Nevin Weinberg

Associate Professor

The University of Texas at Arlington

United States

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About

Dr. Nevin Weinberg is an Associate Professor at The University of Texas at Arlington, United States. His research primarily focuses on astrophysics, particularly the stability and dynamics of celestial bodies, tidal interactions in neutron stars, and the habitability of exoplanetary systems. He has recently published articles exploring the potential for moons around habitable-zone planets, the dynamics of δ Scuti stars, and the tidal responses of various star-planet systems.

Articles (14)

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2025

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2025

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2025

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2024

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2024

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2023

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2022

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2021

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2021

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2020

Collaborators (5)

Hang Yu

Assistant Professor

Montana State University

UNITED STATES

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Billy Quarles

Assistant Professor

Valdosta State University

UNITED STATES

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Francesco Barra

Università degli Studi di Palermo Dipartimento di Fisica e Chimica - Emilio Segrè

ITALY

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Tejaswi Venumadhav Nerella

Assistant Professor

University of California, Santa Barbara

UNITED STATES

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Brian Jackson

Associate Professor

Boise State University

UNITED STATES

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Nevin Weinberg

Research Interests

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Articles (14)

Can Moons Exist around the Habitable-zone Planet K2-18b?

Stability and Dynamics of Three-mode Coupling in δ Scuti Stars

Line detections in photospheric radius expansion bursts from 4U 1820-303

Apparent Diameters of F- to M-type Main-sequence Stars as Viewed from Habitable Zone Planets

Dynamical tides during the inspiral of rapidly spinning neutron stars: Solutions beyond mode resonance

Orbital Decay of Hot Jupiters due to Weakly Nonlinear Tidal Dissipation

Statistics and Habitability of F-type Star–Planet Systems

Doomed Worlds. I. No New Evidence for Orbital Decay in a Long-term Survey of 43 Ultrahot Jupiters

Beyond the linear tide: impact of the non-linear tidal response of neutron stars on gravitational waveforms from binary inspirals

Resonant Mode Coupling in δ Scuti Stars

Tidal Evolution and Diffusive Growth During High-eccentricity Planet Migration: Revisiting the Eccentricity Distribution of Hot Jupiters

Tides in the High-eccentricity Migration of Hot Jupiters: Triggering Diffusive Growth by Nonlinear Mode Interactions

Damping of Oscillations in Red Giants by Resonant Mode Coupling

Non-linear dynamical tides in white dwarf binaries

Collaborators (5)

Hang Yu

Billy Quarles

Francesco Barra

Tejaswi Venumadhav Nerella

Brian Jackson

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