activity
19972024
most citedWald's entropy is equal to a quarter of the horizon area in units of the effective gravitational coupling

125 citations · 300 across the 20 of their papers we have counts for

collaborators

20 papers

hep-th2024

Islands in Bianchi type-I Universe

Ido Ben-Dayan, Merav Hadad, Ayushi Srivastava

We study the conditions for finding an island in an anisotropic universe - Bianchi Type-I filled with radiation. We verify that the existence of islands does not depend on their sh…

hep-th2022★ 13 cited

Islands in the Fluid: Islands are Common in Cosmology

Ido Ben-Dayan, Merav Hadad, Elizabeth Wildenhain

We discuss the possibility of entanglement islands in cosmological spacetimes with a general perfect fluid with an equation of state . We find that flat universes with time-symm…

hep-th2022

Proposed evolution in Marolf-Maxfield toy model obtained through correspondence to spontaneous collapse theory

Merav Hadad

The Marolf-Maxfield topological toy model for 2D gravity gives the full spectrum of boundary theories, but can not describe any evolution. In order to obtain the expected evolution…

hep-th2021★ 6 cited

The Grand Canonical Multiverse and the Small Cosmological Constant

Ido Ben-Dayan, Merav Hadad, Amir Michaelis

We consider the Multiverse as an ensemble of universes. Using standard statistical physics analysis we get that the Cosmological Constant (CC) is exponentially small. The small and…

hep-th2020★ 5 cited

Thermodynamical Interpretation of the Second Law for Cosmology

Ido Ben-Dayan, Merav Hadad

The area of a future holographic screen increases monotonically. Associating this area with entropy results in a generalized second law for Cosmology (GSLC). Unlike black hole hori…

gr-qc2019

Truncation of Einstein equations through Gravitational Foliation

Merav Hadad

In previous works, we suggested considering a (3+1)D quantum gravitational field as an evolution of a (2+1)D renormalized quantum gravitational field along the direction of the gra…

hep-th2019

Derivation of Hamilton-like equations on a non-Cauchy hypersurface and their expected connection to quantum gravity theories

Merav Hadad, Levy Rosenblum

Recently it was found that quantum gravity theories may involve constructing a quantum theory on non-Cauchy hypersurfaces. However this is problematic since the ordinary Poisson br…

hep-th2019

Non-Cauchy surface foliations and their expected connection to quantum gravity theories

Merav Hadad

We argue that quantum gravity theories should involve constructing a quantum theory on non-Cauchy hypersurfaces and suggest that the hypersurface direction should be the same as th…

gr-qc2016

The space time DoF surface density as a phase-space of accelerating reference frames

Merav Hadad

Padmanabhan found a definition for the surface density of space time degrees of freedom. We prove that this density can be constructed from a phase space which is derived with resp…

gr-qc2015★ 5 cited

The two canonical conjugate pairs at the horizon of a D1D5 black hole

Merav Hadad, Levy Rosenblum

The Euclidian opening angle at the surface, at the horizon of a black hole is canonically conjugate to the black hole entropy. We prove that for a black…

hep-th2012★ 28 cited

Wave function of the quantum black hole

Ram Brustein, Merav Hadad

We show that the Wald Noether charge entropy is canonically conjugate to the opening angle at the horizon. Using this canonical relation we extend the Wheeler-DeWitt equation to a…

hep-th2011★ 7 cited

Evaluating the Wald Entropy from two-derivative terms in quadratic actions

Ram Brustein, Dan Gorbonos, Merav Hadad +1

We evaluate the Wald Noether charge entropy for a black hole in generalized theories of gravity. Expanding the Lagrangian to second order in gravitational perturbations, we show th…

gr-qc2010★ 1 cited

Comparison of Variations of Statistical and Wald's Entropies

Merav Hadad, Judy Kupferman

We write the variation of the statistical entropy of matter fields outside a black hole along a Killing vector. This is done for generalized theories of gravity, using a Lie deriva…

hep-th2009★ 60 cited

The Einstein equations for generalized theories of gravity and the thermodynamic relation are equivalent

Ram Brustein, Merav Hadad

We show that the equations of motion of generalized theories of gravity are equivalent to the thermodynamic relation . Our proof relies on extending previous arguments b…

hep-th2007★ 125 cited

Wald's entropy is equal to a quarter of the horizon area in units of the effective gravitational coupling

Ram Brustein, Dan Gorbonos, Merav Hadad

The Bekenstein-Hawking entropy of black holes in Einstein's theory of gravity is equal to a quarter of the horizon area in units of Newton's constant. Wald has proposed that in gen…

hep-ph2000★ 8 cited

Production of fermions in models of string cosmology

Ram Brustein, Merav Hadad

Production of spin 1/2 fermions and gravitinos by the standard mechanism of amplification of quantum fluctuations during the dilaton-driven inflation phase in models of string cosm…

hep-ph1999

Dark Matter in Models of String Cosmology

Ram Brustein, Merav Hadad

The origin of dark matter in the universe may be weakly interacting scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation.…

hep-ph1998★ 6 cited

Cold and Hot Dark Matter from a Single Nonthermal Relic

Ram Brustein, Merav Hadad

The origin of dark matter in the universe may be scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We show, for the fi…

hep-ph1998★ 8 cited

Dark Matter Axions in Models of String Cosmology

Ram Brustein, Merav Hadad

Axions are produced during a period of dilaton-driven inflation by amplification of quantum fluctuations. We show that for some range of string cosmology parameters and some range…

hep-th1997★ 28 cited

Particle production in string cosmology models

Ram Brustein, Merav Hadad

We compute spectra of particles produced during a dilaton-driven kinetic inflation phase within string cosmology models. The resulting spectra depend on the parameters of the model…