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R. C. Essick | Researchclopedia

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R. C. Essick

Perimeter Institute ORCID

193

Works

51,833

Citations

67

h-index

112

i10-index

Research Topics

Pulsars and Gravitational Waves Research Gamma-ray bursts and supernovae Geophysics and Gravity Measurements

Affiliations

Centre National de la Recherche Scientifique2019–2019

Fermi National Accelerator Laboratory2019–2019

Perimeter Institute2021–2025

University of Toronto2023–2025

Laboratoire d’Annecy de Physique des Particules2019–2019

Top Works

Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations

Philippe Landry,R. C. Essick,et al.

2020329 citations

Astrophysical Phenomena and Observations

Cosmology and Gravitation Theories

Nonparametric inference of the neutron star equation of state from gravitational wave observations

Philippe Landry,R. C. Essick

2019192 citations

Nonparametric inference of neutron star composition, equation of state, and maximum mass with GW170817

R. C. Essick,Philippe Landry,et al.

2020191 citations

Impact of the PSR <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi mathvariant="normal">J</mml:mi><mml:mn>0740</mml:mn><mml:mo>+</mml:mo><mml:mn>6620</mml:mn></mml:mrow></mml:math> radius constraint on the properties of high-density matter

Isaac Legred,Katerina Chatziioannou,et al.

2021190 citations

Information-theoretic approach to the gravitational-wave burst detection problem

Ryan S. Lynch,S. Vitale,et al.

2017129 citations

Direct astrophysical tests of chiral effective field theory at supranuclear densities

R. C. Essick,Ingo Tews,et al.

2020122 citations

ORBITAL DECAY OF HOT JUPITERS DUE TO NONLINEAR TIDAL DISSIPATION WITHIN SOLAR-TYPE HOSTS

R. C. Essick,Nevin N. Weinberg

2015116 citations

Application of machine learning algorithms to the study of noise artifacts in gravitational-wave data

R. Biswas,Lindy Blackburn,et al.

2013113 citations

Detailed examination of astrophysical constraints on the symmetry energy and the neutron skin of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Pb</mml:mi><mml:mprescripts/><mml:none/><mml:mn>208</mml:mn></mml:mmultiscripts></mml:math> with minimal modeling assumptions

R. C. Essick,Philippe Landry,et al.

202187 citations