We examine the continuum limit of the piecewise flat locally finite gravity model introduced by ’t Hooft. In the linear weak field limit, we find the energy–momentum tensor and metric perturbation of an arbitrary configuration of defects. The energy–momentum turns out to be restricted to satisfy certain conditions. The metric perturbation is mostly fixed by the energy–momentum except for its lightlike modes which reproduce linear gravitational waves, despite no such waves being present at the microscopic level
We study the plane (not necessarily monochromatic) gravitational waves at nonlinear quadratic order ...
The energy density " g of asymptoticaly flat gravitational fields can be calculated from a simp...
Matter interacting classically with gravity in 3+1 dimensions usually gives rise to a continuum of d...
We generalize our previous linear result (van de Meent 2011 Class. Quantum Grav 28 075005) in obtain...
We consider the (3+1)-dimensional locally finite gravity model pro-posed by ’t Hooft [1]. In particu...
We study a model for gravity in 3+1 dimensions, inspired in general relativity in 2+1 dimensions. In...
We study a model for gravity in 3+1 dimensions, inspired in general relativity in 2+1 dimensions. In...
We study a model for gravity in 3+1 dimensions, inspired in general relativity in 2+1 dimensions. In...
We derive the gravitational waves for $$f\left( T, B\right) $$ gravity which is an extension of tele...
We consider the (3+1)-dimensional locally finite gravity model proposed by ’t Hooft (2008 Found. Phy...
We study gravity in backgrounds that are smooth generalizations of the Randall-Sundrum model, with a...
Perturbation of gravitational fields may be decomposed into scalar, vector and tensor components. In...
We consider the propagation of gravitational waves in six dimensions induced by sources living on 3-...
We study the plane (not necessarily monochromatic) gravitational waves at nonlinear quadratic order ...
Modified gravity theories generally aim to solve part of the cosmological constant problem by provid...
We study the plane (not necessarily monochromatic) gravitational waves at nonlinear quadratic order ...
The energy density " g of asymptoticaly flat gravitational fields can be calculated from a simp...
Matter interacting classically with gravity in 3+1 dimensions usually gives rise to a continuum of d...
We generalize our previous linear result (van de Meent 2011 Class. Quantum Grav 28 075005) in obtain...
We consider the (3+1)-dimensional locally finite gravity model pro-posed by ’t Hooft [1]. In particu...
We study a model for gravity in 3+1 dimensions, inspired in general relativity in 2+1 dimensions. In...
We study a model for gravity in 3+1 dimensions, inspired in general relativity in 2+1 dimensions. In...
We study a model for gravity in 3+1 dimensions, inspired in general relativity in 2+1 dimensions. In...
We derive the gravitational waves for $$f\left( T, B\right) $$ gravity which is an extension of tele...
We consider the (3+1)-dimensional locally finite gravity model proposed by ’t Hooft (2008 Found. Phy...
We study gravity in backgrounds that are smooth generalizations of the Randall-Sundrum model, with a...
Perturbation of gravitational fields may be decomposed into scalar, vector and tensor components. In...
We consider the propagation of gravitational waves in six dimensions induced by sources living on 3-...
We study the plane (not necessarily monochromatic) gravitational waves at nonlinear quadratic order ...
Modified gravity theories generally aim to solve part of the cosmological constant problem by provid...
We study the plane (not necessarily monochromatic) gravitational waves at nonlinear quadratic order ...
The energy density " g of asymptoticaly flat gravitational fields can be calculated from a simp...
Matter interacting classically with gravity in 3+1 dimensions usually gives rise to a continuum of d...