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19932026
most citedBlack holes, gravitational waves and fundamental physics: a roadmap

742 citations · 4.1k across the 231 of their papers we have counts for

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Showing 2015 · gr-qcShow all

12 papers · 2 filters

gr-qc2015

Metric-Independent Spacetime Volume-Forms and Dark Energy/Dark Matter Unification

Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

The method of non-Riemannian (metric-independent) spacetime volume-forms (alternative generally-covariant integration measure densities) is applied to construct a modified model of…

gr-qc2015★ 1 cited

Kruskal-Penrose Formalism for Lightlike Thin-Shell Wormholes

Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva +1

The original formulation of the "Einstein-Rosen bridge" in the classic paper of Einstein and Rosen (1935) is historically the first example of a static spherically-symmetric wormho…

gr-qc2015★ 14 cited

Curvaton reheating in a Scale Invariant Two Measures Theory

Eduardo I. Guendelman, Ramon Herrera

The curvaton reheating mechanism in a Scale Invariant Two Measures Theory defined in terms of two independent non-Riemannian volume forms (alternative generally covariant integrati…

gr-qc2015★ 46 cited

Unified Dark Energy and Dust Dark Matter Dual to Quadratic Purely Kinetic K-Essence

Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

We consider a modified gravity plus single-scalar-field model, where the scalar Lagrangian couples symmetrically both to the standard Riemannian volume-form (spacetime integration…

gr-qc2015

On some topological deformation of stationary spacetimes

Arka Prabha Banik, Eduardo Guendelman

We define a completely new space-time starting from the well known Schwarzschild Space time by defining a new polar angle and then redefining the periodicity: instead o…

gr-qc2015★ 7 cited

Dark Energy and Dark Matter From Hidden Symmetry of Gravity Model with a Non-Riemannian Volume Form

Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

We show that dark energy and dark matter can be described simultaneously by ordinary Einstein gravity interacting with a single scalar field provided the scalar field Lagrangian co…

gr-qc2015★ 1 cited

Cosmology via Metric-Independent Volume-Form Dynamics

Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

The method of non-Riemannian volume-forms (metric-independent covariant integration measure densities on the spacetime manifold) is applied to construct a unified model of dynamica…

gr-qc2015★ 8 cited

Classically and Quantum stable Emergent Universe from Conservation Laws

Sergio del Campo, Eduardo I. Guendelman, Ramon Herrera +1

It has been recently pointed out by Mithani-Vilenkin that certain emergent universe scenarios which are classically stable are nevertheless unstable semiclassically to collapse. He…

gr-qc2015★ 19 cited

Vacuum Structure and Gravitational Bags Produced by Metric-Independent Spacetime Volume-Form Dynamics

Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

We propose a new class of gravity-matter-gauge theories in terms of two different non-Riemannian volume-forms independent of the Riemannian metric. The nonlinear gauge field system…

gr-qc2015★ 2 cited

Metric-Independent Volume-Forms in Gravity and Cosmology

Eduardo Guendelman, Emil Nissimov, Svetlana Pacheva

Employing alternative spacetime volume-forms (generally-covariant integration measure densities) independent of the pertinent Riemannian spacetime metric have profound impact in ge…

gr-qc2015★ 1 cited

The Schwarzschild metric and the Friedmann equations from Newtonian Gravitational collapse

Eduardo I. Guendelman, Arka Prabha Banik, Gilad Granit +2

As is well known, the 0 - 0 component of the Schwarzschild space can be obtained by the requirement that the geodesic of slowly moving particles match the Newtonian equation. Given…

gr-qc2015★ 1 cited

Schwarzschild and Friedmann Lemaître Robertson Walker metrics from Newtonian Gravitational collapse

Eduardo I. Guendelman, Arka Prabha Banik, Gilad Granit +2

As it is well known, the component of the Schwarzschild space can be obtained by the requirement that the geodesic of slowly moving particles match the Newtonian equation. Gi…