory,” Class. Quant. Grav. 37
Original
1910
Earlier work this paper cites.
M. Minamitsuji and J. Edholm, “Black holes with a nonconstant kinetic term in degenerate higher-order scalar tensor theories,” Phys. Rev. D 101
Original
1912
Earlier work this paper cites.
G. Domènech, A. Naruko, M. Sasaki and C. Wetterich, “Could the black hole singularity be a field singularity?,” Int. J. Mod. Phys. D 29
Original
1912
Earlier work this paper cites.
M. A. Gorji, A. Allahyari, M. Khodadi and H. Firouzjahi, “Mimetic black holes,” Phys. Rev. D 101
Original
1912
Earlier work this paper cites.
H. Motohashi and S. Mukohyama, “Weakly-coupled stealth solution in scordatura degenerate theory,” JCAP 01
Original
1912
Earlier work this paper cites.
I. Fisher, “Scalar mesostatic field with regard for gravitational effects,” Zh. Eksp. Teor. Fiz. 18
1948
Earlier work this paper cites.
J. Ehlers, “Konstruktionen und Charakterisierung von Losungen der Einsteinschen Gravitationsfeldgleichungen,” other thesis, 1957
1957
Earlier work this paper cites.
R. A. Matzner and C. W. Misner, “Gravitational Field Equations for Sources with Axial Symmetry and Angular Momentum,” Phys. Rev. 154
1967
Earlier work this paper cites.
B. Carter, “Global structure of the Kerr family of gravitational fields,” Phys. Rev. 174
1968
Earlier work this paper cites.
A. Janis, D. Robinson and J. Winicour, “Comments on einstein scalar solutions,” Phys. Rev. 186
1969
Earlier work this paper cites.
B. Voorhees, “Static axially symmetric gravitational fields,” Phys. Rev. D 2
1970
Earlier work this paper cites.
R. P. Geroch, “A Method for generating new solutions of Einstein’s equation. 2,” J. Math. Phys. 13
1972
Earlier work this paper cites.
J. D. Bekenstein, “The Relation between physical and gravitational geometry,” Phys.Rev. D48
1993
Earlier work this paper cites.
D. Galtsov, A. Garcia, and O. Kechkin, “Symmetries of the stationary Einstein-Maxwell dilaton theory,” Class. Quant. Grav. 12
1995
Earlier work this paper cites.
G. Clement, “From Schwarzschild to Kerr: Generating spinning Einstein-Maxwell fields from static fields,” Phys. Rev. D 57
1998
Earlier work this paper cites.

Similar

H. Motohashi and T. Suyama, “Quantum Ostrogradsky theorem,” arXiv:2001.02483
Original
2001
Cited alongside, same era.
I. Bogush and D. Gal’tsov, “Generation of rotating solutions in Einstein-scalar gravity,” arXiv:2001.02936
Original
2001
Cited alongside, same era.
H. Motohashi and W. Hu, “Effective field theory of degenerate higher-order inflation,” Phys. Rev. D 101
Original
2002
Cited alongside, same era.
N. Arkani-Hamed, H.-C. Cheng, M. A. Luty, and S. Mukohyama, “Ghost condensation and a consistent infrared modification of gravity,” JHEP 05
2004
Cited alongside, same era.
K. Takahashi and H. Motohashi, “General Relativity solutions with stealth scalar hair in quadratic higher-order scalar-tensor theories,” JCAP 06

Then

J. Ben Achour, M. Crisostomi, K. Koyama, D. Langlois, K. Noui, and G. Tasinato, “Degenerate higher order scalar-tensor theories beyond Horndeski up to cubic order,” JHEP 12
Original
2016
Later among the works it cites.
M. Crisostomi, M. Hull, K. Koyama, and G. Tasinato, “Horndeski: beyond, or not beyond?,” JCAP 1603
Original
2016
Later among the works it cites.
M. Crisostomi, K. Koyama, and G. Tasinato, “Extended Scalar-Tensor Theories of Gravity,” JCAP 1604
Original
2016
Later among the works it cites.
E. Babichev, C. Charmousis, and A. Lehébel, “Black holes and stars in Horndeski theory,” Class. Quant. Grav. 33
Original
2016
Later among the works it cites.
E. Babichev, C. Charmousis, and A. Lehébel, “Asymptotically flat black holes in Horndeski theory and beyond,” JCAP 1704

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2020

On Rotating Black Holes in DHOST Theories

Achour, Jibril Ben, Liu, Hongguang, Motohashi, Hayato et al.

Understand

Using the disformal solution-generating method, we construct new axisymmetric solutions in Degenerate Higher Order Scalar Tensor (DHOST) theories.

The method consists in first considering a "seed" known solution in DHOST theories and then performing a disformal transformation of the metric to obtain a new solution.
In vacuum, the two solutions are equivalent but they become physically inequivalent when one considers coupling to matter.
In that way, we "disform" the stealth Kerr black hole solution and we obtain a first analytic rotating non-stealth solution in DHOST theories, while the associated scalar field is time-dependent with a constant kinetic density.