Invisible QCD as Dark Energy
We account for the late time acceleration of the Universe by extending the Quantum Chromodynamics (QCD) color to a <inline-formula> <math display="inline"> <semantics> <mrow> <mi>S</mi> <mi>U</mi> <mo>(</mo> <mn>3</mn>...
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doaj-f9f28048c92c4dc1b56f59df70e221da2020-11-25T03:27:10ZengMDPI AGUniverse2218-19972020-05-016757510.3390/universe6060075Invisible QCD as Dark EnergyAndrea Addazi0Stephon Alexander1Antonino Marcianò2Center for Theoretical Physics, College of Physics Science and Technology, Sichuan University, Chengdu 610065, ChinaDepartment of Physics, Brown University, Providence, RI 02912, USACenter for Field Theory and Particle Physics & Department of Physics, Fudan University, Shanghai 200433, ChinaWe account for the late time acceleration of the Universe by extending the Quantum Chromodynamics (QCD) color to a <inline-formula> <math display="inline"> <semantics> <mrow> <mi>S</mi> <mi>U</mi> <mo>(</mo> <mn>3</mn> <mo>)</mo> </mrow> </semantics> </math> </inline-formula> invisible sector (IQCD). If the Invisible Chiral symmetry is broken in the early universe, a condensate of dark pions (dpions) and dark gluons (dgluons) forms. The condensate naturally forms due to strong dynamics similar to the Nambu–Jona-Lasinio mechanism. As the Universe evolves from early times to present times the interaction energy between the dgluon and dpion condensate dominates with a negative pressure equation of state and causes late time acceleration. We conclude with a stability analysis of the coupled perturbations of the dark pions and dark gluons.https://www.mdpi.com/2218-1997/6/6/75dark energynon-Abelian gauge theorycondensate |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Andrea Addazi Stephon Alexander Antonino Marcianò |
spellingShingle |
Andrea Addazi Stephon Alexander Antonino Marcianò Invisible QCD as Dark Energy Universe dark energy non-Abelian gauge theory condensate |
author_facet |
Andrea Addazi Stephon Alexander Antonino Marcianò |
author_sort |
Andrea Addazi |
title |
Invisible QCD as Dark Energy |
title_short |
Invisible QCD as Dark Energy |
title_full |
Invisible QCD as Dark Energy |
title_fullStr |
Invisible QCD as Dark Energy |
title_full_unstemmed |
Invisible QCD as Dark Energy |
title_sort |
invisible qcd as dark energy |
publisher |
MDPI AG |
series |
Universe |
issn |
2218-1997 |
publishDate |
2020-05-01 |
description |
We account for the late time acceleration of the Universe by extending the Quantum Chromodynamics (QCD) color to a <inline-formula> <math display="inline"> <semantics> <mrow> <mi>S</mi> <mi>U</mi> <mo>(</mo> <mn>3</mn> <mo>)</mo> </mrow> </semantics> </math> </inline-formula> invisible sector (IQCD). If the Invisible Chiral symmetry is broken in the early universe, a condensate of dark pions (dpions) and dark gluons (dgluons) forms. The condensate naturally forms due to strong dynamics similar to the Nambu–Jona-Lasinio mechanism. As the Universe evolves from early times to present times the interaction energy between the dgluon and dpion condensate dominates with a negative pressure equation of state and causes late time acceleration. We conclude with a stability analysis of the coupled perturbations of the dark pions and dark gluons. |
topic |
dark energy non-Abelian gauge theory condensate |
url |
https://www.mdpi.com/2218-1997/6/6/75 |
work_keys_str_mv |
AT andreaaddazi invisibleqcdasdarkenergy AT stephonalexander invisibleqcdasdarkenergy AT antoninomarciano invisibleqcdasdarkenergy |
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1724589062165102592 |