activity
20112020
most citedGravitational Waves from Preheating in M-flation

17 citations · 64 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2020★ 4 cited

Quasilocal conservation laws in cosmology: a first look

Marius Oltean, Hossein Bazrafshan Moghaddam, Richard J. Epp

Quasilocal definitions of stress-energy-momentum---that is, in the form of boundary densities (in lieu of local volume densities)---have proven generally very useful in formulating…

gr-qc2020★ 3 cited

Energy of cosmological spacetimes and perturbations: a quasilocal approach

Marius Oltean, Hossein Bazrafshan Moghaddam, Richard J. Epp

Quasilocal definitions of stress-energy-momentum -- that is, in the form of boundary densities (rather than local volume densities) -- have proven generally very useful in formulat…

gr-qc2019★ 1 cited

Study of the Relativistic Dynamics of Extreme-Mass-Ratio Inspirals

Marius Oltean

The principal subject of this thesis is the gravitational two-body problem in the extreme-mass-ratio regime---that is, where one mass is significantly smaller than the other---in t…

gr-qc2019★ 10 cited

Motion of localized sources in general relativity: gravitational self-force from quasilocal conservation laws

Marius Oltean, Richard J. Epp, Carlos F. Sopuerta +2

An idealized "test" object in general relativity moves along a geodesic. However, if the object has a finite mass, this will create additional curvature in the spacetime, causing i…

physics.comp-ph2018★ 4 cited

Particle-without-Particle: a practical pseudospectral collocation method for linear partial differential equations with distributional sources

Marius Oltean, Carlos F. Sopuerta, Alessandro D. A. M. Spallicci

Partial differential equations with distributional sources---in particular, involving (derivatives of) delta distributions---have become increasingly ubiquitous in numerous areas o…

gr-qc2017

Relativistic geoids and time dependence: quasilocal frames versus isochronometric surfaces

Marius Oltean, Richard J. Epp, Paul L. McGrath +1

In a recent paper [D. Philipp, V. Perlick, D. Puetzfeld, E. Hackmann, and C. Lämmerzahl, Phys. Rev. D 95, 104037 (2017)], a definition of a general-relativistic geoid, restricted t…

gr-qc2017★ 1 cited

A frequency-domain implementation of the particle-without-particle approach to EMRIs

Marius Oltean, Carlos F. Sopuerta, Alessandro D. A. M. Spallicci

The gravitational waves emitted by binary systems with extreme mass ratios carry unique astrophysical information expected to be probed by the next generation of gravitational wave…

gr-qc2016★ 2 cited

Entropy theorems in classical mechanics, general relativity, and the gravitational two-body problem

Marius Oltean, Luca Bonetti, Alessandro D. A. M. Spallicci +1

In classical Hamiltonian theories, entropy may be understood either as a statistical property of canonical systems, or as a mechanical property, that is, as a monotonic function of…

gr-qc2015★ 10 cited

Geoids in General Relativity: Geoid Quasilocal Frames

Marius Oltean, Richard J. Epp, Paul L. McGrath +1

We develop, in the context of general relativity, the notion of a geoid -- a surface of constant "gravitational potential". In particular, we show how this idea naturally emerges a…

hep-th2014★ 6 cited

Cosmological Perturbations in Antigravity

Marius Oltean, Robert Brandenberger

We compute the evolution of cosmological perturbations in a recently proposed Weyl-symmetric theory of two scalar fields with oppositely-signed conformal couplings to Einstein grav…

hep-th2013★ 17 cited

Gravitational Waves from Preheating in M-flation

Amjad Ashoorioon, Brandon Fung, Robert B. Mann +2

Matrix inflation, or M-flation, is a string theory motivated inflationary model with three scalar field matrices and gauge fields in the adjoint representation of the $\mathbf{U}(N…

hep-th2011★ 6 cited

Lifshitz Solitons

Robert Mann, Luisa Pegoraro, Marius Oltean

We numerically obtain a class of soliton solutions for Einstein gravity in dimensions coupled to massive abelian gauge fields and with a negative cosmological constant with…