Testing Cotton gravity as dark matter substitute with weak lensing

Fuente: arXiv
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Main Authors: Mo, Geyu, Wang, Qingqing, Ren, Xin, Yan, Weitong, Ong, Yen Chin, Luo, Wentao
Format: Preprint
Published: 2024
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author Mo, Geyu
Wang, Qingqing
Ren, Xin
Yan, Weitong
Ong, Yen Chin
Luo, Wentao
author_facet Mo, Geyu
Wang, Qingqing
Ren, Xin
Yan, Weitong
Ong, Yen Chin
Luo, Wentao
contents Harada proposed a modified theory of gravity called Cotton gravity, and argued that it successfully explains the rotation curves of $84$ galaxies without the need of dark matter. In this work we use galaxy-galaxy lensing technique to test whether the modification effect of Cotton gravity can indeed be a viable substitute for dark matter. Using the spherically symmetric solution of Cotton gravity, we obtain the deflection angle via Gauss-Bonnet theorem and the weak lensing shear. We use five galaxy catalogs divided in 5 stellar mass bins from the Sloan Digital Sky Survey Data Release 7 (SDSS DR7), each of which is further divided into blue star forming galaxy and red passive galaxy sub-catalogs. We find that Cotton gravity on its own has significant deviation from the measured galaxy-galaxy lensing signals, thus it cannot replace the role of dark matter. If we consider the combination of dark matter and Cotton gravity, the modification is tightly constrained. Our analysis also applies to other modified gravity theories whose an additional linear term appears in the Schwarzschild solution.
format Preprint
id arxiv_https___arxiv_org_abs_2405_07215
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Testing Cotton gravity as dark matter substitute with weak lensing
Mo, Geyu
Wang, Qingqing
Ren, Xin
Yan, Weitong
Ong, Yen Chin
Luo, Wentao
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
General Relativity and Quantum Cosmology
Harada proposed a modified theory of gravity called Cotton gravity, and argued that it successfully explains the rotation curves of $84$ galaxies without the need of dark matter. In this work we use galaxy-galaxy lensing technique to test whether the modification effect of Cotton gravity can indeed be a viable substitute for dark matter. Using the spherically symmetric solution of Cotton gravity, we obtain the deflection angle via Gauss-Bonnet theorem and the weak lensing shear. We use five galaxy catalogs divided in 5 stellar mass bins from the Sloan Digital Sky Survey Data Release 7 (SDSS DR7), each of which is further divided into blue star forming galaxy and red passive galaxy sub-catalogs. We find that Cotton gravity on its own has significant deviation from the measured galaxy-galaxy lensing signals, thus it cannot replace the role of dark matter. If we consider the combination of dark matter and Cotton gravity, the modification is tightly constrained. Our analysis also applies to other modified gravity theories whose an additional linear term appears in the Schwarzschild solution.
title Testing Cotton gravity as dark matter substitute with weak lensing
topic Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2405.07215