On the radiative and thermodynamic properties of the cosmic radiations using COBE FIRAS instrument data: II. Extragalactic far infrared background radiation
Using formula to describe the average spectrum of the extragalactic far infrared background (FIRB) radiation measured by the COBE FIRAS instrument in the 0.15–2.4 THz frequency interval at mean temperature T =18.5 K, the radiative and thermodynamic properties, such as the total emissivity, total rad...
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| Veröffentlicht in: | Astrophysics and space science 2014-07, Vol.352 (1), p.231-234 |
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| creator | Fisenko, Anatoliy I. Lemberg, Vladimir |
| description | Using formula to describe the average spectrum of the extragalactic far infrared background (FIRB) radiation measured by the
COBE
FIRAS instrument in the 0.15–2.4 THz frequency interval at mean temperature
T
=18.5 K, the radiative and thermodynamic properties, such as the total emissivity, total radiation power per unit area, total energy density, number density of photons, Helmholtz free energy density, entropy density, heat capacity at constant volume, and pressure are calculated. The value for the total intensity received in the 0.15–2.4 THz frequency interval is equal to 13.6 nW m
−2
sr
−1
. This value is about 19.4 % of the total intensity expected from the energy released by stellar nucleosynthesis over cosmic history. The radiative and thermodynamic functions of the extragalactic far infrared background (FIRB) radiation are calculated at redshift
z
=1.5. |
| doi_str_mv | 10.1007/s10509-014-1880-4 |
| format | Article |
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COBE
FIRAS instrument in the 0.15–2.4 THz frequency interval at mean temperature
T
=18.5 K, the radiative and thermodynamic properties, such as the total emissivity, total radiation power per unit area, total energy density, number density of photons, Helmholtz free energy density, entropy density, heat capacity at constant volume, and pressure are calculated. The value for the total intensity received in the 0.15–2.4 THz frequency interval is equal to 13.6 nW m
−2
sr
−1
. This value is about 19.4 % of the total intensity expected from the energy released by stellar nucleosynthesis over cosmic history. The radiative and thermodynamic functions of the extragalactic far infrared background (FIRB) radiation are calculated at redshift
z
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COBE
FIRAS instrument in the 0.15–2.4 THz frequency interval at mean temperature
T
=18.5 K, the radiative and thermodynamic properties, such as the total emissivity, total radiation power per unit area, total energy density, number density of photons, Helmholtz free energy density, entropy density, heat capacity at constant volume, and pressure are calculated. The value for the total intensity received in the 0.15–2.4 THz frequency interval is equal to 13.6 nW m
−2
sr
−1
. This value is about 19.4 % of the total intensity expected from the energy released by stellar nucleosynthesis over cosmic history. The radiative and thermodynamic functions of the extragalactic far infrared background (FIRB) radiation are calculated at redshift
z
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COBE
FIRAS instrument in the 0.15–2.4 THz frequency interval at mean temperature
T
=18.5 K, the radiative and thermodynamic properties, such as the total emissivity, total radiation power per unit area, total energy density, number density of photons, Helmholtz free energy density, entropy density, heat capacity at constant volume, and pressure are calculated. The value for the total intensity received in the 0.15–2.4 THz frequency interval is equal to 13.6 nW m
−2
sr
−1
. This value is about 19.4 % of the total intensity expected from the energy released by stellar nucleosynthesis over cosmic history. The radiative and thermodynamic functions of the extragalactic far infrared background (FIRB) radiation are calculated at redshift
z
=1.5.</abstract><cop>Dordrecht</cop><pub>Springer Netherlands</pub><doi>10.1007/s10509-014-1880-4</doi><tpages>4</tpages></addata></record> |
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| subjects | Astrobiology Astronomy Astrophysics Astrophysics and Astroparticles Background radiation Cosmic background radiation Cosmology Emissivity Observations and Techniques Original Article Physics Physics and Astronomy Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Thermodynamics |
| title | On the radiative and thermodynamic properties of the cosmic radiations using COBE FIRAS instrument data: II. Extragalactic far infrared background radiation |
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