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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

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • 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

  • 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