Brendan T. Reed
Physics and Astronomy · Indiana University
Publications
32
Citations
1,970
Est. group size
—
Recurring co-author estimate
Active years
9
Publishing since 2018
Brendan T. Reed studies the physics of extremely dense matter, especially the interiors of neutron stars, by combining nuclear physics theory with astronomical observations. The work connects laboratory measurements (such as how electrons scatter off atomic nuclei) with signals from gravitational waves produced by merging neutron stars to constrain how matter behaves under extreme pressure. This includes developing computational tools to estimate nuclear properties from these varied data sources.
Publication activity has been steady over the past several years, averaging around four papers per year since 2020.
Generated by claude-opus-4-8 from public bibliographic data · Jul 11, 2026
- Comment on QED Corrections to the Parity Violating Asymmetry in High-Energy Electron-Nucleus Scattering
arXiv (Cornell University) · 2026
- Comment on QED Corrections to the Parity Violating Asymmetry in High-Energy Electron-Nucleus Scattering
arXiv (Cornell University) · 2026
- From Existing and New Nuclear and Astrophysical Constraints to Stringent Limits on the Equation of State of Neutron-Rich Dense Matter
Physical Review X · 2025
- Connecting relativistic density functional theory to microscopic calculations
Physical Review C · 2025
- Direct Nuclear Parameter Estimation from Gravitational Waves
2025
- Connecting relativistic density functional theory to microscopic calculations
GSI Repository (GSI Helmholtzzentrum für Schwerionenforschung) · 2025
- Toward Accelerated Nuclear-physics Parameter Estimation from Binary Neutron Star Mergers: Emulators for the Tolman–Oppenheimer–Volkoff Equations
The Astrophysical Journal · 2024
- From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter
arXiv (Cornell University) · 2024
- Towards accelerated nuclear-physics parameter estimation from binary neutron star mergers: Emulators for the Tolman-Oppenheimer-Volkoff equations
arXiv (Cornell University) · 2024
- Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817
Physical review. D/Physical review. D. · 2022
- New Measurements of the Beam-Normal Single Spin Asymmetry in Elastic Electron Scattering over a Range of Spin-0 Nuclei
Physical Review Letters · 2022
- Detectability of Sub-Solar Mass Neutron Stars Through a Template Bank Search
arXiv (Cornell University) · 2022
- Precision Determination of the Neutral Weak Form Factor of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>Ca</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>48</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math>
Physical Review Letters · 2022
- Accurate Determination of the Neutron Skin Thickness of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>Pb</mml:mi></mml:mrow><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>208</mml:mn></mml:mrow></mml:mmultiscripts></mml:mrow></mml:math> through Parity-Violation in Electron Scattering
Physical Review Letters · 2021
- Modeling the Galactic Neutron Star Population for Use in Continuous Gravitational Wave Searches
arXiv (Cornell University) · 2021
- arXiv (Cornell University)×10
- Physical Review C×6
- Physical Review Letters×4
- Physical review. D/Physical review. D.×3
- The Astrophysical Journal×2
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 11, 2026.
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