000026880 001__ 26880
000026880 005__ 20140130004430.0
000026880 037__ $$9arXiv$$ahep-ph/0405237$$chep-ph
000026880 035__ $$9arXiv$$zoai:arXiv.org:hep-ph/0405237
000026880 037__ $$aSISSA-34-2004-EP
000026880 035__ $$9DESY$$zD04-13373
000026880 035__ $$9SPIRESTeX$$zBilenky:2004um
000026880 100__ $$aBilenky, S.M.$$uSISSA, Trieste$$uDubna, JINR
000026880 245__ $$aNuclear matrix elements of 0 nu beta beta decay: Possible test of the calculations
000026880 246__ $$9arXiv$$aNuclear matrix elements of 0nu beta beta-decay: Possible test of the calculations.
000026880 269__ $$c2004-05
000026880 300__ $$a12
000026880 520__ $$aA possible model independent test of the theoretically calculated nuclear matrix elements of $0\nu\beta\beta$-decay is proposed. The test can be accomplished if $0\nu\beta\beta$-decay of three (or more) nuclei is observed. The selection of the nuclei for the next generation of $0\nu\beta\beta$-decay experiments should be done taking into account {\it also} considerations regarding the possibility to test the nuclear matrix element calculations.
000026880 65017 $$2INSPIRE$$aTheory-Nucl
000026880 65017 $$2INSPIRE$$aPhenomenology-HEP
000026880 695__ $$2INSPIRE$$adouble-beta decay: (0neutrino)
000026880 695__ $$2INSPIRE$$anucleus: lifetime
000026880 695__ $$2INSPIRE$$anuclear properties
000026880 695__ $$2INSPIRE$$aneutrino: Majorana
000026880 695__ $$2INSPIRE$$aneutrino: mass
000026880 695__ $$2INSPIRE$$aneutrino: mixing angle
000026880 695__ $$2INSPIRE$$aneutrino: solar
000026880 695__ $$2INSPIRE$$aneutrino: cosmic radiation
000026880 695__ $$2INSPIRE$$anumerical calculations
000026880 700__ $$aPetcov, S.T.$$uINFN, Trieste$$uSISSA, Trieste
000026880 909CO $$ooai:jdsweb.jinr.ru:26880$$pglobal
000026880 961__ $$x2004-05-25
000026880 961__ $$c2005-10-19
000026880 970__ $$aSPIRES-5885400
000026880 980__ $$aArxiv
000026880 980__ $$aCiteable
000026880 980__ $$aCORE
000026880 999C5 $$rhep-ex/9807003$$sPhys.Rev.Lett.,81,1562
000026880 999C5 $$rhep-ex/9812014$$sPhys.Rev.Lett.,82,2644
000026880 999C5 $$rhep-ex/0009001$$sPhys.Rev.Lett.,85,3999
000026880 999C5 $$rnucl-ex/0106015$$sPhys.Rev.Lett.,87,071301
000026880 999C5 $$rnucl-ex/0204008$$sPhys.Rev.Lett.,89,011301
000026880 999C5 $$rnucl-ex/0204009$$sPhys.Rev.Lett.,89,011302
000026880 999C5 $$rnucl-ex/0309004$$sPhys.Rev.Lett.,92,181301
000026880 999C5 $$rhep-ex/0212021$$sPhys.Rev.Lett.,90,021802
000026880 999C5 $$rhep-ex/0104049$$sPhys.Rev.,D64,112007
000026880 999C5 $$sNucl.Phys.Proc.Suppl.,118,157
000026880 999C5 $$sSov.Phys.JETP,6,429
000026880 999C5 $$sSov.Phys.JETP,7,172
000026880 999C5 $$sProg.Theor.Phys.,28,870
000026880 999C5 $$rhep-ex/9907037$$sPhys.Lett.,B466,415
000026880 999C5 $$rhep-ex/0301017$$sEur.Phys.J.,C27,331
000026880 999C5 $$rhep-ph/0309174$$sPhys.Lett.,B583,134
000026880 999C5 $$sPhys.Rev.,D64,1120
000026880 999C5 $$sRev.Mod.Phys.,59,671
000026880 999C5 $$sPhys.Lett.,B94,495
000026880 999C5 $$sNucl.Phys.,B282,589
000026880 999C5 $$sProg.Theor.Phys.Suppl.,83,1
000026880 999C5 $$rhep-ph/9901215$$sJ.Phys.G,G24,2139
000026880 999C5 $$sPhys.Rept.,300,123
000026880 999C5 $$rhep-ph/0209347$$sPhys.Rept.,361,1
000026880 999C5 $$rhep-ph/0202264$$sAnn.Rev.Nucl.Part.Sci.,52,115
000026880 999C5 $$rhep-ph/0211332$$sNucl.Phys.Proc.Suppl.,114,141
000026880 999C5 $$rhep-ph/0211462$$sPhys.Rept.,379,69
000026880 999C5 $$rhep-ph/0102265$$sPhys.Rev.,D64,053010
000026880 999C5 $$sPhys.Lett.,B102,323
000026880 999C5 $$rhep-ph/9311204$$sPhys.Lett.,B322,109
000026880 999C5 $$rhep-ph/9907234$$sPhys.Lett.,B465,193
000026880 999C5 $$sRev.Mod.Phys.,74,663
000026880 999C5 $$sPhys.Rev.,D66,010001
000026880 999C5 $$rhep-ph/0103062$$sEur.Phys.J.,A12,147
000026880 999C5 $$rhep-ph/0201231$$sMod.Phys.Lett.,A16,2409
000026880 999C5 $$rhep-ex/0202018$$sMod.Phys.Lett.,A17,1475
000026880 999C5 $$rhep-ph/0404088$$sPhys.Lett.,B586,198
000026880 999C5 $$rphysics/0402115$$sNucl.Instrum.Meth.,A536,79
000026880 999C5 $$rhep-ph/9604364$$sPhys.Rev.,D54,4432
000026880 999C5 $$rhep-ph/0110287$$sPhys.Lett.,B524,319
000026880 999C5 $$sNucl.Phys.,B659,359
000026880 999C5 $$rhep-ph/0205022$$sPhys.Lett.,B544,239
000026880 999C5 $$rhep-ph/0212113$$sPhys.Lett.,B558,141
000026880 999C5 $$rhep-ph/0310003$$sPhys.Lett.,B580,280
000026880 999C5 $$rhep-ph/0402250$$sPhys.Rev.,D70,033003
000026880 999C5 $$rhep-ex/0109033
000026880 999C5 $$sNucl.Phys.,A719,153
000026880 999C5 $$rastro-ph/0310723$$sPhys.Rev.,D69,103501
000026880 999C5 $$rhep-ph/0008044$$sNucl.Phys.,B597,110
000026880 999C5 $$rhep-ph/0209059$$sPhys.Lett.,B549,177
000026880 999C5 $$rhep-ph/0308034
000026880 999C5 $$rnucl-th/0208005$$sNucl.Phys.,A729,867
000026880 999C5 $$rnucl-th/0402046$$sRev.Mod.Phys.,77,427
000026880 999C5 $$rnucl-th/0305005$$sPhys.Rev.,C68,044302
000026880 999C5 $$rhep-ph/0211101$$sPhys.Lett.,B550,154
000026880 999C5 $$sNucl.Phys.,A654,973
000026880 999C5 $$sPhys.Lett.,B453,194
000026880 999C5 $$rhep-ph/0008182$$sPhys.Lett.,B498,35