Is gravitational aberration responsible for the origin of dark energy?
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985840%3A_____%2F12%3A00390183" target="_blank" >RIV/67985840:_____/12:00390183 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Is gravitational aberration responsible for the origin of dark energy?
Original language description
At the end of the 20th century it was discovered that the expansion of the Universe is speeding up. This acceleration is attributed to dark energy, which seems to be distributed uniformly almost everywhere and thus essentially influences the Hubble parameter H=H(t) characterizing this expansion. We will split it into two terms H=HM+Hlambda, where HM(t) is due to gravitational interaction of baryonic and dark matter that slows down the expansion of the Universe, whereas H..(t) corresponds to dark energythat accelerates this expansion. We argue that both terms currently have roughly the same size.
Czech name
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Czech description
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Classification
Type
C - Chapter in a specialist book
CEP classification
BA - General mathematics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/IAA100190803" target="_blank" >IAA100190803: The finite element method for higher dimensional problems</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Book/collection name
Dark energy : theory, implications and roles in cosmology
ISBN
978-1-62257-077-5
Number of pages of the result
28
Pages from-to
29-57
Number of pages of the book
170
Publisher name
Nova Publishers
Place of publication
New York
UT code for WoS chapter
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