scholarly journals Gauge invariant metric fluctuations in the early universe from STM theory of gravity: Nonperturbative formalism

2007 ◽  
Vol 652 (5-6) ◽  
pp. 233-237 ◽  
Author(s):  
Mariano Anabitarte ◽  
Mauricio Bellini
2006 ◽  
Vol 632 (1) ◽  
pp. 6-12 ◽  
Author(s):  
José Edgar Madriz Aguilar ◽  
Mariano Anabitarte ◽  
Mauricio Bellini

2021 ◽  
Vol 52 (1) ◽  
Author(s):  
Alexander P. Sobolev

AbstractThe gravitational equations were derived in general relativity (GR) using the assumption of their covariance relative to arbitrary transformations of coordinates. It has been repeatedly expressed an opinion over the past century that such equality of all coordinate systems may not correspond to reality. Nevertheless, no actual verification of the necessity of this assumption has been made to date. The paper proposes a theory of gravity with a constraint, the degenerate variants of which are general relativity (GR) and the unimodular theory of gravity. This constraint is interpreted from a physical point of view as a sufficient condition for the adiabaticity of the process of the evolution of the space–time metric. The original equations of the theory of gravity with the constraint are formulated. On this basis, a unified model of the evolution of the modern, early, and very early Universe is constructed that is consistent with the observational astronomical data but does not require the hypotheses of the existence of dark energy, dark matter or inflatons. It is claimed that: physical time is anisotropic, the gravitational field is the main source of energy of the Universe, the maximum global energy density in the Universe was 64 orders of magnitude smaller the Planckian one, and the entropy density is 18 orders of magnitude higher the value predicted by GR. The value of the relative density of neutrinos at the present time and the maximum temperature of matter in the early Universe are calculated. The wave equation of the gravitational field is formulated, its solution is found, and the nonstationary wave function of the very early Universe is constructed. It is shown that the birth of the Universe was random.


2001 ◽  
Vol 42 (2) ◽  
pp. 856 ◽  
Author(s):  
Zdzisław A. Golda ◽  
Andrzej Woszczyna

2018 ◽  
Vol 2018 (5) ◽  
Author(s):  
Ranajit Mandal ◽  
Chandramouli Sarkar ◽  
Abhik Kumar Sanyal

2019 ◽  
pp. 64-72
Author(s):  
Nicholas Mee

Most of the matter in the universe exists in an unknown form called dark matter. All estimates of the mass of galaxies and galaxy clusters suggest they contain far more matter than is visible to us in the form of stars. Conventional explanations, such as the existence of large quantities of burnt-out stars known as MACHOs or dark gas clouds, have been ruled out. The most popular explanation is that dark matter consists of vast quantities of hypothetical stable particles known as WIMPs that were produced in vast quantities in the very early universe. Many laboratories around the world are searching for signs of these particles. These include the Italian Gran Sasso laboratory running the XENON100 experiment. Some theorists have suggested the evidence for dark matter would disappear if we had a better theory of gravity. Analysis of the Bullet Cluster indicates such proposals will not work.


2006 ◽  
Vol 635 (5-6) ◽  
pp. 243-246 ◽  
Author(s):  
Agustin Membiela ◽  
Mauricio Bellini

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