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...
Main Authors: | , , |
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Format: | Article |
Language: | English |
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EDP Sciences
2018-01-01
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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. |
first_indexed | 2024-12-17T01:46:50Z |
format | Article |
id | doaj.art-04a37bae6d1745db96fb63dd2e8341fc |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-12-17T01:46:50Z |
publishDate | 2018-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
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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