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18 papers · 2 filters
Consistency of matter coupling in modified gravity
Kazufumi Takahashi, Rampei Kimura, Hayato Motohashi
Matter coupling in modified gravity theories is a nontrivial issue when the gravitational Lagrangian possesses a degeneracy structure to avoid the problem of the Ostrogradsky ghost…
Cosmological stability in gravity
Shinji Tsujikawa
In gravitational theories where a canonical scalar field with a potential is coupled to a Gauss-Bonnet (GB) term with the Lagrangian , we study…
Spin-2 dark matter from anisotropic Universe in bigravity
Yusuke Manita, Katsuki Aoki, Tomohiro Fujita +1
Bigravity is one of the natural extensions of general relativity and contains an additional massive spin-2 field which can be a good candidate for dark matter. To discuss the produ…
Gravitational collapse and formation of a black hole in a type II minimally modified gravity theory
Antonio De Felice, Kei-ichi Maeda, Shinji Mukohyama +1
We study the spherically symmetric collapse of a cloud of dust in VCDM, a class of gravitational theories with two local physical degrees of freedom. We find that the collapse corr…
How does SU()-natural inflation isotropize the universe?
Tomoaki Murata, Tomohiro Fujita, Tsutomu Kobayashi
We study the homogeneous and anisotropic dynamics of pseudoscalar inflation coupled to an SU() gauge field. To see how the initially anisotropic universe is isotropized in such…
Cosmology in theories with spontaneous scalarization of neutron stars
Ratchaphat Nakarachinda, Sirachak Panpanich, Shinji Tsujikawa +1
In a model of spontaneous scalarization of neutron stars proposed by Damour and Esposite-Farese, a general relativistic branch becomes unstable to trigger tachyonic growth of a sca…
Inspiral gravitational waveforms from compact binary systems in Horndeski gravity
Yurika Higashino, Shinji Tsujikawa
In a subclass of Horndeski theories with the speed of gravity equivalent to that of light, we study gravitational radiation emitted during the inspiral phase of compact binary syst…
Symmetry restoration in the vicinity of neutron stars with a nonminimal coupling
Masato Minamitsuji, Shinji Tsujikawa
We propose a new model of scalarized neutron stars (NSs) realized by a self-interacting scalar field nonminimally coupled to the Ricci scalar of the form . The scala…
Hamiltonian formulation and loop quantization of a recent extension of the Kruskal spacetime
Beatriz Elizaga Navascués, Alejandro García-Quismondo, Guillermo A. Mena Marugán
We study the Hamiltonian formulation of the Ashtekar-Olmedo-Singh model for the description of the interior geometry of non-rotating, uncharged black holes. This model incorporates…
Stability of neutron stars in Horndeski theories with Gauss-Bonnet couplings
Masato Minamitsuji, Shinji Tsujikawa
In Horndeski theories containing a scalar coupling with the Gauss-Bonnet (GB) curvature invariant , we study the existence and linear stability of neutron star (NS) s…
Space of solutions of the Ashtekar-Olmedo-Singh effective black hole model
Beatriz Elizaga Navascués, Alejandro García-Quismondo, Guillermo A. Mena Marugán
We consider a general choice of integration constants in the resolution of the dynamical equations derived from a recently proposed effective model that describes black hole spacet…
On the stability of covariant BSSN formulation
Ryosuke Urakawa, Takuya Tsuchiya, Gen Yoneda
In this study, we investigate the numerical stability of the covariant BSSN (cBSSN) formulation proposed by Brown. We calculate the constraint amplification factor (CAF), which is…
Instability of hairy black holes in regularized 4-dimensional Einstein-Gauss-Bonnet gravity
Shinji Tsujikawa
In regularized 4-dimensional Einstein-Gauss-Bonnet (EGB) gravity derived from a Kaluza-Klein reduction of higher-dimensional EGB theory, we study the existence and stability of bla…
Linear stability of black holes with static scalar hair in full Horndeski theories: generic instabilities and surviving models
Masato Minamitsuji, Kazufumi Takahashi, Shinji Tsujikawa
In full Horndeski theories, we show that the static and spherically symmetric black hole (BH) solutions with a static scalar field~ whose kinetic term~ is nonvanishing on the…
VCDM and Cuscuton
Antonio De Felice, Kei-ichi Maeda, Shinji Mukohyama +1
We investigate two Type-IIa Minimally Modified Gravity theories, namely VCDM and Cuscuton theories. We confirm that all acceptable Cuscuton solutions are always solutions for VCDM…
Stable numerical simulation of Einstein equations in gravitational collapse space--time
Takuya Tsuchiya, Ryosuke Urakawa, Gen Yoneda
We perform simulations in a gravitational collapsing model using the Einstein equations. In this paper, we review the equations for constructing the initial values and the evolutio…
Cuscuta-Galileon cosmology: Dynamics, gravitational "constant"s and the Hubble Constant
Kei-ichi Maeda, Sirachak Panpanich
We discuss cosmology based on a Cuscuta-Galileon gravity theory, which preserves just two degrees of freedom. Although there exists no additional degrees of freedom, introduction o…
Linear stability of black holes in shift-symmetric Horndeski theories with a time-independent scalar field
Masato Minamitsuji, Kazufumi Takahashi, Shinji Tsujikawa
We study linear perturbations about static and spherically symmetric black holes with a time-independent background scalar field in shift-symmetric Horndeski theories, whose Lagran…