The Λ and the CDM as Integration Constants
Notoriously, the two main problems of the standard <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula>CDM mod...
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oai:doaj.org-article:08a37d71583b41ba8f8ca013e95f71d12021-11-25T19:06:33ZThe Λ and the CDM as Integration Constants10.3390/sym131120762073-8994https://doaj.org/article/08a37d71583b41ba8f8ca013e95f71d12021-11-01T00:00:00Zhttps://www.mdpi.com/2073-8994/13/11/2076https://doaj.org/toc/2073-8994Notoriously, the two main problems of the standard <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula>CDM model of cosmology are the cosmological constant <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula> and the cold dark matter, CDM. This essay shows that both the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula> and the CDM arise as integration constants in a careful derivation of Einstein’s equations from first principles in a Lorentz gauge theory. The dark sector of the universe might only reflect the geometry of a spontaneous symmetry breaking that is necessary for the existence of spacetime and an observer therein.Priidik GallagherTomi KoivistoMDPI AGarticlecosmologydark matter and dark energygauge theory of gravityMathematicsQA1-939ENSymmetry, Vol 13, Iss 2076, p 2076 (2021) |
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cosmology dark matter and dark energy gauge theory of gravity Mathematics QA1-939 |
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cosmology dark matter and dark energy gauge theory of gravity Mathematics QA1-939 Priidik Gallagher Tomi Koivisto The Λ and the CDM as Integration Constants |
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Notoriously, the two main problems of the standard <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula>CDM model of cosmology are the cosmological constant <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula> and the cold dark matter, CDM. This essay shows that both the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">Λ</mi></semantics></math></inline-formula> and the CDM arise as integration constants in a careful derivation of Einstein’s equations from first principles in a Lorentz gauge theory. The dark sector of the universe might only reflect the geometry of a spontaneous symmetry breaking that is necessary for the existence of spacetime and an observer therein. |
format |
article |
author |
Priidik Gallagher Tomi Koivisto |
author_facet |
Priidik Gallagher Tomi Koivisto |
author_sort |
Priidik Gallagher |
title |
The Λ and the CDM as Integration Constants |
title_short |
The Λ and the CDM as Integration Constants |
title_full |
The Λ and the CDM as Integration Constants |
title_fullStr |
The Λ and the CDM as Integration Constants |
title_full_unstemmed |
The Λ and the CDM as Integration Constants |
title_sort |
λ and the cdm as integration constants |
publisher |
MDPI AG |
publishDate |
2021 |
url |
https://doaj.org/article/08a37d71583b41ba8f8ca013e95f71d1 |
work_keys_str_mv |
AT priidikgallagher thelandthecdmasintegrationconstants AT tomikoivisto thelandthecdmasintegrationconstants AT priidikgallagher landthecdmasintegrationconstants AT tomikoivisto landthecdmasintegrationconstants |
_version_ |
1718410257923833856 |