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  2. Neutron temperature - Wikipedia

    en.wikipedia.org/wiki/Neutron_temperature

    A fast neutron is a free neutron with a kinetic energy level close to 1 M eV (100 T J/kg), hence a speed of 14,000 km/s or higher. They are named fast neutrons to distinguish them from lower-energy thermal neutrons, and high-energy neutrons produced in cosmic showers or accelerators.

  3. Neutron moderator - Wikipedia

    en.wikipedia.org/wiki/Neutron_moderator

    [2] [3] The characteristic neutron temperature of several-MeV neutrons is several tens of billions kelvin. Moderation is the process of the reduction of the initial high speed (high kinetic energy) of the free neutron. Since energy is conserved, this reduction of the neutron speed takes place by transfer of energy to a material called a moderator.

  4. Neutron - Wikipedia

    en.wikipedia.org/wiki/Neutron

    Toggle Neutron temperature subsection. 13.1 Thermal neutrons. 13.2 Cold neutrons. 13.3 Ultracold neutrons. ... Certain nuclides have a high neutron capture cross ...

  5. Neutron radiation - Wikipedia

    en.wikipedia.org/wiki/Neutron_radiation

    Neutron radiation is a form of ionizing radiation that presents as free neutrons.Typical phenomena are nuclear fission or nuclear fusion causing the release of free neutrons, which then react with nuclei of other atoms to form new nuclides—which, in turn, may trigger further neutron radiation.

  6. Cosmic neutrino background - Wikipedia

    en.wikipedia.org/wiki/Cosmic_neutrino_background

    The cosmic neutrino background (CNB or C ν B [a]) is the universe's background particle radiation composed of neutrinos.They are sometimes known as relic neutrinos.. The C ν B is a relic of the Big Bang; while the cosmic microwave background radiation (CMB) dates from when the universe was 379,000 years old, the C ν B decoupled (separated) from matter when the universe was just one second old.

  7. The Devastating Consequences Of A 'Small' Rise In Global ...

    data.huffingtonpost.com/2015/11/two-degrees-will...

    World leaders are meeting in Paris this month in what amounts to a last-ditch effort to avert the worst ravages of climate change. Climatologists now say that the best case scenario — assuming immediate and dramatic emissions curbs — is that planetary surface temperatures will increase by at least 2 degrees Celsius in the coming decades.

  8. Neutron star - Wikipedia

    en.wikipedia.org/wiki/Neutron_star

    The temperature inside a newly formed neutron star is from around 10 11 to 10 12 kelvin. [25] However, the huge number of neutrinos it emits carries away so much energy that the temperature of an isolated neutron star falls within a few years to around 10 6 kelvin. [25] At this lower temperature, most of the light generated by a neutron star is ...

  9. UN: Antarctic high temp records will take months to verify - AOL

    www.aol.com/news/un-antarctic-high-temp-records...

    Record high temperatures reportedly measured in Antarctica will take months to verify, the U.N. weather agency said Sunday. A spokesman for the World Meteorological Organization said the ...