Galaxy rotation curves via conformal factors

Abstract We propose a new formula to explain circular velocity profiles of spiral galaxies obtained from the Starobinsky model in the Palatini formalism. It is based on the assumption that the gravity can be described by two conformally related metrics: one of them is responsible for the measurement...

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Main Authors: Ciprian A. Sporea, Andrzej Borowiec, Aneta Wojnar
Format: Article
Language:English
Published: SpringerOpen 2018-04-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-5792-2
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author Ciprian A. Sporea
Andrzej Borowiec
Aneta Wojnar
author_facet Ciprian A. Sporea
Andrzej Borowiec
Aneta Wojnar
author_sort Ciprian A. Sporea
collection DOAJ
description Abstract We propose a new formula to explain circular velocity profiles of spiral galaxies obtained from the Starobinsky model in the Palatini formalism. It is based on the assumption that the gravity can be described by two conformally related metrics: one of them is responsible for the measurement of distances, while the other, the so-called dark metric, is responsible for a geodesic equation and therefore can be used for the description of the velocity profile. The formula is tested against a subset of galaxies taken from the HI Nearby Galaxy Survey (THINGS).
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spelling doaj.art-a6d19ed2ce4442b2b36d0ba813a2c36a2022-12-21T20:34:08ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-04-017841710.1140/epjc/s10052-018-5792-2Galaxy rotation curves via conformal factorsCiprian A. Sporea0Andrzej Borowiec1Aneta Wojnar2West University of TimişoaraInstitute for Theoretical PhysicsInstitute of Physics, Maria Curie-Sklodowska UniversityAbstract We propose a new formula to explain circular velocity profiles of spiral galaxies obtained from the Starobinsky model in the Palatini formalism. It is based on the assumption that the gravity can be described by two conformally related metrics: one of them is responsible for the measurement of distances, while the other, the so-called dark metric, is responsible for a geodesic equation and therefore can be used for the description of the velocity profile. The formula is tested against a subset of galaxies taken from the HI Nearby Galaxy Survey (THINGS).http://link.springer.com/article/10.1140/epjc/s10052-018-5792-2
spellingShingle Ciprian A. Sporea
Andrzej Borowiec
Aneta Wojnar
Galaxy rotation curves via conformal factors
European Physical Journal C: Particles and Fields
title Galaxy rotation curves via conformal factors
title_full Galaxy rotation curves via conformal factors
title_fullStr Galaxy rotation curves via conformal factors
title_full_unstemmed Galaxy rotation curves via conformal factors
title_short Galaxy rotation curves via conformal factors
title_sort galaxy rotation curves via conformal factors
url http://link.springer.com/article/10.1140/epjc/s10052-018-5792-2
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AT andrzejborowiec galaxyrotationcurvesviaconformalfactors
AT anetawojnar galaxyrotationcurvesviaconformalfactors