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Main Authors: Blümke, Maximilian, Schmitz, Kai, Schröder, Tobias, Agarwal, Deepali, Romano, Joseph D.
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2512.24055
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author Blümke, Maximilian
Schmitz, Kai
Schröder, Tobias
Agarwal, Deepali
Romano, Joseph D.
author_facet Blümke, Maximilian
Schmitz, Kai
Schröder, Tobias
Agarwal, Deepali
Romano, Joseph D.
contents The reported evidence for an isotropic gravitational-wave background (GWB) from pulsar timing array (PTA) collaborations has motivated searches for extrinsic and intrinsic anisotropies. Kinematic anisotropies may arise as a consequence of a boosted observer moving with respect to the frame in which the GWB appears isotropic. In this work, we present an analytical toolbox to describe the effects of kinematic anisotropies on the overlap reduction function. Our analytical results differ from previous findings at the quadrupole order and are detailed in three appendices. For the first time, we also derive the corresponding auto-correlation using two approaches, taking the pulsar distances to be infinite or finite, respectively. Our formulas can be used in forecasts or Bayesian analysis pipelines.
format Preprint
id arxiv_https___arxiv_org_abs_2512_24055
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Kinematic Anisotropies in PTA Observations: Analytical Toolkit
Blümke, Maximilian
Schmitz, Kai
Schröder, Tobias
Agarwal, Deepali
Romano, Joseph D.
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
High Energy Physics - Phenomenology
The reported evidence for an isotropic gravitational-wave background (GWB) from pulsar timing array (PTA) collaborations has motivated searches for extrinsic and intrinsic anisotropies. Kinematic anisotropies may arise as a consequence of a boosted observer moving with respect to the frame in which the GWB appears isotropic. In this work, we present an analytical toolbox to describe the effects of kinematic anisotropies on the overlap reduction function. Our analytical results differ from previous findings at the quadrupole order and are detailed in three appendices. For the first time, we also derive the corresponding auto-correlation using two approaches, taking the pulsar distances to be infinite or finite, respectively. Our formulas can be used in forecasts or Bayesian analysis pipelines.
title Kinematic Anisotropies in PTA Observations: Analytical Toolkit
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Astrophysical Phenomena
Instrumentation and Methods for Astrophysics
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2512.24055