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Urca process

From Wikipedia, the free encyclopedia
Phenomenon in astroparticle physics

Inastroparticle physics, anUrca process is a reaction which emits aneutrino and which is assumed to take part in cooling processes inneutron stars andwhite dwarfs. The process was first discussed byGeorge Gamow andMário Schenberg while they were visiting a casino namedCassino da Urca inUrca,Rio de Janeiro. As Gamow recounts in his autobiography, the name was chosen in part to commemorate the gambling establishment where the two physicists had first met, and "partially because the Urca Process results in a rapid disappearance of thermal energy from the interior of a star, similar to the rapid disappearance of money from the pockets of the gamblers on the Casino de Urca."[1] In Gamow's South Russian dialect,urca (Russian:урка) can also mean a robber or gangster.[2][3]

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
B
2
+

+
ν
l
,
B
2
+

B
1
+
ν
l
,

where B
1
and B
2
arebaryons,

is alepton, and
ν
l
(and
ν
l
) are (anti-)neutrinos. The baryons can benucleons (free or bound),hyperons like
Λ
,
Σ
and
Ξ
, or members of the
Δ
isobar. Thelepton is either anelectron or amuon.

The Urca process is especially important in the cooling of white dwarfs, where a lepton (usually an electron) is absorbed by the nucleus of an ion and then convectively carried away from the core of a star. Then, a beta decay occurs. Convection then carries the element back into the interior of the star, and the cycle repeats many times. Because the neutrinos emitted during this process are unlikely to be reabsorbed, this is effectively a cooling mechanism for white dwarfs.[4]

The process can also be essential in the cooling of neutron stars. If a neutron star contains a central core in which the direct Urca-process is operative, the cooling timescale shortens by many orders of magnitude.[5]

References

[edit]
  1. ^Gamow, George (1970).My World Line: An Informal Autobiography. New York: The Viking Press. p. 137.
  2. ^D. Darling."Urca process".The Internet Encyclopedia of Science. Retrieved2 March 2010.
  3. ^D. K. Nadyozhin (1995). "Gamow and the physics and evolution of stars".Space Science Reviews.74 (3–4):455–461.Bibcode:1995SSRv...74..455N.doi:10.1007/BF00751432.S2CID 122987210.
  4. ^M. Brueggen; A. Kercek (10 January 2000)."The convective URCA process in white dwarfs".Max Planck Institute. Archived fromthe original on 12 January 2010. Retrieved5 February 2010.
  5. ^P. Haensel (1995). "Urca processes in dense matter and neutron star cooling".Space Science Reviews.74 (3–4):427–436.Bibcode:1995SSRv...74..427H.doi:10.1007/BF00751429.S2CID 115313950.
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