Urca-process

Urca-process

In astroparticle physics, an Urca process is a reaction which emits a neutrino and which is assumed to take part in cooling processes in neutron stars. The process was first discussed by George Gamow and Mario Schenberg while they were visiting a casino named "Urca" in Rio de Janeiro. Gamow is reported to have said to Schenberg that "the energy disappears in the nucleus of the supernova as quickly as the money disappeared at that roulette table." In Gamow's South Russian dialect, "urca" can also mean a robber or gangster. [ [http://www.daviddarling.info/encyclopedia/U/Urca_process.html Urca process] , entry in "The Encyclopedia of Astrobiology, Astronomy, and Spaceflight", David Darling, accessed on line July 6, 2007.] [§ 3, [http://www.springerlink.com/content/3137142626548228/ Gamow and the physics and evolution of stars] , D. K. Nadyozhin, "Space Science Reviews", 74, #3–4 (November 1995), pp. 455–461. DOI [http://dx.doi.org/10.1007/BF00751432 10.1007/BF00751432] .]

The direct Urca processes are the simplest neutrino-emitting processes, and are thought to be central in the cooling of neutron stars. They have the general form:::B_1 ightarrow B_2 + l + ar u _l,:::B_2 + l ightarrow B_1 + u _l, where "B"1 and "B"2 are baryons and "l" is a lepton. The baryons can be nucleons (free or bound), hyperons like SubatomicParticle|Lambda, SubatomicParticle|Sigma and SubatomicParticle|Xi, or members of the SubatomicParticle|link=yes|Delta isobar. The lepton is either an electron or a muon.

References


Wikimedia Foundation. 2010.

Игры ⚽ Нужен реферат?

Look at other dictionaries:

  • Mário Schenberg — Born July 2, 1914 Recife, P …   Wikipedia

  • Compact star — In astronomy, the term compact star (sometimes compact object) is used to refer collectively to white dwarfs, neutron stars, other exotic dense stars, and black holes. These objects are all small for their mass. The term compact star is often… …   Wikipedia

  • White dwarf — For other uses, see White dwarf (disambiguation). Image of Sirius A and Sirius B taken by the Hubble Space Telescope. Sirius B, which is a white dwarf, can be seen as a faint pinprick of light to the lower left of the much brighter Sirius A …   Wikipedia

  • Neutron star — redirects here. For the story by Larry Niven, see Neutron Star (short story). Neutron stars crush half a million times more mass than Earth into a sphere no larger than Manhattan. A neutron star is a type of stellar remnant that can result from… …   Wikipedia

  • Magnetar — For the hedge fund, see Magnetar Capital. Artist s conception of a magnetar, with magnetic field lines A magnetar is a type of neutron star with an extremely powerful magnetic field, the decay of which powers the emission of copious amounts of… …   Wikipedia

  • Helium flash — A helium flash is the runaway fusion of helium in the core of low mass stars of less than about 2.25 solar masses and greater than about 0.5 solar mass, or on the surface of an accreting white dwarf star. They may also occur in the outer layers… …   Wikipedia

  • Chandrasekhar limit — When a star starts running out of fuel, it usually cools off and collapses (possibly with a supernova) into one of three compact forms, depending on its total mass: a White Dwarf, a big lump of Carbon and Oxygen atoms, almost like one huge… …   Wikipedia

  • Nova — For other uses, see Nova (disambiguation). Artist s conception of a white dwarf star accreting hydrogen from a larger companion A nova (plural novae) is a cataclysmic nuclear explosion in a star caused by the accretion of hydrogen on to the… …   Wikipedia

  • George Gamow — Born March 4, 1904(1904 03 04) …   Wikipedia

  • Dwarf nova — HT Cas seen in outburst (mag 13.4) on 2010 November 2. Li …   Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”