THE TAU-NEUTRINO AS A MAJORANA PARTICLE

被引:4
作者
CARENA, M
LAMPE, B
WAGNER, CEM
机构
[1] Max Planck Institut für Physik, D-8000 München 40
关键词
D O I
10.1016/0370-2693(93)91579-C
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A Majorana mass term for the tau neutrino would induce neutrino-antineutrino mixing and thereby a process which violates fermion number by two units. We study the possibility of distinguishing between a massive Majorana and a Dirac tau neutrino, by measuring fermion number violating processes in a deep inelastic scattering experiment nup --> tauX. We show that, if the neutrino beam is obtained from the decay of high energetic pions, the probability of obtaining ''wrong sign'' tau leptons is suppressed by a factor O(m(nutau)2theta2/m(mu)2) instead of the naively expected suppression factor theta2m(nutau)2/E(nu)2, where E(nu) is the tau neutrino energy, m(nutau) and m(mu) are the tau neutrino and muon masses, respectively, and theta is the nu(mu)-nu(tau) Mixing angle. If m(nutau) is of the order of 10 MeV and theta is of the order of 0.01-0.04 (the present bounds are (m(nutau) < 35 MeV, theta < 0.04) the next round of experiments may be able to distinguish between Majorana and Dirac tau neutrinos.
引用
收藏
页码:112 / 118
页数:7
相关论文
共 21 条
[1]   MEASUREMENT OF DS-STAR-DS MASS DIFFERENCE [J].
ALBRECHT, H ;
BINDER, U ;
BOCKMANN, P ;
GLASER, R ;
HARDER, G ;
KRUGER, A ;
NIPPE, A ;
SCHAFER, M ;
SCHMIDTPARZEFALL, W ;
SCHRODER, H ;
SCHULZ, HD ;
SEFKOW, F ;
WURTH, R ;
YAGIL, A ;
APPUHN, RD ;
DONKER, JP ;
DRESCHER, A ;
KAMP, D ;
KOLANOSKI, H ;
MATTHIESEN, U ;
SCHECK, H ;
SCHWEDA, G ;
SPAAN, B ;
SPENGLER, J ;
WALTHER, A ;
WEGENER, D ;
GABRIEL, JC ;
RUF, T ;
SCHUBERT, KR ;
STIEWE, J ;
STRAHL, K ;
WALDI, R ;
WERNER, S ;
EDWARDS, KW ;
FRISKEN, WR ;
GILKINSON, DJ ;
GINGRICH, DM ;
KAPITZA, H ;
KIM, PCH ;
KUTSCHKE, R ;
MACFARLANE, DB ;
MCKENNA, JA ;
MCLEAN, KW ;
NILSSON, AW ;
ORR, RS ;
PADLEY, P ;
PARSONS, JA ;
PATEL, PM ;
PRENTICE, JD ;
SEYWERD, HCJ .
PHYSICS LETTERS B, 1988, 207 (03) :349-354
[2]   IMPLICATIONS OF THE GALLEX DETERMINATION OF THE SOLAR NEUTRINO FLUX [J].
ANSELMANN, P ;
HAMPEL, W ;
HEUSSER, G ;
KIKO, J ;
KIRSTEN, T ;
PERNICKA, E ;
PLAGA, R ;
RONN, U ;
SANN, M ;
SCHLOSSER, C ;
WINK, R ;
WOJCIK, M ;
VONAMMON, R ;
EBERT, KH ;
HENRICH, E ;
BALATA, M ;
BELLOTTI, E ;
FERRARI, N ;
LALLA, H ;
STOLARCZYK, T ;
CATTADORI, C ;
CREMONESI, O ;
FIORINI, E ;
PEZZONI, S ;
ZANOTTI, L ;
VONFEILITZSCH, F ;
MOSSBAUER, R ;
SCHANDA, U ;
BERTHOMIEU, G ;
SCHATZMAN, E ;
CARMI, I ;
DOSTROVSKY, I ;
BACCI, C ;
BELLI, P ;
BERNABEI, R ;
DANGELO, S ;
PAOLUZI, L ;
CHARBIT, S ;
CRIBIER, M ;
DUPONT, G ;
GOSSET, L ;
RICH, J ;
SPIRO, M ;
TAO, C ;
VIGNAUD, D ;
HAHN, RL ;
HARTMANN, FX ;
ROWLEY, JK ;
STOENNER, RW ;
WENESER, J .
PHYSICS LETTERS B, 1992, 285 (04) :390-397
[3]  
ASTIER P, 1991, PROPOSAL CERNSPSLC91
[4]   ON THE OSCILLATIONS OF NEUTRINOS WITH DIRAC AND MAJORANA MASSES [J].
BILENKY, SM ;
HOSEK, J ;
PETCOV, ST .
PHYSICS LETTERS B, 1980, 94 (04) :495-498
[5]  
BUNYATOV S, 1990, P WORKSHOP TAU LEPTO
[6]   MASSIVE DIRAC NEUTRINOS AND SN-1987A [J].
BURROWS, A ;
GANDHI, R ;
TURNER, MS .
PHYSICAL REVIEW LETTERS, 1992, 68 (26) :3834-3837
[7]   TIME-REVERSAL VIOLATION IN NEUTRINO OSCILLATION [J].
CABIBBO, N .
PHYSICS LETTERS B, 1978, 72 (03) :333-335
[8]  
DOLGOV A, 1993, UMAC9302 U MICH PREP
[9]  
KAWASAKI M, 1992, OSUTA1092 OH STAT U
[10]  
KAYSER B, 1984, P MORIOND WORKSHOP