Energy Conservation Law in the Closed Universe and a Concept of the Proper Time

To define time in the homogeneous anisotropic Bianchi-IX model of the universe, we propose a classical equation of motion of the proper time of the universe as an additional gauge condition. This equation is the law of conservation of energy. As a result, a new parameter, called a “mass” of the univ...

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Main Authors: Natalia Gorobey, Alexander Lukyanenko, Pavel Drozdov
Format: Article
Language:English
Published: MDPI AG 2020-10-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/6/10/174
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author Natalia Gorobey
Alexander Lukyanenko
Pavel Drozdov
author_facet Natalia Gorobey
Alexander Lukyanenko
Pavel Drozdov
author_sort Natalia Gorobey
collection DOAJ
description To define time in the homogeneous anisotropic Bianchi-IX model of the universe, we propose a classical equation of motion of the proper time of the universe as an additional gauge condition. This equation is the law of conservation of energy. As a result, a new parameter, called a “mass” of the universe, appears. This parameter is added to the anisotropy energy and regarded as an observed quantity. The “mass” of the universe is decisive when it comes to the dynamics of its origin.
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spelling doaj.art-5759a2319f0943f4815065ba61a8a91b2023-11-20T16:45:02ZengMDPI AGUniverse2218-19972020-10-0161017410.3390/universe6100174Energy Conservation Law in the Closed Universe and a Concept of the Proper TimeNatalia Gorobey0Alexander Lukyanenko1Pavel Drozdov2Peter the Great Saint Petersburg Polytechnic University, Polytekhnicheskaya 29, 195251 St. Petersburg, RussiaPeter the Great Saint Petersburg Polytechnic University, Polytekhnicheskaya 29, 195251 St. Petersburg, RussiaPeter the Great Saint Petersburg Polytechnic University, Polytekhnicheskaya 29, 195251 St. Petersburg, RussiaTo define time in the homogeneous anisotropic Bianchi-IX model of the universe, we propose a classical equation of motion of the proper time of the universe as an additional gauge condition. This equation is the law of conservation of energy. As a result, a new parameter, called a “mass” of the universe, appears. This parameter is added to the anisotropy energy and regarded as an observed quantity. The “mass” of the universe is decisive when it comes to the dynamics of its origin.https://www.mdpi.com/2218-1997/6/10/174anisotropic universequantum theoryHamiltonianconstraint equationsproper timemass of the universe
spellingShingle Natalia Gorobey
Alexander Lukyanenko
Pavel Drozdov
Energy Conservation Law in the Closed Universe and a Concept of the Proper Time
Universe
anisotropic universe
quantum theory
Hamiltonian
constraint equations
proper time
mass of the universe
title Energy Conservation Law in the Closed Universe and a Concept of the Proper Time
title_full Energy Conservation Law in the Closed Universe and a Concept of the Proper Time
title_fullStr Energy Conservation Law in the Closed Universe and a Concept of the Proper Time
title_full_unstemmed Energy Conservation Law in the Closed Universe and a Concept of the Proper Time
title_short Energy Conservation Law in the Closed Universe and a Concept of the Proper Time
title_sort energy conservation law in the closed universe and a concept of the proper time
topic anisotropic universe
quantum theory
Hamiltonian
constraint equations
proper time
mass of the universe
url https://www.mdpi.com/2218-1997/6/10/174
work_keys_str_mv AT nataliagorobey energyconservationlawinthecloseduniverseandaconceptofthepropertime
AT alexanderlukyanenko energyconservationlawinthecloseduniverseandaconceptofthepropertime
AT paveldrozdov energyconservationlawinthecloseduniverseandaconceptofthepropertime