Late Time Acceleration of the Universe from Quantum Gravity

We show that the accelerating expansion phase of the universe can emerge from the group field theory formalism, a candidate theory of quantum gravity. The cosmological evolution can be extracted from condensate states using the mean field approximation, in a form of modified FLRW equations. By intro...

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Main Author: Xiankai Pang
Format: Article
Language:English
Published: MDPI AG 2022-03-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/3/163
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author Xiankai Pang
author_facet Xiankai Pang
author_sort Xiankai Pang
collection DOAJ
description We show that the accelerating expansion phase of the universe can emerge from the group field theory formalism, a candidate theory of quantum gravity. The cosmological evolution can be extracted from condensate states using the mean field approximation, in a form of modified FLRW equations. By introducing an effective equation of state <i>w</i>, we can reveal the relevant features of the evolution and show that, with the proper choice of the parameters, <i>w</i> will approach <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>−</mo><mn>1</mn></mrow></semantics></math></inline-formula>, leading to an accelerating phase dominated by the cosmological constant effectively.
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spelling doaj.art-dd395ab637084f3b8b715bd16a540b0a2023-11-30T22:40:40ZengMDPI AGUniverse2218-19972022-03-018316310.3390/universe8030163Late Time Acceleration of the Universe from Quantum GravityXiankai Pang0Arnold-Sommerfeld-Center for Theoretical Physics, Ludwig-Maximilians-Universität, Theresienstraße 37, 80333 Müchen, GermanyWe show that the accelerating expansion phase of the universe can emerge from the group field theory formalism, a candidate theory of quantum gravity. The cosmological evolution can be extracted from condensate states using the mean field approximation, in a form of modified FLRW equations. By introducing an effective equation of state <i>w</i>, we can reveal the relevant features of the evolution and show that, with the proper choice of the parameters, <i>w</i> will approach <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mo>−</mo><mn>1</mn></mrow></semantics></math></inline-formula>, leading to an accelerating phase dominated by the cosmological constant effectively.https://www.mdpi.com/2218-1997/8/3/163dark energy theoryquantum cosmologyquantum gravity phenomenology
spellingShingle Xiankai Pang
Late Time Acceleration of the Universe from Quantum Gravity
Universe
dark energy theory
quantum cosmology
quantum gravity phenomenology
title Late Time Acceleration of the Universe from Quantum Gravity
title_full Late Time Acceleration of the Universe from Quantum Gravity
title_fullStr Late Time Acceleration of the Universe from Quantum Gravity
title_full_unstemmed Late Time Acceleration of the Universe from Quantum Gravity
title_short Late Time Acceleration of the Universe from Quantum Gravity
title_sort late time acceleration of the universe from quantum gravity
topic dark energy theory
quantum cosmology
quantum gravity phenomenology
url https://www.mdpi.com/2218-1997/8/3/163
work_keys_str_mv AT xiankaipang latetimeaccelerationoftheuniversefromquantumgravity