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==Possible origins of R-parity== A very attractive way to motivate R-parity is with a {{nowrap|{{mvar|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 {{mvar|B}} and {{mvar|L}}.<ref> {{cite journal |last=Mohapatra |first=R.N. |year=1986 |title=New contributions to neutrinoless double-beta decay in supersymmetric theories |journal=[[Physical Review D]] |volume=34 |issue=11 |pages=3457–3461 |bibcode=1986PhRvD..34.3457M |doi=10.1103/PhysRevD.34.3457 |pmid=9957083 }}</ref><ref> {{cite journal |last1=Font |first1=A. |last2=Ibáñez |first2=L.E. |last3=Quevedo |first3=F. |year=1989 |title=Does proton stability imply the existence of an extra Z<sup>0</sup>? |journal=[[Physics Letters B]] |volume=228 |issue=1 |pages=79–88 |bibcode= 1989PhLB..228...79F |doi=10.1016/0370-2693(89)90529-7 |url=https://cds.cern.ch/record/198529/files/198907303.pdf }}</ref><ref> {{cite journal |last1=Martin |first1=S.P. |year=1992 |title=Some simple criteria for gauged R parity |journal=[[Physical Review D]] |volume=46 |issue=7 |pages=R2769–R2772 |arxiv=hep-ph/9207218 |bibcode=1992PhRvD..46.2769M |doi=10.1103/PhysRevD.46.R2769 |pmid=10015267 |s2cid=14821065 }}</ref><ref> {{cite journal |last1=Martin |first1=S.P. |year=1996 |title=Implications of supersymmetric models with natural R-parity conservation |journal=[[Physical Review D]] |volume=54 |issue=3 |pages=2340–2348 |arxiv=hep-ph/9602349 |bibcode= 1996PhRvD..54.2340M |doi=10.1103/PhysRevD.54.2340 |pmid=10020912 |s2cid=5751474 }}</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 {{nowrap|3({{mvar|B − L}})}}, then there exist an exactly conserved discrete remnant subgroup which has the desired properties.<ref> {{cite journal |last1=Fayet |first1=P. |year=1975 |title=Supergauge invariant extension of the Higgs mechanism and a model for the electron and its neutrino |journal=[[Nuclear Physics B]] |volume=90 |pages=104–124 |bibcode= 1975NuPhB..90..104F |doi=10.1016/0550-3213(75)90636-7 }}</ref><ref> {{cite journal |last1=Salam |first1=A. |last2=Strathdee |first2=J. |year=1975 |title=Supersymmetry and fermion-number conservation |journal=[[Nuclear Physics B]] |volume=87 |issue=1 |pages=85–92 |bibcode=1975NuPhB..87...85S |doi=10.1016/0550-3213(75)90253-9 }}</ref><ref> {{cite journal |last1=Farrar |first1=G.R. |last2=Weinberg |first2=S. |year=1983 |title=Supersymmetry at ordinary energies. II. R invariance, Goldstone bosons, and gauge-fermion masses |journal=[[Physical Review D]] |volume=27 |issue=11 |pages=2732 |bibcode=1983PhRvD..27.2732F |doi=10.1103/PhysRevD.27.2732 }}</ref><ref> {{cite journal |last1=Fayet |first1=P. |year=1977 |title=Spontaneously broken supersymmetric theories of weak, electromagnetic and strong interactions |journal=[[Physics Letters B]] |volume=69 |issue=4 |pages=489–494 |bibcode=1977PhLB...69..489F |doi=10.1016/0370-2693(77)90852-8 }}</ref><ref> {{cite journal |last1=Farrar |first1=G.R. |last2=Fayet |first2=P. |year=1978 |title=Phenomenology of the production, decay, and detection of new hadronic states associated with supersymmetry |journal=[[Physics Letters B]] |volume=76 |issue=5 |pages=575 |bibcode=1978PhLB...76..575F |doi=10.1016/0370-2693(78)90858-4 }}</ref> The crucial issue is to determine whether the [[sneutrino]] (the supersymmetric partner of neutrino), which is odd under R-parity, develops 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> {{cite journal |last1=Aulakh |first1=C.S. |last2=Melfo |first2=A. |last3=Rašin |first3=A. |last4=Senjanović |first4=G. |year=1998 |title=Supersymmetry and large scale left-right symmetry |journal=[[Physical Review D]] |volume=58 |issue=11 |pages=115007 |arxiv=hep-ph/9712551 |bibcode=1998PhRvD..58k5007A |doi=10.1103/PhysRevD.58.115007 |s2cid=43296921 }}</ref> As a consequence, in such theories R-parity remains exact at all energies. 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> {{cite journal |last1=Aulakh |first1=C.S. |last2=Bajc |first2=B. |last3=Melfo |first3=A. |last4=Rašin |first4=A. |last5=Senjanović |first5=G. |year=2001 |title=SO(10) theory of R-parity and neutrino mass |journal=[[Nuclear Physics B]] |volume=597 |issue= 1–3|pages=89–109 |arxiv=hep-ph/0004031 |bibcode= 2001NuPhB.597...89A |doi=10.1016/S0550-3213(00)00721-5 |s2cid=119100803 }}</ref><ref> {{cite journal |last1=Aulakh |first1=C.S. |last2=Bajc |first2=B. |last3=Melfo |first3=A. |last4=Senjanović |first4=G. |last5=Vissani |first5=F. |year=2004 |title=The minimal supersymmetric grand unified theory |journal=[[Physics Letters B]] |volume=588 |issue=3–4 |pages=196–202 |arxiv=hep-ph/0306242 |bibcode= 2004PhLB..588..196A |doi=10.1016/j.physletb.2004.03.031 |s2cid=119401374 }}</ref>
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