Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology

Based on baryon charge conservation and a generalized Yang-Mills symmetry for Abelian (and non-Abelian) groups, we discuss a new baryonic gauge field and its linear potential for two point-like baryon charges. The force between two point-like baryons is repulsive, extremely weak and independent of d...

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Main Authors: Khan Mehbub, Hao Yun, Hsu Jong-Ping
Format: Article
Language:English
Published: EDP Sciences 2018-01-01
Series:EPJ Web of Conferences
Online Access:https://doi.org/10.1051/epjconf/201816804004
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author Khan Mehbub
Hao Yun
Hsu Jong-Ping
author_facet Khan Mehbub
Hao Yun
Hsu Jong-Ping
author_sort Khan Mehbub
collection DOAJ
description Based on baryon charge conservation and a generalized Yang-Mills symmetry for Abelian (and non-Abelian) groups, we discuss a new baryonic gauge field and its linear potential for two point-like baryon charges. The force between two point-like baryons is repulsive, extremely weak and independent of distance. However, for two extended baryonic systems, we have a dominant linear force α r. Thus, only in the later stage of the cosmic evolution, when two baryonic galaxies are separated by an extremely large distance, the new repulsive baryonic force can overcome the gravitational attractive force. Such a model provides a gauge-field-theoretic understanding of the late-time accelerated cosmic expansion. The baryonic force can be tested by measuring the accelerated Wu-Doppler frequency shifts of supernovae at different distances.
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spelling doaj.art-04a37bae6d1745db96fb63dd2e8341fc2022-12-21T22:08:10ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011680400410.1051/epjconf/201816804004epjconf_icgaxiii-ik2018_04004Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-CosmologyKhan MehbubHao YunHsu Jong-PingBased on baryon charge conservation and a generalized Yang-Mills symmetry for Abelian (and non-Abelian) groups, we discuss a new baryonic gauge field and its linear potential for two point-like baryon charges. The force between two point-like baryons is repulsive, extremely weak and independent of distance. However, for two extended baryonic systems, we have a dominant linear force α r. Thus, only in the later stage of the cosmic evolution, when two baryonic galaxies are separated by an extremely large distance, the new repulsive baryonic force can overcome the gravitational attractive force. Such a model provides a gauge-field-theoretic understanding of the late-time accelerated cosmic expansion. The baryonic force can be tested by measuring the accelerated Wu-Doppler frequency shifts of supernovae at different distances.https://doi.org/10.1051/epjconf/201816804004
spellingShingle Khan Mehbub
Hao Yun
Hsu Jong-Ping
Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology
EPJ Web of Conferences
title Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology
title_full Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology
title_fullStr Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology
title_full_unstemmed Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology
title_short Baryonic Force for Accelerated Cosmic Expansion and Generalized U1b Gauge Symmetry in Particle-Cosmology
title_sort baryonic force for accelerated cosmic expansion and generalized u1b gauge symmetry in particle cosmology
url https://doi.org/10.1051/epjconf/201816804004
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AT hsujongping baryonicforceforacceleratedcosmicexpansionandgeneralizedu1bgaugesymmetryinparticlecosmology