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<p><b>New page</b></p><div>{{More footnotes|date=March 2009}}<br />
'''R-parity''' is a concept in [[particle physics]]. In the [[Minimal Supersymmetric Standard Model]] [[baryon number]] and [[lepton number]] are no longer conserved by all of the renormalizable couplings<br />
in the theory. Since baryon number and lepton number conservation have been tested very precisely, these couplings need to be very small in order not to be in conflict with experimental data. R-parity is a <math>\mathbb{Z}_2</math> symmetry acting on the [[Minimal Supersymmetric Standard Model]] (MSSM) fields that forbids these couplings and can be defined as:<br />
<br />
:''P<sub>R</sub>'' = (-1)<sup>''2s+3B+L''</sup>.<br />
<br />
Or, equivalently, as: <br />
<br />
:''P<sub>R</sub>'' = (-1)<sup>''3(B-L)+2s''</sup>.<br />
<br />
With [[Spin (physics)|spin]] s, baryon number B, and lepton number L.<ref>[http://arxiv.org/pdf/hep-ph/9709356 A Supersymmetry Primer] by S. Martin, 1999</ref> All Standard Model particles have R-parity of 1 while supersymmetric particles have R-parity -1.<br />
<br />
==Dark matter candidate==<br />
With R-parity being preserved, the lightest supersymmetric particle ([[Lightest Supersymmetric Particle|LSP]]) cannot decay. This lightest particle (if it exists) may therefore account for the observed missing mass of the universe that is generally called [[dark matter]].{{Citation needed|date=March 2009}} In order to fit observations, it is assumed that this particle has a mass of 100 GeV to 1 TeV, is neutral and only interacts through [[weak force|weak interactions]] and [[Gravitation|gravitational interactions]]. It is often called a [[Weakly interacting massive particle]] or WIMP.<br />
<br />
Typically the dark matter candidate of the MSSM is an admixture of the electroweak [[gaugino]]s and [[Higgsino]]s and is called a [[neutralino]]. In extensions to the MSSM it is possible to have a [[sneutrino]] be the dark matter candidate. Another possibility is the [[gravitino]], which only interacts via [[Gravitation|gravitational interactions]] and does not require strict R-parity.<br />
<br />
==R-parity violating couplings of the MSSM==<br />
<br />
The renormalizable R-parity violating couplings of the MSSM are<br />
<br />
* <math> \int d^2\theta\; \lambda_1\; U^c D^c D^c </math> violates B by 1 unit<br />
The strongest constraint involving this coupling alone is from the non-observation of [[Antineutron|neutron - antineutron oscillations.]]<br />
<br />
* <math>\int d^2 \theta\; \lambda_2\; Q D^c L </math> violates L by 1 unit<br />
The strongest constraint involving this coupling alone is the violation universality of [[Fermi coupling constant|Fermi constant]] <math>G_F</math> in quark and leptonic charged current decays.<br />
<br />
* <math>\int d^2 \theta\; \lambda_3\; L E^cL </math> violates L by 1 unit<br />
The strongest constraint involving this coupling alone is the violation universality of Fermi constant in leptonic charged current decays.<br />
<br />
* <math>\int d^2 \theta\; \kappa\; L H_u</math> violates L by 1 unit<br />
The strongest constraint involving this coupling alone is that it leads to a large neutrino mass.<br />
<br />
While the constraints on single couplings are reasonably strong, if multiple couplings are combined together, they lead to [[proton decay]]. Thus there are further maximal bounds on values of the couplings from maximal bounds on proton decay rate.<br />
<br />
==Proton decay==<br />
Without baryon and lepton number being conserved and taking [[Big O notation|<math>\mathcal{O}(1)</math>]] couplings for the R-parity violating couplings, the proton can decay in approximately <br />
<math>10^{-2}</math> seconds or if [[minimal flavor violation]] is assumed the proton lifetime can be extended to<br />
1 year. Since the proton lifetime is observed to be greater than <math>10^{33} - 10^{34}</math> years (depending on the exact decay channel), this would highly disfavour the model. <br />
R-parity sets all of the renormalizable baryon and lepton number violating couplings to zero and the proton is stable at the renormalizable level and the lifetime of the proton is increased to <math>10^{32}</math> years and is nearly consistent with current observational data. <br />
<br />
[[Image:R-parity violating decay.svg|frame|right]]<br />
<br />
Because proton decay involves violating both lepton and baryon number simultaneously, no single renormalizable R-parity violating coupling leads to proton decay. This has motivated the study of R-parity violation where only one set of the R-parity violating couplings are non-zero which is sometimes called the single coupling dominance hypothesis.<br />
<br />
==Possible origins of R-parity==<br />
<br />
A very attractive way to motivate R-parity is with a B-L continuous gauge symmetry which is spontaneously broken at a scale inaccessible to current experiments. A continuous <math>U(1)_{B-L}</math> forbids renormalizable terms which violate B and L.<ref>R.N. Mohapatra, Phys. Rev. D 34, 3457 (1986); A. Font, L.E. Ibanez and F. Quevedo, Phys. Lett. B 228, 79 (1989)</ref><ref>S.P. Martin Phys. Rev. D 46, 2769 (1992) http://arxiv.org/pdf/hep-ph/9207218; S.P. Martin Phys. Rev. D 54, 2340 (1996) http://arxiv.org/pdf/hep-ph/9602349</ref> If <math>U(1)_{B-L}</math> is only broken by scalar vacuum expectation values (or other order parameters) that carry even integer values of 3(B-L), then there exist an exactly conserved discrete remnant subgroup which has the desired properties.<ref>P. Fayet, NucI. Phys. B90 (1975) 104.; A. Salam and J. Strathdee, Nucl. Phys. B87 (1975) 85; G.R. Farrar and S. Weinberg, Phys. Rev. D27 (1983) 2732; P. Fayet, Phys. Lett. 69B (1977) 489; G. Farrar and P. Fayet, Phys. Lett. 76B (1978) 575</ref> The crucial issue is to determine whether the [[sneutrino]] (the supersymmetric partner of neutrino), which is odd under R-parity, developes a vacuum expectation value. It can be shown, on phenomenological grounds, that this cannot happen in any theory where <math>U(1)_{B-L}</math> is broken at a scale much above the [[electroweak]] one. This is true in any theory based on a large-scale [[seesaw mechanism]].<ref><br />
C.S. Aulakh, A. Melfo, A. Rasin and G. Senjanovic,<br />
Physics Letters B459 (1999), 557;<br />
"http://arxiv.org/abs/hep-ph/9712551" <br />
</ref> As a consequence, in such theories R-parity remains exact at all energies. <br />
<br />
This phenomenon can arise as an automatic symmetry in [[SO(10)]] [[grand unified theory|grand unified theories]]. This natural occurrence of R-parity is possible because in SO(10) the Standard Model fermions arise from the 16-dimensional [[spinor representation]], while the Higgs arises from a 10 dimensional vector representation. In order to make an SO(10) invariant coupling, one must have an even number of spinor fields (i.e. there is a spinor parity). After GUT symmetry breaking, this spinor parity descends into R-parity so long as no spinor fields were used to break the GUT symmetry. Explicit examples of such SO(10) theories have been constructed.<ref><br />
C.S. Aulakh, B. Bajc, A. Melfo, A Rasin and G. Senjanovic, <br />
Nuclear Physics B597 (2001), 89,<br />
"http://arxiv.org/abs/hep-ph/0004031" ; C.S. Aulakh, B. Bajc, A. Melfo, G. Senjanovic and F. Vissani,<br />
Physics Letters B588 (2004), 196,<br />
"http://arxiv.org/abs/hep-ph/0306242".<br />
</ref><br />
<br />
==References==<br />
{{Reflist}}<br />
<br />
==External links==<br />
*[http://arxiv.org/abs/hep-ph/0406039 R-parity Violating Supersymmetry] by R.Barbier, C.Berat, M.Besancon, M.Chemtob, A.Deandrea, E.Dudas, P.Fayet, S.Lavignac, G.Moreau, E.Perez, and Y.Sirois.<br />
*[http://xstructure.inr.ac.ru/x-bin/theme3.py?level=2&index1=236116 R-parity Violating on arxiv.org]<br />
*[http://cepa.fnal.gov/psm/simulation/mcgen/lund/pythia_manual/pythia6.3/pythia6301/node114.html R-parity Violating on fnal]<br />
<br />
{{DEFAULTSORT:R-Parity}}<br />
[[Category:Particle physics]]<br />
[[Category:Supersymmetry]]</div>en>Giftlite