Testing Gravitation from Light-second to Cosmological Scales with Radio Pulsars

Fuente: arXiv
Saved in:
Bibliographic Details
Main Author: Fonseca, Emmanuel
Format: Preprint
Published: 2025
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866916983152312320
author Fonseca, Emmanuel
author_facet Fonseca, Emmanuel
contents Pulsars are spinning neutron stars typically observed as pulses emitted at radio wavelengths. These pulsations exhibit a rotational stability that rival the best atomic clocks, making pulsars one of the most important tools for resolving gravitational phenomena in extreme environments. I will present an overview of the ways in which radio pulsars can be used to test strong-field gravity and observe gravitational radiation, both in the context of historical and ongoing experiments. I will also describe how these measurements can be translated to sought-after quantities like the masses and moments of inertia of neutron stars.
format Preprint
id arxiv_https___arxiv_org_abs_2510_01062
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Testing Gravitation from Light-second to Cosmological Scales with Radio Pulsars
Fonseca, Emmanuel
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
Pulsars are spinning neutron stars typically observed as pulses emitted at radio wavelengths. These pulsations exhibit a rotational stability that rival the best atomic clocks, making pulsars one of the most important tools for resolving gravitational phenomena in extreme environments. I will present an overview of the ways in which radio pulsars can be used to test strong-field gravity and observe gravitational radiation, both in the context of historical and ongoing experiments. I will also describe how these measurements can be translated to sought-after quantities like the masses and moments of inertia of neutron stars.
title Testing Gravitation from Light-second to Cosmological Scales with Radio Pulsars
topic High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2510.01062