• Thumbnail for Cosmic neutrino background
    The cosmic neutrino background (CNB or CνB) is the universe's background particle radiation composed of neutrinos. They are sometimes known as relic neutrinos...
    19 KB (2,354 words) - 20:20, 13 September 2024
  • Thumbnail for Cosmic background radiation
    individual source. See cosmic infrared background and X-ray background. See also cosmic neutrino background and extragalactic background light. 1896: Charles...
    5 KB (514 words) - 00:56, 11 January 2024
  • Thumbnail for Neutrino
    cosmic neutrino background is also a probe of whether neutrinos are Majorana particles, since there should be a different number of cosmic neutrinos detected...
    141 KB (14,038 words) - 09:56, 23 October 2024
  • Cosmic background may refer to: Cosmic microwave background radiation (CMB) Cosmic neutrino background (CνB) Cosmic gravitational wave background (GWB)...
    636 bytes (85 words) - 02:41, 28 May 2021
  • 000 years after the Big Bang. They form the cosmic neutrino background (abbreviated CνB or CNB). The neutrinos from this event have a very low energy, around...
    11 KB (1,457 words) - 23:57, 27 August 2021
  • Thumbnail for Chronology of the universe
    in the universe. At about one second, neutrinos decouple; these neutrinos form the cosmic neutrino background (CνB). If primordial black holes exist...
    138 KB (13,947 words) - 15:11, 21 November 2024
  • Thumbnail for Polarization (cosmology)
    Big Bang - namely, neutrino decoupling and photon decoupling led to the cosmic neutrino background and cosmic microwave background respectively, in that...
    26 KB (3,113 words) - 06:53, 19 November 2024
  • Thumbnail for Neutrino astronomy
    gamma ray bursts, the cosmic neutrino background, origins of ultra-high-energy neutrinos, neutrino properties (such as neutrino mass hierarchy), dark...
    38 KB (4,742 words) - 02:19, 3 November 2024
  • Thumbnail for Cosmic microwave background
    The cosmic microwave background (CMB, CMBR), or relic radiation, is microwave radiation that fills all space in the observable universe. With a standard...
    108 KB (13,172 words) - 18:52, 18 September 2024
  • The DSNB is not to be confused with the cosmic neutrino background (CNB), which is comprised by relic neutrinos that were produced during the Big Bang...
    15 KB (2,007 words) - 04:14, 4 August 2024
  • Thumbnail for Decoupling (cosmology)
    are photon decoupling and neutrino decoupling, as these led to the cosmic microwave background and cosmic neutrino background, respectively. Photon decoupling...
    7 KB (922 words) - 21:22, 4 May 2024
  • Thumbnail for IceCube Neutrino Observatory
    neutrino signals from any direction, but neutrinos coming from the direction of the southern hemisphere are swamped by the cosmic-ray muon background...
    117 KB (4,850 words) - 06:50, 12 November 2024
  • Thumbnail for Neutrino detector
    underground, to isolate the detector from cosmic rays and other background radiation. The field of neutrino astronomy is still very much in its infancy...
    32 KB (3,877 words) - 10:30, 23 October 2024
  • Thumbnail for Gravitational wave background
    leading candidates. Physics portal Cosmic background radiation Cosmic microwave background Cosmic neutrino background Gravitational-wave astronomy O'Callaghan...
    19 KB (1,943 words) - 11:47, 2 September 2024
  • Thumbnail for Cosmic Background Explorer
    The Cosmic Background Explorer (COBE /ˈkoʊbi/ KOH-bee), also referred to as Explorer 66, was a NASA satellite dedicated to cosmology, which operated from...
    33 KB (3,843 words) - 00:40, 28 October 2024
  • Thumbnail for Equation of state (cosmology)
    The equation of state for ultra-relativistic 'radiation' (including neutrinos, and in the very early universe other particles that later became non-relativistic)...
    8 KB (1,059 words) - 01:59, 13 August 2024
  • Thumbnail for Copernican principle
    kinetic Sunyaev–Zeldovich effect in relation to dark energy; cosmic neutrino background; the integrated Sachs–Wolfe effect testing the isotropy and homogeneity...
    21 KB (2,473 words) - 18:29, 17 November 2024
  • the proposed Z-burst model, an ultra-high-energy cosmic neutrino collides with a relic anti-neutrino in our galaxy and annihilates to hadrons. This process...
    17 KB (2,309 words) - 00:23, 12 November 2024
  • Thumbnail for Wilkinson Microwave Anisotropy Probe
    Wilkinson Microwave Anisotropy Probe (category Cosmic microwave background experiments)
    in neutrinos, but WMAP's measurements have found, for the first time in 2008, that the data prefer the existence of a cosmic neutrino background with...
    50 KB (4,509 words) - 04:38, 28 July 2024
  • Thumbnail for Void (astronomy)
    of the masses of all neutrino species by comparing the statistical properties of void samples to theoretical predictions. Cosmic voids contain a mix of...
    37 KB (4,466 words) - 00:59, 18 November 2024
  • Thumbnail for Outer space
    electromagnetic radiation, cosmic rays, neutrinos, magnetic fields and dust. The baseline temperature of outer space, as set by the background radiation from the...
    138 KB (13,572 words) - 02:34, 20 November 2024
  • Thumbnail for Physical cosmology
    the neutrino masses. Newer experiments, such as QUIET and the Atacama Cosmology Telescope, are trying to measure the polarization of the cosmic microwave...
    77 KB (7,671 words) - 13:04, 2 November 2024
  • Thumbnail for Redshift
    Redshift (redirect from Cosmic redshift)
    observable are the cosmic neutrino background from about two seconds after the Big Bang (and a redshift in excess of z > 1010) and the cosmic gravitational...
    87 KB (9,312 words) - 16:06, 12 November 2024
  • Thumbnail for Timeline of the early universe
    Gravity governs the expansion of the universe: neutrinos decouple from matter creating a cosmic neutrino background. c. 10 seconds: Photon epoch begins: Most...
    36 KB (5,008 words) - 07:50, 6 October 2024
  • streaming. Similarly, the surface of the cosmic neutrino background, if it could be observed, would mark when neutrinos decoupled and began to stream freely...
    2 KB (238 words) - 10:32, 4 November 2024
  • Thumbnail for Age of the universe
    (1995). "Cosmic concordance". arXiv:astro-ph/9505066. de Bernardis, F.; Melchiorri, A.; Verde, L.; Jimenez, R. (2008). "The Cosmic Neutrino Background and...
    34 KB (3,946 words) - 06:39, 1 November 2024
  • Thumbnail for Cosmic infrared background
    Cosmic infrared background is infrared radiation caused by stellar dust. Recognizing the cosmological importance of the darkness of the night sky (Olbers'...
    17 KB (2,415 words) - 18:55, 16 July 2024
  • Thumbnail for Observable universe
    calculations, the current comoving distance to particles from which the cosmic microwave background radiation (CMBR) was emitted, which represents the radius of...
    64 KB (6,628 words) - 03:14, 10 November 2024
  • Thumbnail for Cosmic inflation
    appears to be the same in all directions (isotropic), why the cosmic microwave background radiation is distributed evenly, why the universe is flat, and...
    108 KB (12,912 words) - 15:10, 15 November 2024
  • Thumbnail for Expansion of the universe
    conventionally called radiation, by the time of neutrino decoupling at about 1 second. During radiation domination, cosmic expansion decelerated, with the scale...
    53 KB (6,979 words) - 12:02, 20 November 2024