Search for neutral Higgs bosons from supersymmetry in Z decays

Décamp, D.; Deschizeaux, B.; Lees, J. P.; Minard, M.-N.; Crespo, J.M.; Delfino, M.; Fernández, E.; Martı́nez, M.; Miquel, R.; Mir, L. M.; Orteu, S.; Pacheco, A.; Perlas, J. A.; Tubau, E.; Catanesi, M. G.; Palma, M. De; Farilla, A.; Iaselli, G.; Mäggi, G.; Natali, S.; Nuzzo, S.; Ranieri, A.; Raso, G.; Romanò, F.; Ruggieri, F.; Selvaggi, G.; Silvestris, L.; Tempesta, P.; Zito, G.; Hu, H.; Huang, D.; Lin, J.; Ruan, T.; Wang, T.; Wu, W.; Xie, Y.; Xu, D.; Xu, R.; Zhang, J.; Zhao, W.; Albrecht, H.; Atwood, W. B.; Bird, F.; Blucher, E.; Burnett, T. H.; Charity, T.; Drevermann, H.; Garrido, Ll.; Grab, C.; Hagelberg, R.; Haywood, S. J.; Jost, B.; Kasemann, M.; Kellner, G.; Knobloch, J.; Lacourt, A.; Lehraus, I.; Löhse, T.; Lüke, D.; Marchioro, A.; Mató, P.; May, J.; Minten, A.; Miotto, A.; Palazzi, P.; Pepe-Altarelli, M.; Ranjard, F.; Roth, A.; Rothberg, J.; Rotscheidt, H.; Rüden, W. von; Denis, R. St.; Schlatter, D.; Takashima, M.; Talby, M.; Taureg, H.; Tejessy, W.; Wachsmuth, H.; Wheeler, S.; Wiedenmann, W.; Witzeling, W.; Wotschack, J.; Ajaltouni, Z.; Bardadin-Otwinowska, M.; Falvard, A.; Henrard, P.; Jousset, J.; Michel, B.; Montret, J. C.; Pallin, D.; Perret, P.; Proriol, J.; Prulhière, F.; Hansen, J. D.; Hansen, J. R.; Hansen, P. H.; Möllerud, R.; Petersen, G.; Simopoulou, E.; Vayaki, A.; Badier, J.; Blondel, A.; Bonneaud, G. R.; Bourotte, J.; Braems, F.; Brient, J. C.; Ciocci, M. A.; Fouque, G.; Guirlet, R.; Rougé, A.; Rumpf, M.; Tanaka, R.; Videau, H.; Videau, I.; Candlin, D. J.; Conti, A.; Parrini, G.; Corden, M.; Georgiopoulos, C.; Goldman, J.H.; Ikeda, M.; Lannutti, J.; Levinthal, D.; Mermikides, M.; Sawyer, L.; Stimpfl, G.; Antonelli, A.; Baldini, R.; Bencivenni, G.; Bologna, G.; Bossi, F.; Campana, P.; Capon, G.; Chiarella, V.; Ninno, G. De; D’Ettorre-Piazzoli, B.; Felici, G.; Laurelli, P.; Mannocchi, G.; Murtas, F.; Murtas, F.; Nicoletti, G.; Picchi, P.; Zografou, P.; Altoon, B.; Boyle, O.; Halley, A.W.; Have, I. ten; Hearns, J. L.; Hughes, I. S.; Lynch, J.G.; Morton, W. T.; Raine, C.; Scarr, J. M.; Smith, K. M.; Thompson, A. S.; Brandl, B.; Braun, O.; Geiges, R.; Geweniger, C.; Hanke, P.; Hepp, V.; Kluge, E.-E.; Maumary, Y.; Panter, M.; Putzer, A.; Rensch, B.; Stahl, A.; Tittel, K.; Wunsch, M.; Belk, A. T.; Beuselinck, R.; Binnie, D. M.; Cameron, W.; Cattaneo, M.; Dornan, P. J.; Dugeay, S.; Forty, R.; Greene, A. M.; Hassard, J. F.; Patton, S.; Sedgbeer, J. K.; Taylor, G. P.; Tomalin, I. R.; Wright, A. G.; Girtler, P.; Kühn, D.; Rudolph, G.; Bowdery, C. K.; Brodbeck, T. J.; Finch, A. J.; Foster, F.; Hughes, G.; Keemer, N. R.; Nuttall, M.; Rowlingson, B. S.; Sloan, T.; Snow, S. W.; Barczewski, T.; Bauerdick, L. A. T.; Kleinknecht, K.; Renk, B.; Roehn, S.; Sander, H. G.; Schmelling, M.; Steeg, F.; Albanèse, J.P.; Aubert, J.J.; Benchouk, C.; Bonissent, A.; Courvoisier, D.; Etienne, F.; Matsinos, E.; Papalexiou, S.; Payre, P.; Pietrzyk, B.; Qian, Z.; Blum, W.; Cattaneo, P. W.; Cowan, G.; Dehning, B.; Dietl, H.; Fernández-Bosman, M.; Hauff, D.; Jahn, A.; Lange, E.; Lütjens, G.; Lütz, G.; Männer, W.; Moser, H. G.; Pan, Y.; Richter, R.; Schwarz, A. S.; Settles, R.; Stiegler, U.; Stierlin, U.; Thomas, J. P.; Waltermann, G.; Bertín, V.; Bouard, G. de; Boucrot, J.; Callot, O.; Chen, X.; Cordier, A.; Davier, M.; Ganis, G.; Grivaz, J.-F.; Heusse, P.; Janot, P.; Journé, V.; Kim, D. W.; Lefrançois, J.; Lutz, A. M.; Veillet, J. J.; Zomer, F.; Amendolia, S. R.; Bagliesi, G.; Batignani, G.; Bosisio, L.; Bottigli, U.; Bradaschia, C.; Ferrante, I.; Fidecaro, F.; Foà, L.; Focardi, E.; Forti, F.; Giassi, A.; Giorgi, M. A.; Ligabue, F.; Lusiani, A.; Mannelli, E. B.; Marrocchesi, P. S.; Messineo, A.; Palla, F.; Sanguinetti, G.; Scapellato, S.; Steinberger, J.; Тенчини, Р.; Tonelli, G.; Triggiani, G.; Carter, J. M.; Green, M. G.; March, P.V.; Medcalf, T.; Saich, M.; Strong, J. A.; Thomas, R. M.; Wildish, T.; Botterill, D.; Clifft, R. W.; Edgecock, R.; Edwards, M.; Fisher, S. M.; Harvey, J.; Jones, T. J.; Norton, P. R.; Salmon, D. P.; Thompson, J.C.; Aubourg, E.; Bloch-Devaux, B.; Colas, P.; Klopfenstein, C.; Lançon, E.; Locci, E.; Loucatos, S.; Mirabito, L.; Monnier, E.; Pérez, P.; Perrier, Frédéric; Rander, J.; Renardy, J. F.; Roussarie, A.; Schuller, J. P.; Ashman, J. G.; Booth, C. N.; Combley, F.; Dinsdale, M.; Martin, J. P.; Parker, D.; Thompson, L.F.; Brandt, Siegmund; Burkhardt, Hans; Grupen, C.; Meinhard, H.; Neugebauer, E.; Schäfer, U.; Seywerd, H.; Gobbo, B.; Liello, F.; Milotti, E.; Ragusa, F.; Rolandi, G.; Bellantoni, L.; Boudreau, J.; Cinabro, D.; Conway, J.; Cowen, D. F.; Feng, Z.; Harton, J. L.; Hilgart, J.; Jared, R. C.; Johnson, R.P.; LeClaire, B. W.; Pan, Y. B.; Parker, T.E.; Pater, J. R.; Saadi, Y.; Sharma, V.; Wear, J.; Weber, F. V.; Wu, S. L.; Xue, S.; Zobernig, G.

doi:10.1016/0370-2693(90)91447-j

Cited by 64 publications

(2 citation statements)

References 41 publications

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“…This is now called: the EGM effect (from the initials of Evolution of Gaugino Masses). To compute the energy threshold using only the 'running' of the gauge couplings (α 1 , α 2 , α 3 ) corresponds to neglecting nearly three orders of magnitude in the energy threshold for the discovery of the first particle (the lightest) of the Superworld [12][13][14][15][16][17][18][19][20][21][22][23][24][25][26][27][28].…”

Section: The Unification Of All Fundamental Forcesmentioning

confidence: 99%

Time-Shift in the Opera Setup: Proof Against Superluminal Neutrinos Without the Need of Knowing the Cern–lngs Distance and Reminiscences on the Origin of the Gran Sasso Lab, of the Third Neutrino and of the "Teramo Anomaly"

Zichichi¹

2012

Int. J. Mod. Phys. A

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The LVD time stability allows one to establish a time-shift in the OPERA experiment, thus providing the first proof against superluminal neutrinos, using the horizontal muons of the "Teramo Anomaly." This proof is particularly interesting since it does not need the knowledge of the distance between the location at which the neutrinos are produced (CERN) and the location they are detected (LNGS). Since the superluminal neutrinos generated in the physics community a vivid interest in good and bad behavior in physics research, the author thought it was appropriate to recall the origin of the Gran Sasso Lab, of the third neutrino, of the horizontal muons due to the "Teramo Anomaly" and of the oscillation between leptonic flavors, when the CERN–Gran Sasso neutrino beam was included in the project for the most powerful underground laboratory in the world.

show abstract

Section: The Unification Of All Fundamental Forcesmentioning

confidence: 99%

Time-Shift in the Opera Setup: Proof Against Superluminal Neutrinos Without the Need of Knowing the Cern–lngs Distance and Reminiscences on the Origin of the Gran Sasso Lab, of the Third Neutrino and of the "Teramo Anomaly"

Zichichi¹

2012

Int. J. Mod. Phys. A

View full text Add to dashboard Cite

show abstract

Section: The Unification Of All Fundamental Forcesmentioning

confidence: 99%

Time-Shift in the OPERA Setup: Proof against Superluminal Neutrinos without the need of knowing the CERN-LNGS distance and Reminiscences on the Origin of the Gran Sasso Lab, of the Third Neutrino and of the "Teramo Anomaly"

Zichichi

2012

Asia Pac. Phys. Newslett.

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The LVD time stability allows one to establish a time-shift in the OPERA experiment, thus providing the first proof against superluminal neutrinos, using the horizontal muons of the "Teramo Anomaly." This proof is particularly interesting because it does not need the knowledge of the distance between the location at which the neutrinos are produced (CERN) and the location they are detected (LNGS). Since the superluminal neutrinos generated in the physics community a vivid interest in good and bad behavior in physics research, the author thought it was appropriate to recall the origin of the Gran Sasso Lab, of the third neutrino, of the horizontal muons due to the "Teramo Anomaly" and of the oscillation between leptonic flavors, when the CERN-Gran Sasso neutrino beam was included in the project for the most powerful underground laboratory in the world.

show abstract

Constraints on SUSY models from LEP

Ellwanger

1990

Z. Phys. C - Particles and Fields

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Search for neutral Higgs bosons from supersymmetry in Z decays

Cited by 64 publications

References 41 publications

Time-Shift in the Opera Setup: Proof Against Superluminal Neutrinos Without the Need of Knowing the Cern–lngs Distance and Reminiscences on the Origin of the Gran Sasso Lab, of the Third Neutrino and of the "Teramo Anomaly"

Time-Shift in the Opera Setup: Proof Against Superluminal Neutrinos Without the Need of Knowing the Cern–lngs Distance and Reminiscences on the Origin of the Gran Sasso Lab, of the Third Neutrino and of the "Teramo Anomaly"

Time-Shift in the OPERA Setup: Proof against Superluminal Neutrinos without the need of knowing the CERN-LNGS distance and Reminiscences on the Origin of the Gran Sasso Lab, of the Third Neutrino and of the "Teramo Anomaly"

Constraints on SUSY models from LEP

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