Missing dust signature in the cosmic microwave background

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985530%3A_____%2F17%3A00475246" target="_blank" >RIV/67985530:_____/17:00475246 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1093/mnrasl/slx069" target="_blank" >http://dx.doi.org/10.1093/mnrasl/slx069</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnrasl/slx069" target="_blank" >10.1093/mnrasl/slx069</a>

Result language
angličtina
Original language name
Missing dust signature in the cosmic microwave background
Original language description
I examine a possible spectral distortion of the cosmic microwave background (CMB) due to its absorption by galactic and intergalactic dust. I show that even subtle intergalactic opacity of 1 x 10(-7) mag h Gpc(-1) at the CMB wavelengths in the local Universe causes non-negligible CMB absorption and decline of the CMB intensity because the opacity steeply increases with redshift. The CMB should be distorted even during the epoch of the Universe defined by redshifts z < 10. For this epoch, the maximum spectral distortion of the CMB is at least 20 x 10(-22)W m(-2) Hz(-1) sr(-1) at 300 GHz, which is well above the sensitivity of the COBE/FIRAS, WMAP or Planck flux measurements. If dust mass is considered to be redshift dependent with noticeable dust abundance at redshifts 2-4, the predicted CMB distortion would be even higher. The CMB would also be distorted in a perfectly transparent universe due to dust in galaxies, but this effect is lower by one order than that due to intergalactic opacity. The fact that the distortion of the CMB by dust is not observed is intriguing and questions either opacity and extinction law measurements or validity of the current model of the Universe.
Czech name
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Czech description
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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)

Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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