• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Nathaniel A Strauss, Bernard F Whiting and Anne T Franzen

We extend the discussion of the antipodal identification of black holes to the Reissner–Nordström (RN) spacetime by developing the classical tools necessary to define the corresponding quantum field theory (QFT). We solve the massless Klein–Gordon equation in the RN background in terms of scattering coefficients and provide a procedure for constructing a solution for an arbitrary analytic extension

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Fernando Abalos and Oscar Reula

In this work, we study constant-coefficient first order systems of partial differential equations and give necessary and sufficient conditions for those systems to have a well-posed Cauchy problem. In many physical applications, due to the presence of constraints, the number of equations in the PDE system is larger than the number of unknowns, thus the standard Kreiss conditions can not be directly

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Sara Rezvanjou, Reza Saffari, Mozhgan Masoudi and Saheb Soroushfar

In this paper, some dynamical properties of neutral and charged particles around a weakly magnetized five-dimensional static black string have been studied. The perturbation method was also used to calculate the innermost stable circular orbit (ISCO) of this metric in the presence of a magnetic field. The escape velocity of neutral and charged particles around the black string was derived. In the next

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Joan Josep Ferrando and Juan Antonio Sáez

The necessary and sufficient conditions for a three-dimensional Riemannian metric to admit a transitive group of isometries are obtained. These conditions are intrinsic, deductive, explicit and algorithmic, and they offer an IDEAL labeling of these geometries. It is shown that the transitive action of the group naturally falls into an unfolding of some of the ten types in the Bianchi–Behr classification

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Christian G Böhmer and Franco Fiorini

The regular black hole solution arising as a spherically symmetric vacuum solution of Born–Infeld gravity possesses an asymptotic interior structure which is very well described by a four-dimensional generalization of the non-rotating BTZ metric. According to this picture no singularity exists, and instead, infalling observers experience a constant curvature manifold as they travel towards future null

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Arthur George Suvorov

The set of all metrics that can be placed on a given manifold defines an infinite-dimensional ‘superspace’ that can itself be imbued with the structure of a Riemannian manifold. Geodesic distances between points on Met( M ) measure how close two different metrics over M are to one another. Restricting our attention to only those metrics that describe physical black holes, these distances may therefore

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Jose Queiruga

We describe a spacetime endowed with a non-metricity tensor which effectively serves as a model of a spacetime foam. We explore the consequences of the non-metricity in several f ( R ) theories.

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Marcin Kisielowski

Recently, a new class of scalar constraint operators has been introduced in loop quantum gravity. They are defined on a space of solutions to the Gauss constraint and partial solutions to the vector constraint, called a vertex Hilbert space. We propose a subspace of the vertex Hilbert space formed by homogeneous-isotropic states, which is invariant under the action of the new scalar constraint operators

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
J R B Peleteiro and C E Valcárcel

Mielke–Baekler gravity consists in the usual Einstein–Hilbert action with a cosmological term and rotational and translational Chern–Simons terms with arbitrary couplings. For a particular choice of these couplings, we can obtain Einstein–Hilbert action, its teleparallel equivalent and the exotic Witten’s gravity. In this work, we use the Chern–Simons formalism to generalize the three dimensional Mielke–Baekler

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-11
Norbert Bodendorfer and Dennis Wuhrer

We present an analytic computation of an explicit renormalisation group flow for cosmological states in loop quantum gravity. A key ingredient in our analysis are Perelomov coherent states for the Lie group SU(1, 1) whose representation spaces are embedded into the standard loop quantum cosmology (LQC) Hilbert space. The SU(1, 1) group structure enters our analysis by considering a classical set of

更新日期：2020-08-12
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-09
S Habib Mazharimousavi and M Halilsoy

We consider the pure electric type power-law Lagrangian in nonlinear electrodynamics theory of dimensions n + 1. Conformally flat form of Bertotti–Robinson type spacetimes are obtained in all these dimensions with the specific power ##IMG## [http://ej.iop.org/images/0264-9381/37/17/177001/cqgaba222ieqn1.gif] {$s=-\frac{1}{n-4}$} , which naturally excludes n = 4. This particular dimension is considered

更新日期：2020-08-10
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
C Stachie, T Dal Canton, E Burns, N Christensen, R Hamburg, M Briggs, J Broida, A Goldstein, F Hayes, T Littenberg, P Shawhan, J Veitch, P Veres and C A Wilson-Hodge

Presented is the description of a new and general method used to search for γ-ray counterparts to gravitational-wave (GW) triggers. This method is specifically applied to single GW detector triggers. Advanced LIGO data from observing runs O1 and O2 were analyzed, thus each GW trigger comes from either the LIGO-Livingston or the LIGO-Hanford interferometer. For each GW trigger, Fermi Gamma-ray burst

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
Zhiming Huang, Haozhen Situ and Zhimin He

We analyze the quantum Fisher information (QFI) for a particle detector coupled to a thermal electromagnetic field in the cosmic string spacetime. It is found that vacuum fluctuation, temperature, detector polarization and nontrivial spacetime topology affect the QFI. Vacuum fluctuation and temperature degrade QFI. When deficit angle parameter ν = 1 and detector is far away from the string, the results

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
Alexandru Dima and Enrico Barausse

Photons propagating in a plasma acquire an effective mass μ , which is given by the plasma frequency and which scales with the square root of the plasma density. As noted previously in the literature, for electron number densities n e ∼ 10 −3 cm −3 (such as those measured in the interstellar medium) the effective mass induced by the plasma is μ ∼ 10 −12 eV. This would cause superradiant instabilities

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
Ángel Rincón and J R Villanueva

In this paper, we investigate the Sagnac effect by calculating the difference in travel time and phase shift observed for photon beams counter-propagating in a rotating interferometer on a BTZ black hole solution in the context of scale-dependent gravity, which describes the field around a massive static and rotating object in 2 + 1 gravity.

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
Jorge G Russo

In presence of magnetic fields, the orbits of charged particles can be displaced from the equatorial plane. We study circular orbits of electrically charged massive objects around a magnetic black hole in the probe approximation. We show that there exist a one-parameter family of circular orbits at constant polar angle θ and constant radius r , parameterized by the angular momentum. The angle θ can

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
Koray Düztaş, Mubasher Jamil, Sanjar Shaymatov and Bobomurat Ahmedov

We test the validity of the weak cosmic censorship conjecture for the (2 + 1)-dimensional charged anti-de Sitter black hole solution, which was derived by Martinez et al (MTZ). We first construct a thought experiment by throwing test charged particles on an extremal MTZ black hole. We derive that extremal (2 + 1) dimensional black holes can be overcharged by test particles, unlike their analogues in

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
G Hörmann, Y Sanchez Sanchez, C Spreitzer and J A Vickers

In this paper we develop the mathematics required in order to provide a description of the observables for quantum fields on low-regularity spacetimes. In particular we consider the case of a massless scalar field ϕ on a globally hyperbolic spacetime M with C 1,1 metric g . This first entails showing that the (classical) Cauchy problem for the wave equation is well-posed for initial data and sources

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
Barrett M Frank, Brandon Piotrzkowski, Brett Bolen, Marco Cavaglià and Shane L Larson

One source of noise for the laser interferometer space antenna (LISA) will be time-varying changes of the space environment in the form of solar wind particles and photon pressure from fluctuating solar irradiance. The approximate magnitude of these effects can be estimated from the average properties of the solar wind and the solar irradiance. We use data taken by the ACE (advanced Compton explorer)

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-08-04
A Biswas, J McIver and A Mahabal

A network of three or more gravitational wave detectors simultaneously taking data is required to generate a well-localized sky map for gravitational wave sources, such as GW170817. Local seismic disturbances often cause the LIGO and Virgo detectors to lose light resonance in one or more of their component optic cavities, and the affected detector is unable to take data until resonance is recovered

更新日期：2020-08-05
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-29
Hing-Tong Cho and Kin-Wang Ng

In this work we study the effects of the electromagnetic coupling in natural inflation in a systematic manner using the Schwinger–Keldysh formalism. The corresponding influence functional is evaluated in the one-loop level. It can be interpreted as due to a single stochastic force. The equation of motion of the inflaton field is therefore given in the form of a Langevin equation. Lastly, the two-point

更新日期：2020-07-30
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Blake Moore and Nicolás Yunes

Gravitational waves allow us to test general relativity in the highly dynamical regime. While current observations have been consistent with waves emitted by quasi-circular binaries, eccentric binaries may also produce detectable signals in the near future with ground- and space-based detectors. We here explore how tests of general relativity scale with the orbital eccentricity of the source during

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Mikica Kocic, Francesco Torsello, Marcus Högås and Edvard Mörtsell

We present a method for solving the constraint equations in the Hassan–Rosen bimetric theory to determine the initial data for the gravitational collapse of spherically symmetric dust. The setup leads to equations similar to those for a polytropic fluid in general relativity, here called Lane–Emden-like equations. Using a numerical code which solves the evolution equations in the standard 3 + 1 form

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
R X Adhikari, K Arai, A F Brooks, C Wipf, O Aguiar, P Altin, B Barr, L Barsotti, R Bassiri, A Bell, G Billingsley, R Birney, D Blair, E Bonilla, J Briggs, D D Brown, R Byer, H Cao, M Constancio, S Cooper, T Corbitt, D Coyne, A Cumming, E Daw, R deRosa, G Eddolls, J Eichholz, M Evans, M Fejer, E C Ferreira, A Freise, V V Frolov, S Gras, A Green, H Grote, E Gustafson, E D Hall, G Hammond, J Harms, G

The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravitational wave astronomy, revealing a previously hidden side of the cosmos. To maximize the reach of the existing LIGO observatory facilities, we have designed a new instrument able to detect gravitational waves at distances 5 times further away than possible with Advanced LIGO, or at greater than 100

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Richard Lieu and Kristen A Lackeos

The Gaussian phase noise of intensity time series is demonstrated to be drastically reduced when the raw voltage data are digitally filtered through an arbitrarily large number n of orthornormal bandpass profiles (eigen-filters) sharing the same intensity bandwidth, and the resulting intensity series are co-added. Specifically, the relative noise variance of the summed series at the resolution of one

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28

We analyze the asymptotic symmetries and their associated charges at spatial infinity in four-dimensional asymptotically-flat spacetimes. We use the covariant formalism of Ashtekar and Hansen where the asymptotic fields and symmetries live on the three-manifold of spatial directions at spatial infinity, represented by a timelike unit-hyperboloid (or de Sitter space). Using the covariant phase space

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Celia Escamilla-Rivera and Jackson Levi Said

In this work we present a further investigation about teleparallel gravity cosmology. We demonstrate that according to the current astrophysical data (CC + Pantheon + BAO samplers with late Universe measurements SH0ES + H0LiCOW), an f ( T , B ) theory can provide another interpretation to the oscillatory behaviour of the dark energy equation of state when applied to late times. The four f ( T , B )

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Lin Zhang and Xiaoning Wu

In this paper, we study the initial-boundary problem of the massive wave equation which is conformal regular on an asymptotically anti-de Sitter spacetime, where the initial-boundary data are given on an outgoing null hypersurface and a timelike hypersurface, and the asymptotic information is given on the future null infinity. After a conformal rescaling, this problem will reduce to a null-timelike

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
S P Miao, L Tan and R P Woodard

Cosmological Coleman–Weinberg potentials are induced when normal matter is coupled to the inflaton. It has long been known that the corrections from bosonic fields are positive whereas those from fermionic fields are negative. In flat space both take the form ± φ 4 ln( φ ), and they can be made to cancel by appropriately choosing the coupling constants. In an expanding Universe the bosonic and fermionic

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Atsushi Higuchi and Lasse Schmieding

It is well known that linearized gravity in spacetimes with compact Cauchy surfaces and continuous symmetries suffers from linearization instabilities: solutions to classical linearized gravity in such a spacetime must satisfy so-called linearization stability conditions (or constraints) for them to extend to solutions in the full non-linear theory. Moncrief investigated implications of these conditions

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Asta Heinesen and Thomas Buchert

Recently it has been noted by Di Valentino, Melchiorri and Silk (2019) that the enhanced lensing signal relative to that expected in the spatially flat ΛCDM model poses a possible crisis for the Friedmann–Lemaître–Robertson–Walker (FLRW) class of models usually used to interpret cosmological data. The ‘crisis’ amounts to inconsistencies between cosmological datasets arising when the FLRW curvature

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-28
Steffen Gielen and Axel Polaczek

We extend various recent results regarding the derivation of effective cosmological Friedmann equations from the dynamics of group field theory (GFT). Restricting ourselves to a single GFT field mode (or fixed values of Peter–Weyl representation labels), we first consider dynamics given by a quadratic Hamiltonian, which takes the form of a squeezing operator, and then add a quartic interaction that

更新日期：2020-07-29
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-16
Károly Csukás and István Rácz

Systematic numerical investigations of the asymptotics of near Schwarzschild vacuum initial data sets is carried out by inspecting solutions to the parabolic–hyperbolic and to the algebraic–hyperbolic forms of the constraints, respectively. One of our most important findings is that the concept of near Schwarzschild configurations, applied previously in [4, 5], is far too restrictive. It is demonstrated

更新日期：2020-07-17
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-15
Julian Adamek, Cristian Barrera-Hinojosa, Marco Bruni, Baojiu Li, Hayley J Macpherson and James B Mertens

A number of codes for general-relativistic simulations of cosmological structure formation have been developed in recent years. Here we demonstrate that a sample of these codes produce consistent results beyond the Newtonian regime. We simulate solutions to Einstein’s equations dominated by gravitomagnetism—a vector-type gravitational field that does not exist in Newtonian gravity and produces frame-dragging

更新日期：2020-07-16
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-12
Thiago Guerreiro

We discuss the quantum mechanical description of a gravitational wave interacting with a cavity electromagnetic field. Quantum fluctuations of the gravitational vacuum induce squeezing in the optical field. Moreover, this squeezing experiences revivals, a purely quantum effect. Measuring these gravitationally induced revivals, although out of reach from experiments, would provide evidence on the quantum

更新日期：2020-07-13
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-12
Fay Dowker and Rafael D Sorkin

We offer further evidence that discreteness of the sort inherent in a causal set cannot, in and of itself, serve to break Poincaré invariance. In particular we prove that a Poisson sprinkling of Minkowski spacetime cannot endow spacetime with a distinguished spatial or temporal orientation, or with a distinguished lattice of spacetime points, or with a distinguished lattice of timelike directions (corresponding

更新日期：2020-07-13
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-09
Justin L Ripley and Frans Pretorius

We report on a numerical investigation of black hole evolution in an Einstein dilaton Gauss–Bonnet (EdGB) gravity theory where the Gauss–Bonnet coupling and scalar (dilaton) field potential are symmetric under a global change in sign of the scalar field (a ‘ ##IMG## [http://ej.iop.org/images/0264-9381/37/15/155003/cqgab9bbbieqn2.gif] {${\mathbb{Z}}_{2}$} ’ symmetry). We find that for sufficiently small

更新日期：2020-07-10
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-09
Christopher Evans, Deborah Ferguson, Bhavesh Khamesra, Pablo Laguna and Deirdre Shoemaker

A popular approach in numerical simulations of black hole binaries is to model black holes as punctures in the fabric of spacetime. The location and the properties of the black hole punctures are tracked with apparent horizons, namely outermost marginally outer trapped surfaces (MOTSs). As the holes approach each other, a common apparent horizon suddenly appears, engulfing the two black holes and signaling

更新日期：2020-07-10
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-09
Viqar Husain and Suprit Singh

We present a study of the evolution of entanglement entropy of matter and geometry in quantum cosmology. For a variety of Gaussian initial states and their linear combinations, and with evolution defined with respect to a relational time, we show numerically that (i) entanglement entropy increases rapidly at very early times, and subsequently saturates to a constant non-zero value, and (ii) that the

更新日期：2020-07-10
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-09
John Ryan Westernacher-Schneider, Charalampos Markakis and Bing Jyun Tsao

The dynamics of self-gravitating fluid bodies is described by the Euler–Einstein system of partial differential equations. The break-down of well-posedness on the fluid–vacuum interface remains a challenging open problem, which is manifested in simulations of oscillating or inspiraling binary neutron-stars. We formulate and implement a well-posed canonical hydrodynamic scheme, suitable for neutron-star

更新日期：2020-07-10
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-09
Ernesto Contreras, Francisco Tello-Ortiz and S K Maurya

We implement the gravitational decoupling through the minimal geometric deformation method and explore its effect on exterior solutions by imposing a regularity condition in the Tolman–Oppenheimer–Volkoff equation of the decoupling sector. We obtain that the decoupling function can be expressed formally in terms of an integral involving the g tt component of the metric of the seed solution. As a particular

更新日期：2020-07-10
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-09
Massimo Blasone, Gaetano Lambiase, Giuseppe Gaetano Luciano, Luciano Petruzziello and Luca Smaldone

We derive the Mandelstam–Tamm time–energy uncertainty relation for neutrino oscillations in a generic stationary curved spacetime. In particular, by resorting to Stodolsky covariant formula of the quantum mechanical phase, we estimate gravity effects on the neutrino energy uncertainty. Deviations from the standard Minkowski result are explicitly evaluated in Schwarzschild, Lense–Thirring and Rindler

更新日期：2020-07-10
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-08
Miguel Duarte and David Hilditch

For mathematical convenience initial data sets in numerical relativity are often taken to be conformally flat. Employing the dual-foliation formalism, we investigate the physical consequences of this assumption. Working within a large class of asymptotically flat spacetimes we show that the ADM linear momentum is governed by the leading Lorentz part of a boost even in the presence of supertranslation-like

更新日期：2020-07-09
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-06
Patrick Chi-Kit Cheong, Lap-Ming Lin and Tjonnie Guang Feng Li

We present a new open-source axisymmetric general relativistic hydrodynamics code Gmunu ( g eneral-relativistic mu ltigrid nu merical solver) which uses a multigrid method to solve the elliptic metric equations in the conformally flat condition (CFC) approximation on a spherical grid. Most of the existing relativistic hydrodynamics codes are based on formulations which rely on a free-evolution approach

更新日期：2020-07-07
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-05
Luca Romano

We apply the Lie algebra expansion method to the ##IMG## [http://ej.iop.org/images/0264-9381/37/14/145016/cqgab8bbcieqn2.gif] {$\mathcal{N}=1$} super-Poincaré algerba in four dimensions. We define a set of p-brane projectors that induce a decomposition of the super-Poincaré algebra preparatory for the expansion. We show that starting from the ##IMG## [http://ej.iop.org/images/0264-9381/37/14/145016/cqgab8bbcieqn3

更新日期：2020-07-06
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
Rodolfo Gambini, Saeed Rastgoo and Jorge Pullin

In a previous paper, we showed how to use the techniques of the group of loops to formulate the loop approach to gravity proposed by Mandelstam in the 1960’s. Those techniques allow to overcome some of the difficulties that had been encountered in the earlier treatment. In this approach, gravity is formulated entirely in terms of Dirac observables without constraints, opening attractive new possibilities

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
Alejandra Castro and Beatrix Mühlmann

We revisit the holographic description of the near horizon geometry of the BTZ black hole in AdS 3 gravity, with a gravitational Chern–Simons term included. After a dimensional reduction of the three dimensional theory, we use the framework of nAdS 2 /nCFT 1 to describe the near horizon physics. This setup allows us to contrast the role of the gravitational and conformal anomaly inherited from AdS

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
Ben David Normann and Sigbjørn Hervik

What is the asymptotic future of a scalar-field model if the assumption of isotropy is relaxed in generic, homogeneous Universe models? This paper is a continuation of our previous work on Bianchi cosmologies with a p -form field (where p ∈ {1, 3})—or equivalently: an inhomogeneous, mass-less scalar gauge field with a homogeneous gradient. In this work we investigate such matter sector in general relativity

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
Brian C Seymour and Kent Yagi

Pulsar timing observations precisely test general relativity. Recently, the hierarchical triple system PSR J0337 + 1715 has placed new constraints on the existence of a fifth force from violation in the strong equivalence principle. Many alternative gravity theories exist with massive (pseudo-)scalar fields to explain a variety of phenomena from the accelerating expansion of the Universe at large scales

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
D Dalmazi and A L R dos Santos

Here we start from a dual version of Vasiliev’s first order action for massless spin-2 particles (linearized first order Einstein–Hilbert) and derive, via Kaluza–Klein dimensional reduction from D + 1 to D dimensions, a set of dual massive spin-2 models. This set includes the massive ‘BR’ model, a spin-2 analogue of the spin-1 Cremmer–Scherk model. In our approach the linearized Riemann curvature emerges

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
Marcus Högås, Mikica Kocic, Francesco Torsello and Edvard Mörtsell

In general relativity, the endpoint of spherically symmetric gravitational collapse is a Schwarzschild–[(A)dS] black hole. In bimetric gravity, it has been speculated that a static end state must also be Schwarzschild–[(A)dS]. To this end, we present a set of exact solutions, including collapsing massless dust particles. For these, the speculation is confirmed.

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
Alejandro Aguilar-Salas, Alberto Molgado and Efraín Rojas

The Hamilton–Jacobi formalism for a geodetic brane-like Universe described by the Regge–Teitelboim model is developed. We focus on the description of the complete set of Hamiltonians that ensure the integrability of the model in addition to obtaining the Hamilton principal function S . In order to do this, we avoid the second-order in derivative nature of the model by appropriately defining a set of

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-07-01
Muhammed Amir, Md Sabir Ali and Sunil D Maharaj

We derive a rotating counterpart of the five-dimensional electrically charged Bardeen regular black holes spacetime by employing the Giampieri algorithm on static one. The associated nonlinear electrodynamics source is computed in order to justify the rotating solution. We thoroughly discuss the energy conditions and the other properties of the rotating spacetime. The black hole thermodynamics of the

更新日期：2020-07-02
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-06-30
Jian Wang and Yu-Xiao Liu

In this paper, we adopt the method of quantum fields in curved spacetime to quantize a free scalar matter field in the braneworld background whose warped factor is of the form that could generate Pöschl–Teller potential. Then we consider the interaction between the scalar field ϕ ( x ) and a classical scalar source ρ ( x ) with the form ##IMG## [http://ej.iop.org/images/0264-9381/37/14/145009/cqgab971bieqn1

更新日期：2020-07-01
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-06-30
Alessandro Longo, Stefano Bianchi, Wolfango Plastino, Nicolas Arnaud, Antonino Chiummo, Irene Fiori, Bas Swinkels and Michal Was

A methodology of adaptive time series analysis, based on empirical mode decomposition (EMD) and on its time varying version tvf-EMD, has been applied to strain data from the gravitational wave interferometer (IFO) Virgo in order to characterise scattered light noise affecting the sensitivity of the IFO in the detection frequency band. Data taken both during hardware injections, when a part of the IFO

更新日期：2020-07-01
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-06-24
Yujie Duan, Weiyu Hu, Ke Huang and Junji Jia

Geodesics of both lightrays and timelike particles with nonzero mass are deflected in a gravitational field. In this work we apply the perturbative method developed in reference [1] to compute the deflection angle of both null and timelike rays in the weak field limit for four spacetimes. We obtained the deflection angles for the Bardeen spacetime to the eleventh order of m / b where m is the ADM mass

更新日期：2020-06-25
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-06-24
Raúl Carballo-Rubio, Francesco Di Filippo, Stefano Liberati and Matt Visser

We present a geometric classification of all spherically symmetric spacetimes that could result from singularity regularization, using a kinematic construction that is both exhaustive and oblivious to the dynamics of the fields involved. Due to the minimal geometric assumptions underlying it, this classification encompasses virtually all modified gravity theories, and any theory of quantum gravity

更新日期：2020-06-25
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-06-24
Derek Davis, Laurel V White and Peter R Saulson

Advanced LIGO data contains numerous noise transients, or ‘glitches’, that have been shown to reduce the sensitivity of matched filter searches for gravitational waves from compact binaries. These glitches increase the rate at which random coincidences occur, which reduces the significance of identified gravitational-wave events. The presence of these transients has precipitated extensive work to establish

更新日期：2020-06-25
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-06-24
Daniel Molano, Fabián Darío Villalba, Leonardo Castañeda and Pedro Bargueño

Perturbative techniques are important for modified theories of gravity since they allow to calculate deviations from general relativity without recurring to exact solutions, which can be difficult to find. When applied to models such as f ( R ) gravity, these techniques introduce corrections in the field equations that involve higher order derivatives. Such corrections must be handled carefully to

更新日期：2020-06-25
• Classical Quant. Grav. (IF 3.071) Pub Date : 2020-06-24
Maarten van de Meent

We provide analytical closed form solutions for the parallel transport along a bound geodesic in Kerr spacetime. This can be considered the lowest order approximation for the motion of a spinning black hole in an extreme mass-ratio inspiral. As an illustration of the usefulness of our new found expressions we scope out the locations of spin–spin resonances in quasi-circular EMRIs. All solutions are

更新日期：2020-06-25
Contents have been reproduced by permission of the publishers.

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