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22 results on '"14.80.Mz"'

13. Study of 2β-decay of 100Mo and 82Se using the NEMO3 detector

Author

Arnold, R., Augier, C., Baker, J., Barabash, A., Brudanin, V., Caffrey, A. J., Egorov, V., Guyonnet, J. L., Hubert, F., Hubert, Ph., Jenner, L., Jollet, C., Jullian, S., Klimenko, A., Kochetov, O., Konovalov, S., Kovalenko, V., Lalanne, D., Leccia, F., Linck, I., Longuemare, C., Lutter, G., Marquet, Ch., Mauger, F., Nicholson, H. W., Ohsumi, H., Piquemal, F., Reyss, J. -L., Saakyan, R., Sarazin, X., Scheibling, F., Shitov, Yu., Simard, L., Smolnikov, A., Stekl, I., Suhonen, J., Sutton, C. S., Szklarz, G., Timkin, V., Thomas, J., Tretyak, V., Umatov, V., Vala, L., Vanyushin, I., Vasiliev, S., Vasilyev, V., Vorobel, V., and Vylov, Ts.

Published
2004
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19. Constraints on spin-dependent short-range interactions using gravitational quantum levels of ultracold neutrons

Author

K.V. Protasov, Guillaume Pignol, S. Baeßler, Valery Nesvizhevsky, A. Yu. Voronin, Institut Laue-Langevin (ILL), ILL, Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), T. Soldner, V. Nesvizhevsky, C. Plonka-Spehr, K. Protasov, K. Schreckenbach, and O. Zimmer

Subjects
Nuclear and High Energy Physics, FOS: Physical sciences, 01 natural sciences, Short range interactions, Gravitation, Nuclear physics, [PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph], 0103 physical sciences, Bound state, Neutron, Nuclear Experiment (nucl-ex), 010306 general physics, Nuclear Experiment, Instrumentation, Quantum, ComputingMilieux_MISCELLANEOUS, Spin-½, Physics, 010308 nuclear & particles physics, Ultra-cold neutrons, 11.30.Er, 14.80.Mz, 04.80.Cc, CP violation, Orders of magnitude (time), Ultracold neutrons
Abstract

In this paper, we discuss a possibility to improve constraints on spin-dependent short-range interactions in the range of 1 - 200 micrometer significantly. For such interactions, our constraints are without competition at the moment. They were obtained through the observation of gravitationally bound states of ultracold neutrons. We are going to improve these constraints by about three orders of magnitude in a dedicated experiment with polarized neutrons using the next-generation spectrometer GRANIT., Comment: 5 pages, 4 figures, accepted for publication in the Proceedings of the International Workshop on Particle Physics with Cold Neutrons, Grenoble, May 2008, to be published in Nucl. Instr. and Meth. A

Published
2009
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20. Search for beta+EC and ECEC processes in 112Sn and beta beta decay of 124Sn to the excited states of 124Te

Author

BARABASH, A. S., HUBERT, Ph., NACHAB, A., KONOVALOV, S. I., VANYUSHIN, I. A., UMATOV, V. I., Institute of Theoretical and Experimental Physics [Moscow] (ITEP), National Research Center 'Kurchatov Institute' (NRC KI), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), and Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
23.40.-s, 14.80.Mz, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Nuclear Experiment
Abstract

Limits on $\beta^+$EC and ECEC processes in $^{112}$Sn and on $\beta^-\beta^-$ decay of $^{124}$Sn to the excited states of $^{124}$Te have been obtained using a 380 cm$^3$ HPGe detector and an external source consisting of natural tin. A limit with 90% C.L. on the $^{112}$Sn half-life of $0.92\times 10^{20}$ y for the ECEC(0$\nu$) transition to the $0^+_3$ excited state in $^{112}$Cd (1871.0 keV) has been established. This transition is discussed in the context of a possible enhancement of the decay rate by several orders of magnitude given that the ECEC$(0\nu)$ process is nearly degenerate with an excited state in the daughter nuclide. Prospects for investigating such a process in future experiments are discussed. The $\beta^-\beta^-$ decay limits for $^{124}$Sn to the excited states of $^{124}$Te were obtained on the level of $(0.8-1.2)\times 10^{21}$ y at the 90% C.L., Comment: 17 pages, 5 figures

Published
2008

21. Nucleon-Nucleon Bremsstrahlung emission of massive Axion

Author

Fabrizio Nesti, Maurizio Giannotti, M., Giannotti, and Nesti, Fabrizio

Subjects
Nuclear and High Energy Physics, Particle physics, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Luminosity, Nuclear physics, High Energy Physics::Theory, High Energy Physics - Phenomenology (hep-ph), 95.30.Cq, Nuclear Experiment, Axion, Physics, Astrophysics (astro-ph), High Energy Physics::Phenomenology, Bremsstrahlung, Massless particle, Supernova, High Energy Physics - Phenomenology, 14.80.Mz, Production (computer science), 97.60.Bw, 14.80.Mz, 95.30.Cq, 97.60.Bw, Nucleon, Gamma-ray burst
Abstract

We consider the problem of axion production by bremsstrahlung emission in a nuclear medium. The usual assumption of a massless axion is replaced by more general hypotheses, so that we can describe the emission process for axions with mass up to a few MeV. We point out that in certain physical situations the contribution from non-zero mass is non-negligible. In particular, in the mechanism for the production of Gamma Ray Bursts via emission of heavy axions the axion mass m_a ~ 1MeV is comparable with the temperature of the nuclear medium and thus can not be disregarded. Looking at our results we find, in fact, a fairly considerable reduction of the axion luminosity in that mechanism., 16 pages, 5 figures

Published
2005

22. Study of 2$\beta$-decay of $^{100}$Mo and $^{82}$Se using the NEMO3 detector

Author

Arnold, R., Augier, C., Baker, J., Barabash, A., Brudanin, V., Caffrey, A.J., Egorov, V., Guyonnet, J.L., Hubert, F., Hubert, P., Jenner, L., Jollet, C., Jullian, Sophie, Klimenko, A., Kochetov, O., Konovalov, S., Kovalenko, V., Lalanne, D., Leccia, F., Linck, I., Longuemare, C., Lutter, G., Marquet, Ch., Mauger, F., Nicholson, H.W., Ohsumi, H., Piquemal, F., Reyss, J.-L., Saakyan, R., Sarazin, X., Scheibling, F., Shitov, Yu., Simard, L., Smolnikov, A., Stekl, I., Suhonen, J., Sutton, C.S., Szklarz, G., Timkin, V., Thomas, J., Tretyak, V., Umatov, V., Vala, L., Vanyushin, I., Vasiliev, S., Vasilyev, V., Vorobel, V., Vylov, Ts., Institut de Recherches Subatomiques (IReS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Cancéropôle du Grand Est-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de physique corpusculaire de Caen (LPCC), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-École Nationale Supérieure d'Ingénieurs de Caen (ENSICAEN), Normandie Université (NU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), NEMO, Heyd, Yvette, Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), and Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)

Subjects
[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], 14.80.Mz, 23.40.-s
Published
2004

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