Universe opacity and Type Ia supernova dimming
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985530%3A_____%2F19%3A00509007" target="_blank" >RIV/67985530:_____/19:00509007 - isvavai.cz</a>
Result on the web
<a href="https://academic.oup.com/mnrasl/article/489/1/L63/5551485" target="_blank" >https://academic.oup.com/mnrasl/article/489/1/L63/5551485</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnrasl/slz128" target="_blank" >10.1093/mnrasl/slz128</a>
Alternative languages
Result language
angličtina
Original language name
Universe opacity and Type Ia supernova dimming
Original language description
In this paper, I revoke a debate about an origin of Type Ia supernova (SN Ia) dimming. I argue that except for a commonly accepted accelerating expansion of the Universe, a conceivable alternative for explaining this observation is universe opacity caused by light extinction by intergalactic dust, even though it is commonly assumed that this effect is negligible. Using data of the Union2.1 SN Ia compilation, I find that the standard Lambda cold dark matter (Lambda CDM) model and the opaque universe model fit the SN Ia measurements at redshifts z < 1.4 comparably well. The optimum solution for the opaque universe model is characterized by the B-band intergalactic opacity lambda(B) = 0.10 +/- 0.03 Gpc(-1) and the Hubble constant H-0 = 68.0 +/- 2.5 kms(-1) Mpc(-1). The intergalactic opacity is higher than that obtained from independent observations but still within acceptable limits. This result emphasizes that the issue of the accelerating expansion of the Universe as the origin of the SN Ia dimming is not yet definitely resolved. Obviously, the opaque universe model as an alternative to the Lambda CDM model is attractive, because it avoids puzzles and controversies associated with dark energy and the accelerating expansion.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Monthly Notices of the Royal Astronomical Society
ISSN
0035-8711
e-ISSN
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Volume of the periodical
489
Issue of the periodical within the volume
October
Country of publishing house
GB - UNITED KINGDOM
Number of pages
6
Pages from-to
"L63"-"L68"
UT code for WoS article
000491355100012
EID of the result in the Scopus database
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