250 results on '"Navick, X-F"'
Search Results
202. Status of the R&D for surface events rejection in the EDELWEISS experiment
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Navick, X-F, primary and Collaboration, the EDELWEISS, additional
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- 2008
- Full Text
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203. EURECA — the European Future of Dark Matter Searches with Cryogenic Detectors
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Kraus, H., primary, Bauer, M., additional, Bavykina, I., additional, Benoit, A., additional, Blümer, J., additional, Broniatowski, A., additional, Brudanin, V., additional, Burghart, G., additional, Camus, P., additional, Chantelauze, A., additional, Chapellier, M., additional, Chardin, G., additional, Christ, P., additional, Ciemniak, C., additional, Coppi, C., additional, De Jésus, M., additional, De Lesquen, A., additional, Deschamps, H., additional, Di Stefano, P., additional, Dumoulin, L., additional, Eitel, K., additional, von Feilitzsch, F., additional, Fesquet, M., additional, Gascon, J., additional, Gerbier, G., additional, Goldbach, C., additional, Gros, M., additional, Hauff, D., additional, Henry, S., additional, Horn, M., additional, Imber, J., additional, Isaila, C., additional, Jochum, J., additional, Juillard, A., additional, Kimmerle, M., additional, Lanfranchi, J.-C., additional, Lemrani, R., additional, Lubashevsky, A., additional, Luca, M., additional, Malek, M., additional, Marnieros, S., additional, McGowan, R., additional, Mikhailik, V., additional, Navick, X.-F., additional, Niinikoski, T., additional, Nollez, G., additional, Pantic, E., additional, Pari, P., additional, Perevoshchikov, L., additional, Petricca, F., additional, Pfister, S., additional, Potzel, W., additional, Pröbst, F., additional, Rau, W., additional, Ritter, F., additional, Rottler, K., additional, Sanglard, V., additional, Scholl, S., additional, Schwamm, F., additional, Seidel, W., additional, Smolnikov, A., additional, Stern, M., additional, Teshima, M., additional, Tolhurst, B., additional, Westphal, W., additional, Wikus, P., additional, Wolf, J., additional, and Yakushev, E., additional
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- 2007
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204. Identification of backgrounds in the EDELWEISS-I dark matter search experiment
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Fiorucci, S., primary, Benoit, A., additional, Bergé, L., additional, Blümer, J., additional, Broniatowski, A., additional, Censier, B., additional, Chantelauze, A., additional, Chapellier, M., additional, Chardin, G., additional, Collin, S., additional, Defay, X., additional, De Jésus, M., additional, Deschamps, H., additional, Di Stefano, P., additional, Dolgorouky, Y., additional, Dumoulin, L., additional, Eitel, K., additional, Fesquet, M., additional, Gascon, J., additional, Gerbier, G., additional, Goldbach, C., additional, Gros, M., additional, Horn, M., additional, Juillard, A., additional, Lemrani, R., additional, de Lesquen, A., additional, Lubashevskiy, A., additional, Luca, M., additional, Marnieros, S., additional, Mosca, L., additional, Navick, X.-F., additional, Nollez, G., additional, Olivieri, E., additional, Pari, P., additional, Sanglard, V., additional, Schoeffel, L., additional, Schwamm, F., additional, Stern, M., additional, and Yakushev, E., additional
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- 2007
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205. EURECA – THE EUROPEAN UNDERGROUND RARE EVENT CALORIMETER ARRAY
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KRAUS, H., primary, BAUER, M., additional, BAVYKINA, I., additional, BENOIT, A., additional, BLÜMER, J., additional, BRONIATOWSKI, A., additional, BRUDANIN, V., additional, BURGHART, G., additional, CAMUS, P., additional, CHANTELAUZE, A., additional, CHAPELLIER, M., additional, CHARDIN, G., additional, CIEMNIAK, C., additional, COPPI, C., additional, DE JÉSUS, M., additional, DE LESQUEN, A., additional, DESCHAMPS, H., additional, DI STEFANO, P., additional, DUMOULIN, L., additional, EITEL, K., additional, VON FEILITZSCH, F., additional, FESQUET, M., additional, GASCON, J., additional, GERBIER, G., additional, GOLDBACH, C., additional, GROS, M., additional, HAUFF, D., additional, HENRY, S., additional, HORN, M., additional, IMBER, J., additional, INGLEBY, S., additional, ISAILA, C., additional, JOCHUM, J., additional, JUILLARD, A., additional, KIMMERLE, M., additional, LANFRANCHI, J.-C., additional, LEMRANI, R., additional, LUBASHEVSKY, A., additional, LUCA, M., additional, MALEK, M., additional, MARNIEROS, S., additional, MCGOWAN, R., additional, MIKHAILIK, V., additional, NAVICK, X.-F., additional, NIINIKOSKI, T., additional, NOLLEZ, G., additional, PANTIC, E., additional, PARI, P., additional, PEREVOSHCHIKOV, L., additional, PETRICCA, F., additional, PFISTER, S., additional, POTZEL, W., additional, PRÖBST, F., additional, RITTER, F., additional, ROTTLER, K., additional, SANGLARD, V., additional, SCHOLL, S., additional, SCHWAMM, F., additional, SEIDEL, W., additional, SMOLNIKOV, A., additional, STERN, M., additional, TESHIMA, M., additional, TOLHURST, B., additional, WESTPHAL, W., additional, WIKUS, P., additional, WOLF, J., additional, and YAKUSHEV, E., additional
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- 2007
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206. Measurement of the response of heat-and-ionization germanium detectors to nuclear recoils
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Benoit, A., primary, Bergé, L., additional, Blümer, J., additional, Broniatowski, A., additional, Censier, B., additional, Chantelauze, A., additional, Chapellier, M., additional, Chardin, G., additional, Collin, S., additional, Defay, X., additional, De Jésus, M., additional, Deschamps, H., additional, Di Stefano, P., additional, Dolgorouky, Y., additional, Dumoulin, L., additional, Eitel, K., additional, Fesquet, M., additional, Fiorucci, S., additional, Gascon, J., additional, Gerbier, G., additional, Goldbach, C., additional, Gros, M., additional, Horn, M., additional, Juillard, A., additional, Lemrani, R., additional, de Lesquen, A., additional, Luca, M., additional, Marnieros, S., additional, Mosca, L., additional, Navick, X.-F., additional, Nollez, G., additional, Olivieri, E., additional, Pari, P., additional, Sanglard, V., additional, Schoeffel, L., additional, Schwamm, F., additional, and Stern, M., additional
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- 2007
- Full Text
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207. EURECA — the European future of cryogenic dark matter searches
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Kraus, H, primary, Bauer, M, additional, Benoit, A, additional, Blümer, J, additional, Broniatowski, A, additional, Camus, P, additional, Chantelauze, A, additional, Chapellier, M, additional, Chardin, G, additional, Christ, P, additional, Coppi, C, additional, Jésus, M De, additional, Lesquen, A De, additional, Deschamps, H, additional, Stefano, P Di, additional, Dumoulin, L, additional, Eitel, K, additional, Feilitzsch, F von, additional, Fesquet, M, additional, Gascon, J, additional, Gerbier, G, additional, Goldbach, C, additional, Gros, M, additional, Hauff, D, additional, Henry, S, additional, Horn, M, additional, Isaila, C, additional, Kimmerle, M, additional, Jochum, J, additional, Juillard, A, additional, Lemrani, R, additional, Luca, M, additional, Marnieros, S, additional, McGowan, R, additional, Mikhailik, V, additional, Navick, X-F, additional, Niinikoski, T, additional, Nollez, G, additional, Pantic, E, additional, Pari, P, additional, Petricca, F, additional, Potzel, W, additional, Pröbst, F, additional, Rau, W, additional, Ritter, F, additional, Rottler, K, additional, Scholl, S, additional, Seidel, W, additional, Sanglard, V, additional, Stern, M, additional, Schwamm, F, additional, Teshima, M, additional, Tolhurst, B, additional, Westphal, W, additional, Wikus, P, additional, and Wolf, J, additional
- Published
- 2006
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208. Background suppression in the Edelweiss-III experiment.
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Navick, X.-F. and EDELWEISS Collaboration
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WEAKLY interacting massive particles , *DARK matter , *BACKGROUND radiation , *RADIOACTIVITY , *NEUTRON flux , *NEUTRONS , *RADIATION shielding , *COSMIC rays - Abstract
In dark matter WIMP searches the neutron shielding plays a crucial role in attenuating neutron flux and hence, suppressing nuclear recoil event rate - one of the key background mimicking WIMP interactions. The transition from EDELWEISS-II to EDELWEISS-III with 40 detectors with increased mass and improved background rejection has required the modification of the neutron shielding. In this paper we describe the new neutron shielding design and give an estimate of the expected neutron rate in comparison with the previous stage of the experiment. [ABSTRACT FROM AUTHOR]
- Published
- 2013
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209. Sensitivity of the EDELWEISS WIMP search to spin-dependent interactions
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Benoit, A., primary, Bergé, L., additional, Blümer, J., additional, Broniatowski, A., additional, Censier, B., additional, Chabert, L., additional, Chapellier, M., additional, Chardin, G., additional, Collin, S., additional, De Jésus, M., additional, Deschamps, H., additional, Di Stefano, P., additional, Dolgorouky, Y., additional, Drain, D., additional, Dumoulin, L., additional, Eitel, K., additional, Fesquet, M., additional, Fiorucci, S., additional, Gascon, J., additional, Gerbier, G., additional, Goldbach, C., additional, Gros, M., additional, Gumbsheimer, R., additional, Horn, M., additional, Juillard, A., additional, de Lesquen, A., additional, Luca, M., additional, Mallet, J., additional, Marnieros, S., additional, Mosca, L., additional, Navick, X.-F., additional, Nollez, G., additional, Pari, P., additional, Razeti, M., additional, Sanglard, V., additional, Schoeffel, L., additional, Stern, M., additional, and Villar, V., additional
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- 2005
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210. Calibration of the EDELWEISS cryogenic heat-and-ionization germanium detectors for dark matter search
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Martineau, O., primary, Benoı̂t, A., additional, Bergé, L., additional, Broniatowski, A., additional, Chabert, L., additional, Chambon, B., additional, Chapellier, M., additional, Chardin, G., additional, Charvin, P., additional, De Jésus, M., additional, Di Stefano, P., additional, Drain, D., additional, Dumoulin, L., additional, Gascon, J., additional, Gerbier, G., additional, Gerlic, E., additional, Goldbach, C., additional, Goyot, M., additional, Gros, M., additional, Hadjout, J.P., additional, Hervé, S., additional, Juillard, A., additional, de Lesquen, A., additional, Loidl, M., additional, Mallet, J., additional, Marnieros, S., additional, Mirabolfathi, N., additional, Mosca, L., additional, Navick, X.-F., additional, Nollez, G., additional, Pari, P., additional, Riccio, C., additional, Sanglard, V., additional, Schoeffel, L., additional, Stern, M., additional, and Vagneron, L., additional
- Published
- 2004
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211. LATEST RESULTS OF THE EDELWEISS EXPERIMENT
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DRAIN, D., primary, BONNEVAUX, A., additional, CHABERT, L., additional, CHAMBON, B., additional, DE JESUS, M., additional, DI STEFANO, P., additional, GASCON, J., additional, GERLIC, E., additional, GOYOT, M., additional, HADJOUT, J. P., additional, MARTINEAU, O., additional, SANGLARD, V., additional, STERN, M., additional, VAGNERON, L., additional, BENOIT, A., additional, CAUSSIGNAC, M., additional, RODENAS, H., additional, BERGÉ, L., additional, BRONIATOWSKI, A., additional, COLLIN, S., additional, DUMOULIN, L., additional, JUILLARD, A., additional, MARNIEROS, S., additional, MIRABOLFATHI, N., additional, CHAPELLIER, M., additional, PARI, P., additional, CHARDIN, G., additional, DESCHAMPS, H., additional, GERBIER, G., additional, GROS, M., additional, HERVÉ, S., additional, DE LESQUEN, A., additional, LOIDL, M., additional, MALLET, J., additional, MOSCA, L., additional, NAVICK, X. F., additional, NIZERY, F., additional, SHOEFFEL, L., additional, CHARVIN, P., additional, RICCIO, C., additional, GOLDBACH, C., additional, MARTIN, M., additional, and NOLLEZ, G., additional
- Published
- 2003
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212. Dark Matter Searches with the Experiment EDELWEISS-II.
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Navick, X-F.
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DARK matter , *GERMANIUM diodes , *IONIZATION (Atomic physics) , *DETECTORS , *ELECTRODES - Abstract
The EDELWEISS II experiment is devoted to the search for the Weakly Interactive Massive Particles (WIMPs) that would constitute the Dark Matter halo of our Galaxy. For this purpose, the experiment uses cryogenic germanium detectors, cooled down to 20 mK, in which the collision of a WIMP with an atom produces characteristic signals in terms of ionization and elevation of temperature. We present the preliminary results of the first operation of the detectors installed in the underground laboratory of the Frejus Tunnel (LSM), attesting to the very low radioactive background conditions achieved so far. Novel detectors, with a special electrode design for active rejection of surface events, have been shown to be suited for searches of WIMPs with scattering cross-sections on nucleons well below 10-8 pb. Preliminary results of WIMP searches performed with a first set of these detectors will be shown as well. [ABSTRACT FROM AUTHOR]
- Published
- 2009
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213. The development of x-ray bolometers based on SOI technology for astronomy.
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Aliane, A., De Moro, F., Agnese, P., Pigot, C., Sauvageot, J.-L., Szeflinski, V., Gasse, A., Arnaud, M., de la Broïse, X., Navick, X.-F., Routin, J., Mathieu, L., Cigna, J.-C., Berger, F., Ribot, H., and Gobil, Y.
- Published
- 2008
- Full Text
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214. Surface events identification in the EDELWEISS germanium bolometers.
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Navick, X.-F.
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DETECTORS , *BOLOMETERS , *RADIOACTIVITY , *THIN films , *PHYSICS - Abstract
In the first phase of the EDELWEISS-II Dark Matter search, 23 germanium detectors with NTD thermal sensors and 7 detectors with NbSi thin films are going to be used at 20mK for the direct detection of WIMPs. In this paper, we are describing the different techniques of identification of surface events that might improve strongly the physics results of this experiment. © 2007 American Institute of Physics [ABSTRACT FROM AUTHOR]
- Published
- 2007
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215. Improved exclusion limits from the EDELWEISS WIMP search
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Benoit, A, primary, Bergé, L, additional, Broniatowski, A, additional, Chabert, L, additional, Chambon, B, additional, Chapellier, M, additional, Chardin, G, additional, Charvin, P, additional, De Jésus, M, additional, Di Stefano, P, additional, Drain, D, additional, Dumoulin, L, additional, Gascon, J, additional, Gerbier, G, additional, Gerlic, E, additional, Goldbach, C, additional, Goyot, M, additional, Gros, M, additional, Hadjout, J.P, additional, Hervé, S, additional, Juillard, A, additional, de Lesquen, A, additional, Loidl, M, additional, Mallet, J, additional, Marnieros, S, additional, Martineau, O, additional, Mirabolfathi, N, additional, Mosca, L, additional, Navick, X.-F, additional, Nollez, G, additional, Pari, P, additional, Riccio, C, additional, Sanglard, V, additional, Stern, M, additional, and Vagneron, L, additional
- Published
- 2002
- Full Text
- View/download PDF
216. First results of the EDELWEISS WIMP search using a 320 g heat-and-ionization Ge detector
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Benoit, A., primary, Bergé, L., additional, Broniatowski, A., additional, Chambon, B., additional, Chapellier, M., additional, Chardin, G., additional, Charvin, P., additional, De Jésus, M., additional, Di Stefano, P., additional, Drain, D., additional, Dumoulin, L., additional, Gascon, J., additional, Gerbier, G., additional, Goldbach, C., additional, Goyot, M., additional, Gros, M., additional, Hadjout, J.P., additional, Juillard, A., additional, de Lesquen, A., additional, Loidl, M., additional, Mallet, J., additional, Marnieros, S., additional, Martineau, O., additional, Mirabolfathi, N., additional, Mosca, L., additional, Miramonti, L., additional, Navick, X.-F., additional, Nollez, G., additional, Pari, P., additional, Stern, M., additional, and Vagneron, L., additional
- Published
- 2001
- Full Text
- View/download PDF
217. DARK MATTER SEARCH IN THE EDELWEISS EXPERIMENT
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Chapellier, M., primary, Benoit, A., additional, Bergé, L., additional, Broniatowski, A., additional, Chambon, B., additional, Chardin, G., additional, Charvin, P., additional, De Jésus, M., additional, Di Stefano, P., additional, Drain, D., additional, Dumoulin, L., additional, Gascon, J., additional, Gerbier, G., additional, Goldbach, C., additional, Goyot, M., additional, Gros, M., additional, Hadjout, J.P., additional, Hervé, S., additional, Juillard, A., additional, de Lesquen, A., additional, Loidl, M., additional, Mallet, J., additional, Marnieros, S., additional, Martineau, O., additional, Mirabolfathi, N., additional, Miramonti, L., additional, Mosca, L., additional, Navick, X.-F., additional, Nollez, G., additional, Pari, P., additional, Pastor, C., additional, Simon, E., additional, Stern, M., additional, and Vagneron, L., additional
- Published
- 2001
- Full Text
- View/download PDF
218. Background discrimination capabilities of a heat and ionization germanium cryogenic detector
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Di Stefano, P., primary, Bergé, L., additional, Chambon, B., additional, Chapellier, M., additional, Chaumont, J., additional, Chardin, G., additional, Charvin, P., additional, De Jésus, M., additional, Drain, D., additional, Dumoulin, L., additional, Forget, P., additional, Garoche, P., additional, Gascon, J., additional, Goldbach, C., additional, L'Hôte, D., additional, Mallet, J., additional, Mangin, J., additional, Marnieros, S., additional, Miramonti, L., additional, Mosca, L., additional, Navick, X-F., additional, Nollez, G., additional, Pari, P., additional, Pécourt, S., additional, Simon, E., additional, Stab, L., additional, Torre, J-P., additional, Tourbot, R., additional, and Yvon, D., additional
- Published
- 2001
- Full Text
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219. Dark matter search in the EDELWEISS experiment using a 320 g ionization-heat Ge-detector.
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Navick, X.-F., Benoit, A., Berge´, L., Broniatowski, A., Chambon, B., Chapellier, M., Chardin, G., Charvin, P., De Je´sus, M., Drain, D., Dumoulin, L., Gascon, J., Gerbier, G., Goldbach, C., Goyot, M., Gros, M., Hadjout, J-P., Herve´, S., Juillard, A., and de Lesquen, A.
- Subjects
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DETECTORS , *LOW temperature engineering - Abstract
The EDELWEISS collaboration has performed a direct search for WIMPs using a 320g ionization-heat Ge-cryogenic detector operated in a low-background environment in the Laboratoire Souterrain de Modane. No nuclear recoils events are observed in the fiducial volume in the 30-200 keV energy range during an effective exposure of 4.53 kg.days. A limit on the cross-section of the WIMP-proton spin-independent interaction as a function of the WIMP mass is deduced. The central value of the signal reported by the DAMA experiment is excluded at 90% CL. [ABSTRACT FROM AUTHOR]
- Published
- 2002
220. 320 g ionization-heat cryogenic detector for dark matter search in the EDEL WEISS experiment.
- Author
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Martineau, O., Chapellier, M., Chardin, G., De Je´sus, M., Gascon, J., Herve´, S., Juillard, A., Loidl, M., Navick, X-F., and Nollez, G.
- Subjects
DETECTORS ,LOW temperature engineering ,DARK matter - Abstract
The EDELWEISS experiment is presently using for direct WIMP detection a 320g heat-and-ionization cryogenic Ge detector operated in a low-background environment in the Laboratoire Souterrain de Modane (LSM). This detector presents an increase of more than 4 times the mass of previous detectors. Calibrations of this detector are used to determine its energy resolution and fiducial volume, and to optimize the detector design for the 1kg phase of the EDELWEISS-I experiment. Analysis of the calibrations and characteristics of a first series of 320g-detectors are presented. [ABSTRACT FROM AUTHOR]
- Published
- 2002
221. Erratum to: “Ionization measurement at very low temperature for nuclear and electron recoils discrimination by ionization-heat simultaneous measurement for dark matter research” [Nucl. Instr. and Meth. A 442 (2000) 267–274]
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Navick, X.-F, primary, L’Hôte, D, additional, and Tourbot, R, additional
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- 2000
- Full Text
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222. Event categories in the EDELWEISS WIMP search experiment
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Benoit, A., primary, Bergé, L., additional, Broniatowski, A., additional, Chambon, B., additional, Chapellier, M., additional, Chardin, G., additional, Charvin, P., additional, De Jésus, M., additional, Di Stefano, P., additional, Drain, D., additional, Dumoulin, L., additional, Garoche, P., additional, Gascon, J., additional, Goldbach, C., additional, Gros, M., additional, Juillard, A., additional, de Lesquen, A., additional, L'Hôte, D., additional, Mallet, J., additional, Mangin, J., additional, Marnieros, S., additional, Mirabolfathi, N., additional, Miramonti, L., additional, Mosca, L., additional, Navick, X-F., additional, Nollez, G., additional, Pari, P., additional, Pécourt, S., additional, Simon, E., additional, Stern, M., additional, and Torre, J-P., additional
- Published
- 2000
- Full Text
- View/download PDF
223. Charge and heat collection in a 70 g heat/ionization cryogenic detector for dark matter search
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L’Hôte, D., primary, Navick, X. F., additional, Tourbot, R., additional, Mangin, J., additional, and Pesty, F., additional
- Published
- 2000
- Full Text
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224. Status of the EDELWEISS experiment
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Bergé, L., primary, Berkes, I., additional, Chambon, B., additional, Chapellier, M., additional, Chardin, G., additional, Charvin, P., additional, De Jésus, M., additional, Di Stefano, P., additional, Drain, D., additional, Dumoulin, L., additional, Goldbach, C., additional, Juillard, A., additional, L'Hôte, D., additional, Marnieros, S., additional, Miramonti, L., additional, Mosca, L., additional, Navick, X.-F., additional, Nollez, G., additional, Pari, P., additional, Pastor, C., additional, Pecourt, S., additional, Tourbot, R., additional, and Yvon, D., additional
- Published
- 1999
- Full Text
- View/download PDF
225. Status of the EDELWEISS experiment
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Drain, D., primary, Benoit, A., additional, Bergé, L., additional, Berkes, I., additional, Chambon, B., additional, Chapellier, M., additional, Chardin, G., additional, Charvin, P., additional, Jésus, M.De, additional, Stefano, P.Di, additional, Dumoulin, L., additional, Goldbach, C., additional, Hadjout, J.-P., additional, Juilliard, A., additional, L’Hôte, D., additional, Mallet, J., additional, Marnieros, S., additional, Miramonti, L., additional, Mosca, L., additional, Navick, X.-F., additional, Nollez, G., additional, Pari, P., additional, Pastor, C., additional, Pécourt, S., additional, Simon, E., additional, Turbot, R., additional, Vagneron, L., additional, and Yvon, D., additional
- Published
- 1998
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226. First results of the EDELWEISS experiment
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de Bellefon, A., primary, Berger, L., additional, Berkés, I., additional, Bobin, C., additional, Broszkiewicz, D., additional, Chambon, B., additional, Chapellier, M., additional, Chardin, G., additional, Charvin, Ph., additional, Chazal, V., additional, Coron, N., additional, De Jesus, M., additional, Drain, D., additional, Dumoulin, L., additional, Giraud-Héraud, Y., additional, Goldbach, C., additional, Guerrier, G., additional, Hadjout, J.P., additional, Leblanc, J., additional, Marchand, D., additional, Messous, Y., additional, Navick, X.-F., additional, Nollez, G., additional, Pan, P., additional, Pastor, C., additional, Perillo-Isaac, M.C., additional, Prostakov, I., additional, and Yvon, D., additional
- Published
- 1996
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227. 320g ionization-heat bolometers design for the EDELWEISS experiment
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Navick, X. F., Chapellier, M., Deliot, F., Herve, S., and Miramonti, L.
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- 2000
- Full Text
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228. CUPID pre-CDR
- Author
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Armstrong, W. R., Chang, C., Hafidi, K., Lisovenko, M., Novosad, V., Pearson, J., Polakovic, T., Wang, G., Yefremenko, V., Zhang, J., Bucci, C., Canonica, L., Cappelli, L., Caracciolo, V., Copello, S., D Addabbo, A., Gorla, P., Nisi, S., Orlandi, D., Pagliarone, C. E., Pattavina, L., Pirro, S., Rusconi, C., Schaffner, K., Benato, G., Drobizhev, A., Fujikawa, B. K., Huang, R., Kolomensky, Yu G., Marini, L., Norman, E., Sakai, M., Schmidt, B., Singh, V., Vetter, K., Wagaarachchi, S., Wallig, J., Welliver, B., Oro, S., O Donnell, T., Zucchelli, S., Moggi, N., Boldrini, V., Mancarella, F., Rizzi, R., Johnston, J., Ouellet, J., Formaggio, J., Winslow, L., Avignone, F., Creswick, R., Wilson, K., Franceschi, A., Napolitano, T., Caminata, A., Di Domizio, S., Pallavicni, M., Velazquez, M., Peng, H., Xue, M., Danevich, F., Kobychev, V., Polischuk, O., Tretyak, V., Azzolini, O., Keppel, G., Pira, C., Ferroni, F., Dompè, V., Fantini, G., Alfonso, K., Huang, H. Z., Arnaud, Q., Augier, C., Billard, J., Cazes, A., Charlieux, F., Elkhoury, E., Gascon, J., Jesus, M., Juillard, A., Misiak, D., Sanglard, V., Vagneron, L., Beretta, M., Biassoni, M., Brofferio, C., Capelli, S., Carniti, P., Chiesa, D., Clemenza, M., Cremonesi, O., Faverzani, M., Ferri, E., Giachero, A., Gironi, L., Gotti, C., Nastasi, M., Nutini, I., Pagnanini, L., Pavan, M., Pessina, G., Pozzi, S., Previtali, E., Puiu, A., Sisti, M., Barabash, A., Konovalov, S., Yumatov, V., Heeger, K., Maruyama, R., Nikkel, J., Speller, D., Surukuchi, P. T., Shlegel, V., Bergé, L., Chapellier, M., Dumoulin, L., Giuliani, A., Khalife, H., Marcillac, P., Marnieros, S., Olivieri, E., Poda, D., Redon, T., Zolotarova, A., Brière, M., Bourgeois, C., Guerard, E., Loaiza, P., Taffarello, L., Karapetrov, G., Fabio Bellini, Cardani, L., Casali, N., Cruciani, A., Dafinei, I., Pettinacci, V., D Imperio, G., Tomei, C., Vignati, M., Colantoni, I., Armengaud, E., Charrier, A., Combarieu, M., Ferri, F., Gras, Ph, Gros, M., Helis, D., Navick, X. F., Nones, C., Pari, P., Paul, B., Gutierrez, T., Han, K., Ma, L., Shen, Y., He, W., and Martinez, M.
229. EURECA Conceptual Design Report
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Angloher, G., Armengaud, E., Augier, C., Benoit, A., Bergmann, T., Blümer, J., Broniatowski, A., Brudanin, V., Camus, P., Cazes, A., Chapellier, M., Coron, N., Cox, G.A., Cuesta, C., Danevich, F.A., Jésus, M.D., Dumoulin, L., Eitel, K., Erb, A., Ertl, A., Feilitzsch, F.V., Filosofov, D., Fourches, N., García, E., Gascon, J., Gerbier, G., Ginestra, C., Gironnet, J., Giuliani, A., Gros, M., Gütlein, A., Hauff, D., Henry, S., Heuermann, G., Jochum, J., Jokisch, S., Juillard, A., Kister, C., Kleifges, M., Kluck, H., Korolkova, E.V., Kozlov, V.Y., Kraus, H., Kudryavtsev, V.A., Lanfranchi, J.-C., Loaiza, P., Loebell, J., Machulin, I., Marnieros, S., Martínez, M., Menshikov, A., Münster, A., Navick, X.-F., Nones, C., Ortigoza, Y., Pari, P., Petricca, F., Potzel, W., Povinec, P.P., Pröbst, F., Puimedón, J., Reindl, F., Robinson, M., Rolón, T., Roth, S., Rottler, K., Rozov, S., Sailer, C., Salinas, A., Sanglard, V., Sarsa, M.L., Schäffner, K., Schmidt, B., Scholl, S., Schönert, S., Seidel, W., Siebenborn, B., Sivers, M.V., Strandhagen, C., Strauß, R., Tanzke, A., Tretyak, V.I., Turad, M., Ulrich, A., Usherov, I., Veber, P., Velazquez, M., Villar, J.A., Viraphong, O., Walker, R.J., Wawoczny, S., Weber, M., Willers, M., Wüstrich, M., Yakushev, E., Zhang, X., and Zöller, A.
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7. Clean energy
230. Conceptual Design of BabyIAXO, the intermediate stage towards the International Axion Observatory
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Abeln, A., Altenmüller, K., Arguedas Cuendis, S., Armengaud, E., Attié, D., Aune, S., Basso, S., Bergé, L., Biasuzzi, B., Borges De Sousa, P. T. C., Brun, P., Bykovskiy, N., Calvet, D., Carmona, J. M., Castel, J. F., Cebrián, S., Chernov, V., Christensen, F. E., Civitani, M. M., Cogollos, C., Dafní, T., Derbin, A., Desch, K., Díez, D., Dinter, M., Döbrich, B., Drachnev, I., Dudarev, A., Dumoulin, L., Ferreira, D. D. M., Ferrer-Ribas, E., Fleck, I., Galán, J., Gascón, D., Gastaldo, L., Giannotti, M., Giomataris, Y., Giuliani, A., Gninenko, S., Golm, J., Golubev, N., Hagge, L., Hahn, J., Hailey, C. J., Hengstler, D., Henriksen, P. L., Houdy, T., Iglesias-Marzoa, R., Iguaz-Gutierrez, F. J., Irastorza, I. G., Iñiguez, C., Jakovčić, K., Kaminski, J., Kanoute, B., Karstensen, S., Kravchuk, L., Lakić, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, Axel, Loidl, M., Lomskaya, I., López-Alegre, G., Lubsandorzhiev, B., Ludwig, Kai, Luzón, G., Malbrunot, C., Margalejo, C., Marin-Franch, A., Marnieros, S., Marutzky, F., Mauricio, J., Menesguen, Y., Mentink, M., Mertens, S., Mescia, F., Miralda-Escudé, J., Mirallas, H., Mols, J. P., Muratova, V., Navick, X. F., Nones, C., Notari, A., Nozik, A., Obis, L., Oriol, C., Orsini, F., Ortiz De Solórzano, A., Oster, S., Pais Da Silva, H. P., Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Pérez, O., Picatoste, E., Pivovaroff, M. J., Poda, D. V., Redondo, J., Ringwald, A., Rodrigues, M., Rueda-Teruel, F., Rueda-Teruel, S., Ruiz-Choliz, E., Ruz, J., Saemann, E. O., Salvado, J., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Segui, L., Tavecchio, F., Ten Kate, H. H. J., Tkachev, I., Troitsky, S., Unger, D., Unzhakov, E., Ushakov, N., Vogel, J. K., Voronin, D., Weltman, A., Werthenbach, U., Wuensch, W., and Yanes-Díaz, A.
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7. Clean energy - Abstract
This article describes BabyIAXO, an intermediate experimental stage of the International Axion Observatory (IAXO), proposed to be sited at DESY. IAXO is a large-scale axion helioscope that will look for axions and axion-like particles (ALPs), produced in the Sun, with unprecedented sensitivity. BabyIAXO is conceived to test all IAXO subsystems (magnet, optics and detectors) at a relevant scale for the final system and thus serve as prototype for IAXO, but at the same time as a fully-fledged helioscope with relevant physics reach itself, and with potential for discovery. The BabyIAXO magnet will feature two 10 m long, 70 cm diameter bores, and will host two detection lines (optics and detector) of dimensions similar to the final ones foreseen for IAXO. BabyIAXO will detect or reject solar axions or ALPs with axion-photon couplings down to $g_{a\gamma} \sim 1.5 \times 10^{-11}$ GeV$^{-1}$, and masses up to $m_a\sim 0.25$ eV. BabyIAXO will offer additional opportunities for axion research in view of IAXO, like the development of precision x-ray detectors to identify particular spectral features in the solar axion spectrum, and the implementation of radiofrequency-cavity-based axion dark matter setups.
231. Background optimization for a new spherical gas detector for very light WIMP detection
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Dastgheibi-Fard, A., Giomataris, I., Gerbier, G., Derré, J., Gros, M., Magnier, P., Jourde, D., Bougamont, E., Navick, X. -F, Papaevangelou, T., Galan, J., Tsiledakis, G., Piquemal, F., Zampaolo, M., Pia Loaiza, and Savvidis, I.
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Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) - Abstract
The Spherical gaseous detector (or Spherical Proportional Counter, SPC) is a novel type of par- ticle detector, with a broad range of applications. Its main features include a very low energy threshold independent of the volume (due to its very low capacitance), a good energy resolution, robustness and a single detection readout channel, in its simplest version. Applications range from radon emanation gas monitoring, neutron flux and gamma counting and spectroscopy to dark matter searches, in particular low mass WIMPs and coherent neutrino scattering measure- ment. Laboratories interested in these various applications share expertise within the NEWS (New Experiments With Sphere) network. SEDINE, a low background prototype installed at underground site of Laboratoire Souterrain de Modane is currently being operated and aims at measuring events at very low energy threshold, around 100 eV. We will present the energy cali- bration with 37Ar, the surface background reduction, the measurement of detector background at sub-keV energies, and show anticipated sensitivities for light dark matter search., 5 pages, 3 figures
232. Precise measurement of $2\nu \beta \beta $ decay of $^{100}$Mo with the CUPID-Mo detection technology
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Armengaud, E., Augier, C., Barabash, A. S., Bellini, F., Benato, G., Benoît, A., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu. A., Bourgeois, Ch., Briere, M., Brudanin, V., Camus, P., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Charlieux, F., De Combarieu, M., Dafinei, I., Danevich, F. A., De Jesus, M., Dumoulin, L., Eitel, K., Elkhoury, E., Ferri, F., Fujikawa, B. K., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Guerard, E., Helis, D. L., Huang, H. Z., Huang, R., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S. I., Leder, A., Kotila, J., Loaiza, P., Ma, L., Makarov, E. P., De Marcillac, P., Marini, L., Marnieros, S., Misiak, D., Navick, X.-F., Nones, C., Novati, V., Olivieri, E., Ouellet, J. L., Pagnanini, L., Pari, P., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D. V., Polischuk, O. G., Previtali, E., Redon, Th., Rozov, S., Rusconi, C., Sanglard, V., Schäffner, K., Schmidt, B., Shen, Y., Shlegel, V. N., Siebenborn, B., Singh, V., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Velázquez, M., Weber, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., and Zolotarova, A. S.
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3. Good health - Abstract
We report the measurement of the two-neutrino double-beta (2νββ) decay of $^{100}$Mo to the ground state of $^{100}$Ru using lithium molybdate (Li$_{2}$$^{100}$MoO$_{4}$) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory (France). From a total exposure of 42.235 kg×day, the half-life of $^{100}$Mo is determined to be T2ν¦(1/2)=[7.12(+0.18)¦(-0.14) (stat.)±0.10(syst.)]×10$^{18}$ years. This is the most accurate determination of the 2νββ half-life of $^{100}$Mo to date.
233. Measurement of the cosmogenic activation of germanium detectors in EDELWEISS-III
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Armengauda, E., Arnaud, Q., Augier, C., Benoît, A., Bergé, L., Billard, J., Blümer, J., De Boissière, T., Broniatowski, A., Camus, P., Cazes, A., Chapellier, M., Charlieux, F., De Jésus, M., Dumoulin, L., Eitel, K., Foerster, N., Gascon, J., Giuliani, A., Gros, M., Hehn, L., Heuermann, G., Jin, Y., Juillard, A., Kéfélian, C., Kleifges, M., Kozlov, V., Kraus, H., Kudryavtsev, V.A., Le-Sueur, H., S. Marnieros, S., Navick, X.-F., Nones, C., Olivieri, E., Pari, P., Paul, B., Piro, M.-C., Poda, D., Queguiner, E., Rozov, S., Sanglard, V., Schmidt, B., Scorza, S., Siebenborn, B., Tcherniakhovski, D., Vagneron, L., Weber, M., and Yakushev, E.
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13. Climate action ,7. Clean energy
234. Axion search with BabyIAXO in view of IAXO
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Abeln, A., Altenmüller, K., Cuendis, S. Arguedas, Armengaud, E., Attié, D., Aune, S., Basso, S., Bergé, L., Biasuzzi, B., De Sousa, P. T. C. Borges, Brun, P., Bykovskiy, N., Calvet, D., Carmona, J. M., Castel, J. F., Cebrián, S., Chernov, V., Christensen, F. E., Civitani, M. M., Cogollos, C., Dafni, T., Derbin, A., Deschu, K., Díez, D., Dinter, M., Döbrich, B., Drachnev, I., Dudarev, A., Dumoulin, L., Ferreira, D. D. M., Ferrer-Ribas, E., Fleck, I., Galan, Javier, Gascón, D., Gastaldo, L., Giannotti, M., Giomataris, Y., Giuliani, A., Gninenko, S., Golm, J., Golubev, N., Hagge, L., Hahn, J., Hailey, J., Hengstler, D., Henriksen, P. L., Iglesias-Marzoa, R., Iguaz-Gutierrez, F. J., Irastorza, I. G., Iñiguez, C., Jakovcic, K., Kaminski, J., Kanoute, B., Karstensen, S., Kravchuk, L., Lakic, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, A., Loidl, M., Lomskaya, I., López-Alegre, G., Lubsandorzhiev, B., Ludwig, K., Luzón, G., Malbrunot, C., Margalejo, C., Marin-Franch, A., Marnieros, S., Marutzky, F., Mauricio, J., Menesguen, Y., Mentink, M., Mescia, F., Miralda-Escudé, J., Mirallas, H., Mols, J. P., Muratova, V., Navick, X. F., Nones, C., Notari, A., Nozik, A., Obis, L., Oriol, C., Orsini, F., Ortiz De Solórzano, A., Oster, S., Pais Da Silva, H. P., Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Pérez, O., Picatoste, E., Pivovaroff, M. J., Poda, D. V., Redondo, J., Ringwald, A., Rodrigues, M., Rueda-Teruel, F., Rueda-Teruel, S., Ruiz-Choliz, E., Ruz, J., Saemann, E. O., Salvado, J., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Segui, L., Tavecchio, F., Ten Kate, H. H. J., Tkachev, I., Troitsky, S., Unger, D., Unzhakov, E., Ushakov, N., Vogel, J. K., Voronin, D., Weltman, A., Werthenbach, U., Wuensch, W., and Yanes-Díaz, A.
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experimental methods ,axion: solar ,IAXO ,7. Clean energy ,activity report ,detector: design - Abstract
Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for Dark Matter, and in addition, they would be copiously produced at the sun's core. A relevant effort during the last decade has been the CAST experiment at CERN, the most sensitive axion helioscope to-date. The International Axion Observatory (IAXO) is a large-scale 4th generation helioscope. As its primary physics goal, IAXO will look for solar axions or ALPs with a signal to background ratio of about 5 orders of magnitude higher than CAST. Recently the IAXO collaboration has proposed and intermediate experimental stage, BabyIAXO, conceived to test all IAXO subsystems (magnet, optics, detectors and sun-tracking systems) at a relevant scale for the final system and thus serve as pathfinder for IAXO but at the same time as a fully-fledged helioscope with record and relevant physics reach in itself with potential for discovery. BabyIAXO was endorsed by the Physics Review committee of DESY last May 2019. Here we will review the status and prospects of BabyIAXO and its potential to probe the most physics motivated regions of the axion & ALPs parameter space.
235. Physics potential of the International Axion Observatory (IAXO)
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Armengaud, E., Attie, D., Basso, S., Brun, P., Bykovskiy, N., Carmona, J. M., Castel, J. F., Cebrián, S., Cicoli, M., Civitani, M., Cogollos, C., Conlon, J. P., Costa, D., Dafni, T., Daido, R., Derbin, A. V., Descalle, M. A., Desch, K., Dratchnev, I. S., Döbrich, B., Dudarev, A., Ferrer-Ribas, E., Fleck, I., Galán, J., Galanti, G., Garrido, L., Gascon, D., Gastaldo, L., Germani, C., Ghisellini, G., Giannotti, M., Giomataris, I., Gninenko, S., Golubev, N., Graciani, R., Irastorza, I. G., Jakovčí C, K., Kaminski, J., Krčmar, M., Krieger, C., Lakić, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, A., Lomskaya, I., Lubsandorzhiev, B., Luzón, G., Marsh, M. C. D., Mergalejo, C., Mescia, F., Meyer, M., Miralda-Escudé, J., Mirallas, H., Muratova, V. N., Navick, X. F., Nones, C., Notari, A., Nozik, A., Ortiz De Solórzano, A., Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Picatoste, E., Pivovaroff, M. J., Redondo, J., Ringwald, A., Roncadelli, M., Ruiz-Chóliz, E., Ruz, J., Saikawa, K., Salvadó, J., Samperiz, M. P., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Silva, H., Tagliaferri, G., Takahashi, F., Tavecchio, F., Ten Kate, H., Tkachev, I., Troitsky, S., Unzhakov, E., Vedrine, P., Vogel, J. K., Weinsheimer, C., Weltman, A., and Yin., W.
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transparency ,electron ,cosmological model ,photon ,quantum chromodynamics: axion ,sensitivity ,7. Clean energy ,inflation: model ,dark matter ,observatory ,X-ray ,13. Climate action ,gamma ray ,galaxy: cluster ,axion-like particles ,axion: mass ,string model ,axion: solar ,strong interaction: CP - Abstract
We review the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO). Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as $g_{a\gamma}\sim 10^{-12}$ GeV$^{-1}$, or to electrons $g_{ae}\sim$10$^{-13}$, IAXO has the potential to find the QCD axion in the 1 meV$\sim$1 eV mass range where it solves the strong CP problem, can account for the cold dark matter of the Universe and be responsible for the anomalous cooling observed in a number of stellar systems. At the same time, IAXO will have enough sensitivity to detect lower mass axions invoked to explain: 1) the origin of the anomalous 'transparency' of the Universe to gamma-rays, 2) the observed soft X-ray excess from galaxy clusters or 3) some inflationary models. In addition, we review string theory axions with parameters accessible by IAXO and discuss their potential role in cosmology as Dark Matter and Dark Radiation as well as their connections to the above mentioned conundrums.
236. Physics potential of the International Axion Observatory (IAXO)
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Armengaud, E., Attie, D., Basso, S., Brun, P., Bykovskiy, N., Carmona, J. M., Castel, J. F., Cebrián, S., Cicoli, M., Civitani, M., Cogollos, C., Conlon, J. P., Costa, D., Dafni, T., Daido, R., Derbin, A. V., Descalle, M. A., Desch, K., Dratchnev, I. S., Döbrich, B., Dudarev, A., Ferrer-Ribas, E., Fleck, I., Galán, J., Galanti, G., Garrido, L., Gascon, D., Gastaldo, L., Germani, C., Ghisellini, G., Giannotti, M., Giomataris, I., Gninenko, S., Golubev, N., Graciani, R., Irastorza, I. G., Jakovčí C, K., Kaminski, J., Krčmar, M., Krieger, C., Lakić, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, Axel, Lomskaya, I., Lubsandorzhiev, B., Luzón, G., Marsh, M. C. D., Mergalejo, C., Mescia, F., Meyer, M., Miralda-Escudé, J., Mirallas, H., Muratova, V. N., Navick, X. F., Nones, C., Notari, A., Nozik, A., Ortiz De Solórzano, A., Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., Picatoste, E., Pivovaroff, M. J., Redondo, J., Ringwald, A., Roncadelli, M., Ruiz-Chóliz, E., Ruz, J., Saikawa, K., Salvadó, J., Samperiz, M. P., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Silva, H., Tagliaferri, G., Takahashi, F., Tavecchio, F., Ten Kate, H., Tkachev, I., Troitsky, S., Unzhakov, E., Vedrine, P., Vogel, J. K., Weinsheimer, C., Weltman, A., and Yin., W.
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13. Climate action ,7. Clean energy - Abstract
Journal of cosmology and astroparticle physics 1906(06), 047 (2019). doi:10.1088/1475-7516/2019/06/047, We review the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO). Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as $g_{a\gamma}\sim 10^{-12}$ GeV$^{-1}$, or to electrons $g_{ae}\sim$10$^{-13}$, IAXO has the potential to find the QCD axion in the 1 meV$\sim$1 eV mass range where it solves the strong CP problem, can account for the cold dark matter of the Universe and be responsible for the anomalous cooling observed in a number of stellar systems. At the same time, IAXO will have enough sensitivity to detect lower mass axions invoked to explain: 1) the origin of the anomalous 'transparency' of the Universe to gamma-rays, 2) the observed soft X-ray excess from galaxy clusters or 3) some inflationary models. In addition, we review string theory axions with parameters accessible by IAXO and discuss their potential role in cosmology as Dark Matter and Dark Radiation as well as their connections to the above mentioned conundrums., Published by IOP, London
237. Conceptual design of BabyIAXO, the intermediate stage towards the International Axion Observatory
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Abeln, A., Altenm��ller, K., Arguedas Cuendis, S., Armengaud, E., Atti��, D., Aune, S., Basso, S., Berg��, L., Biasuzzi, B., Borges De Sousa, P. T. C., Brun, P., Bykovskiy, N., Calvet, D., Carmona, J. M., Castel, J. F., Cebri��n, S., Chernov, V., Christensen, F. E., Civitani, M. M., Cogollos, C., Dafn��, T., Derbin, A., Desch, K., D��ez, D., Dinter, M., D��brich, B., Drachnev, I., Dudarev, A., Dumoulin, L., Ferreira, D. D. M., Ferrer-Ribas, E., Fleck, I., Gal��n, J., Gasc��n, D., Gastaldo, L., Giannotti, M., Giomataris, Y., Giuliani, A., Gninenko, S., Golm, J., Golubev, N., Hagge, L., Hahn, J., Hailey, C. J., Hengstler, D., Henriksen, P. L., Houdy, T., Iglesias-Marzoa, R., Iguaz, F. J., Irastorza, I. G., I��iguez, C., Jakov��i��, K., Kaminski, J., Kanoute, B., Karstensen, S., Kravchuk, L., Laki��, B., Lasserre, T., Laurent, P., Limousin, O., Lindner, A., Loidl, M., Lomskaya, I., L��pez-Alegre, G., Lubsandorzhiev, B., Ludwig, K., Luz��n, G., Malbrunot, C., Margalejo, C., Marin-Franch, A., Marnieros, S., Marutzky, F., Mauricio, J., Menesguen, Y., Mentink, M., Mertens, S., Mescia, F., Miralda-Escud��, J., Mirallas, H., Mols, J. P., Muratova, V., Navick, X. F., Nones, C., Notari, A., Nozik, A., Obis, L., Oriol, C., Orsini, F., Ortiz de Sol��rzano, A., Oster, S., Pais Da Silva, H. P., Pantuev, V., Papaevangelou, T., Pareschi, G., Perez, K., P��rez, O., Picatoste, E., Pivovaroff, M. J., Poda, D. V., Redondo, J., Ringwald, A., Rodrigues, M., Rueda-Teruel, F., Rueda-Teruel, S., Ruiz-Choliz, E., Ruz, J., Saemann, E. O., Salvado, J., Schiffer, T., Schmidt, S., Schneekloth, U., Schott, M., Segui, L., Tavecchio, F., ten Kate, H. H. J., Tkachev, I., Troitsky, S., Unger, D., Unzhakov, E., Ushakov, N., Vogel, J. K., Voronin, D., Weltman, A., Werthenbach, U., Wuensch, W., and Yanes-D��az, A.
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axion: dark matter ,CP violation ,Beyond Standard Model ,Dark matter ,axion-like particles ,Other experiments ,axion: solar ,IAXO ,sensitivity ,7. Clean energy ,optics ,detector: design - Abstract
Journal of high energy physics 05(5), 137 (2021). doi:10.1007/JHEP05(2021)137, This article describes BabyIAXO, an intermediate experimental stage of the International Axion Observatory (IAXO), proposed to be sited at DESY. IAXO is a large-scale axion helioscope that will look for axions and axion-like particles (ALPs), produced in the Sun, with unprecedented sensitivity. BabyIAXO is conceived to test all IAXO subsystems (magnet, optics and detectors) at a relevant scale for the final system and thus serve as prototype for IAXO, but at the same time as a fully-fledged helioscope with relevant physics reach itself, and with potential for discovery. The BabyIAXO magnet will feature two 10 m long, 70 cm diameter bores, and will host two detection lines (optics and detector) of dimensions similar to the final ones foreseen for IAXO. BabyIAXO will detect or reject solar axions or ALPs with axion-photon couplings down to g$_{a��}$ ��� 1.5 �� 10$^{���11}$ GeV$^{���1}$, and masses up to m$_{a}$ ��� 0.25 eV. BabyIAXO will offer additional opportunities for axion research in view of IAXO, like the development of precision x-ray detectors to identify particular spectral features in the solar axion spectrum, and the implementation of radiofrequency-cavity-based axion dark matter setups.[graphic not available: see fulltext], Published by SISSA, [Trieste]
238. The CUPID-Mo experiment for neutrinoless double-beta decay: performance and prospects
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Armengaud, E., Augier, C., Barabash, A. S., Bellini, F., Benato, G., Benoît, A., Beretta, M., Bergé, L., Billard, J., Borovlev, Yu. A., Bourgeois, Ch., Briere, M., Brudanin, V. B., Camus, P., Cardani, L., Casali, N., Cazes, A., Chapellier, M., Charlieux, F., De Combarieu, M., Dafinei, I., Danevich, F. A., De Jesus, M., Dumoulin, L., Eitel, K., Elkhoury, E., Ferri, F., Fujikawa, B. K., Gascon, J., Gironi, L., Giuliani, A., Grigorieva, V. D., Gros, M., Guerard, E., Helis, D. L., Huang, H. Z., Huang, R., Johnston, J., Juillard, A., Khalife, H., Kleifges, M., Kobychev, V. V., Kolomensky, Yu. G., Konovalov, S. I., Leder, A., Loaiza, P., Ma, L., Makarov, E. P., De Marcillac, P., Marini, L., Marnieros, S., Misiak, D., Navick, X. -F., Nones, C., Novati, V., Olivieri, E., Ouellet, J. L., Pagnanini, L., Pari, P., Pattavina, L., Paul, B., Pavan, M., Peng, H., Pessina, G., Pirro, S., Poda, D. V., Polischuk, O. G., Previtali, E., Redon, Th., Rozov, S., Rusconi, C., Sanglard, V., Schäffner, K., Schmidt, B., Shen, Y., Shlegel, V. N., Siebenborn, B., Singh, V., Sorbino, S., Tomei, C., Tretyak, V. I., Umatov, V. I., Vagneron, L., Velázquez, M., Weber, M., Welliver, B., Winslow, L., Xue, M., Yakushev, E., and Zolotarova, A. S.
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7. Clean energy
239. Instrument On-chip: All-Silicon Polarimetric Detectors in the Submillimeter Domain.
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Rodriguez, L., Gevin, O., Poglitsch, A., Dussopt, L., Revéret, V., Navick, X.-F., Aliane, A., de la Broise, X., Goudon, V., Vandeneynde, A., Delisle, C., Lasfargues, G., Tollet, T., Kaya, H., and Demonti, A.
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SUBMILLIMETER astronomy , *DETECTORS , *LIGHT absorption , *SILICON detectors , *BOLOMETERS , *POLARIMETRY - Abstract
Characterization of the magnetic fields at different scales in the Universe is a new frontier for submillimeter astronomy. Polarimetric measurements between 50 and 500 µm are the golden path for this research. We develop, in the prospect of space observatories, all-silicon 50 mK bolometer arrays with polarimetric capabilities in the pixel. Here, we present the first results of the new detectors: performances of thermal sensors, optical absorption and polarimetry. [ABSTRACT FROM AUTHOR]
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- 2024
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240. Systematic study of massive germanium pin diode detectors at 20 mK
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L'Hote, D., Navick, X. F., Barbier, A., Stab, L., Chapellier, M., Chaumont, J., Chardin, G., Ponpon, J. P., Prostakov, I., and Yvon, D.
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- 1996
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241. A sparkless resistive glass correction electrode for the spherical proportional counter.
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Katsioulas, I., Giomataris, I., Knights, P., Gros, M., Navick, X. F., Nikolopoulos, K., and Savvidis, I.
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- 2018
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242. Perspectives of a single-anode cylindrical chamber operating in ionization mode and high gas pressure.
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Bouet, R., Busto, J., Cecchini, V., Charpentier, P., Chapellier, M., Dastgheibi-Fard, A., Druillole, F., Jollet, C., Hellmuth, P., Gros, M., Lautridou, P., Meregaglia, A., Navick, X. F., Piquemal, F., Roche, M., and Thomas, B.
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As part of the R2D2 (Rare Decays with Radial Detector) R &D, the use of a gas detector with a spherical or cylindrical cathode, equipped with a single anode and operating at high pressure, was studied for the search of rare phenomena such as neutrinoless double-beta decay. The presented measurements were obtained with a cylindrical detector, covering gas pressures ranging from 1 to 10 bar in argon and 1 to 6 bar in xenon, using both a point-like source of 210 Po (5.3 MeV α ) and a diffuse source of 222 Rn (5.5 MeV α ). Analysis and interpretation of the data were developed using the anodic current waveform. Similar detection performances were achieved with both gases, and comparable energy resolutions were measured with both sources. As long as the purity of the gas was sufficient, no significant degradation of the measured energy was observed by increasing the pressure. At the highest operating pressure, an energy resolution better than 1.5% full-width at half-maximum (FWHM) was obtained for both gaseous media, although optimal noise conditions were not reached. [ABSTRACT FROM AUTHOR]
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- 2024
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243. A multiball read-out for the spherical proportional counter.
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Giganon, A., Giomataris, I., Gros, M., Katsioulas, I., Navick, X. F., Tsiledakis, G., Savvidis, I., Dastgheibi-Fard, A., and Brossard, A.
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- 2017
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244. Physical interpretation of the Neganov-Luke and related effects
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Chapellier, M. P., Chardin, G., Miramonti, L., and Navick, X. F.
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- 2000
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245. A solid ionization chamber operated at 20 mK
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Navick, X. F., L'Hote, D., Barbier, A., Stab, L., Chapellier, M., Chaumont, J., Chardin, G., Ponpon, J. P., Prostakov, I., and Yvon, D.
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- 1996
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246. A CUPID Li$_2$ $^{100} $MoO$_4$ scintillating bolometer tested in the CROSS underground facility
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A. S. Barabash, V. Yumatov, G. D'Imperio, M. De Deo, Ezio Previtali, J. M. Calvo-Mozota, Evelyn Ferri, B. Welliver, L. Gironi, L. Marini, E. Guerard, D. Misiak, D. V. Poda, J. Johnston, V. Dompè, F. T. Avignone, Whitney Armstrong, A. Charrier, O. Tellier, I. Colantoni, A. D'Addabbo, S. Di Domizio, P. Pari, Tomas Polakovic, Massimiliano Clemenza, V. Shlegel, R. Mariam, Yu. G. Kolomensky, Luigi Cappelli, Monica Sisti, M. Pavan, S. Zucchelli, Laura Cardani, P. de Marcillac, C. Augier, Goran Karapetrov, X.-F. Navick, B. K. Fujikawa, Stefano Pozzi, L. Pagnanini, P. T. Surukuchi, O. Azzolini, G. Fantini, Federico Ferri, B. Schmidt, C. Oriol, C. Pagliarone, E. Celi, T. O'Donnell, S. H. Fu, S. Dell'Oro, Giovanni Benato, M. Xue, Yuting Liu, Ch. Bourgeois, C. C. Chang, Stefano Nisi, James R. Wilson, S. Milana, G. Olivier, A. Cruciani, A. Franceschi, Changbo Fu, I. Dafinei, M. Chapellier, C. Gotti, S. Copello, C. Brofferio, S. Pirro, Jie Yang, V. Sharma, D. L. Helis, A. Barresi, J. Camilleri, R. Rizzoli, L. Ma, L. Dumoulin, Davide Chiesa, A. S. Zolotarova, Paolo Carniti, V. Pettinacci, A. Juillard, A. Candela, M. Gros, M. Madhukuttan, I. C. Bandac, M. De Jesus, E. V. Hansen, O. G. Polischuk, A. Drobizhev, Ke Han, F. Bellini, A. Ressa, Reina H. Maruyama, V.I. Tretyak, F.A. Danevich, J. A. Scarpaci, C. Bucci, T. D. Gutierrez, M. Faverzani, Matias Velázquez, P. Loaiza, Kai Vetter, Massimiliano Nastasi, S. I. Konovalov, L. Taffarello, D. Reynet, V. V. Kobychev, L. Bergé, J. Gascon, V. Sanglard, L. Yan, L. Imbert, Virendra Singh, M. M. Zarytskyy, Valentyn Novosad, C. Rosenfeld, Danielle Speller, Andrea Giachero, N. Casali, A. Branca, L. Pattavina, A. Ianni, E. Olivieri, R. J. Creswick, Eric B. Norman, V. Boldrini, P. Gras, K. Wilson, S. Pagan, J. Billard, S. Marnieros, Li Wang, T. Napolitano, R. Nipoti, A. Cazes, P. Gorla, F. Ferroni, E. Figueroa-Feliciano, C. Tomei, C. Pira, Haiping Peng, Oliviero Cremonesi, M. Biassoni, D. Mayer, Jonathan Ouellet, G. Bari, Lindley Winslow, M. de Combarieu, Joseph A. Formaggio, A. Tsymbaliuk, Y. Mei, A. Armatol, K. M. Heeger, R. G. Huang, F. Mancarella, B. Paul, M. I. Martínez, G. Pessina, Jie Zhang, C. Nones, A. Puiu, A. Giuliani, B. Mauri, James Nikkel, Irene Nutini, G. Wang, H. Z. Huang, V. G. Yefremenko, G. Keppel, H. Khalife, E. Armengaud, D. Baudin, M. Beretta, S. L. Wagaarachchi, F. Collamati, Simone Capelli, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Institut Rayonnement Matière de Saclay (IRAMIS), Science et Ingénierie des Matériaux et Procédés (SIMaP), Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), CUPID, CROSS, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Armatol A., Armengaud E., Armstrong W., Augier C., Iii F.T.A., Azzolini O., Bandac I.C., Barabash A.S., Bari G., Barresi A., Baudin D., Bellini F., Benato G., Beretta M., Berge L., Bourgeois C., Biassoni M., Billard J., Boldrini V., Branca A., Brofferio C., Bucci C., Calvo-Mozota J.M., Camilleri J., Candela A., Capelli S., Cappelli L., Cardani L., Carniti P., Casali N., Cazes A., Celi E., Chang C., Chapellier M., Charrier A., Chiesa D., Clemenza M., Colantoni I., Collamati F., Copello S., Cremonesi O., Creswick R.J., Cruciani A., D'Addabbo A., D'Imperio G., Dafinei I., Danevich F.A., De Combarieu M., Deo M.D., Jesus M.D., De Marcillac P., Dell'Oro S., Domizio S.D., Dompe V., Drobizhev A., Dumoulin L., Fantini G., Faverzani M., Ferri E., Ferri F., Ferroni F., Figueroa-Feliciano E., Formaggio J., Franceschi A., Fu C., Fu S., Fujikawa B.K., Gascon J., Giachero A., Gironi L., Giuliani A., Gorla P., Gotti C., Gras P., Gros M., Guerard E., Gutierrez T.D., Han K., Hansen E.V., Heeger K.M., Helis D.L., Huang H.Z., Huang R.G., Ianni A., Imbert L., Johnston J., Juillard A., Karapetrov G., Keppel G., Khalife H., Kobychev V.V., Kolomensky Y.G., Konovalov S.I., Liu Y., Loaiza P., Ma L., Madhukuttan M., Mancarella F., Mariam R., Marini L., Marnieros S., Martinez M., Maruyama R.H., Mauri B., Mayer D., Mei Y., Milana S., Misiak D., Napolitano T., Nastasi M., Navick X.-F., Nikkel J., Nipoti R., Nisi S., Nones C., Norman E.B., Novosad V., Nutini I., O'Donnell T., Olivier G., Olivieri E., Oriol C., Ouellet J.L., Pagan S., Pagliarone C., Pagnanini L., Pari P., Pattavina L., Paul B., Pavan M., Peng H., Pessina G., Pettinacci V., Pira C., Pirro S., Poda D.V., Polakovic T., Polischuk O.G., Pozzi S., Previtali E., Puiu A., Ressa A., Reynet D., Rizzoli R., Rosenfeld C., Sanglard V., Scarpaci J.A., Schmidt B., Sharma V., Shlegel V.N., Singh V., Sisti M., Speller D., Surukuchi P.T., Taffarello L., Tellier O., Tomei C., Tretyak V.I., Tsymbaliuk A., Velazquez M., Vetter K.J., Wagaarachchi S.L., Wang G., Wang L., Welliver B., Wilson J., Wilson K., Winslow L.A., Xue M., Yan L., Yang J., Yefremenko V., Yumatov V.I., Zarytskyy M.M., Zhang J., Zolotarova A.S., Zucchelli S., Armatol, A, Armengaud, E, Armstrong, W, Augier, C, Avignone F. T., I, Azzolini, O, Bandac, I, Barabash, A, Bari, G, Barresi, A, Baudin, D, Bellini, F, Benato, G, Beretta, M, Berge, L, Bourgeois, C, Biassoni, M, Billard, J, Boldrini, V, Branca, A, Brofferio, C, Bucci, C, Calvo-Mozota, J, Camilleri, J, Candela, A, Capelli, S, Cappelli, L, Cardani, L, Carniti, P, Casali, N, Cazes, A, Celi, E, Chang, C, Chapellier, M, Charrier, A, Chiesa, D, Clemenza, M, Colantoni, I, Collamati, F, Copello, S, Cremonesi, O, Creswick, R, Cruciani, A, D'Addabbo, A, D'Imperio, G, Dafinei, I, Danevich, F, De Combarieu, M, Deo, M, Jesus, M, De Marcillac, P, Dell'Oro, S, Domizio, S, Dompe, V, Drobizhev, A, Dumoulin, L, Fantini, G, Faverzani, M, Ferri, E, Ferri, F, Ferroni, F, Figueroa-Feliciano, E, Formaggio, J, Franceschi, A, Fu, C, Fu, S, Fujikawa, B, Gascon, J, Giachero, A, Gironi, L, Giuliani, A, Gorla, P, Gotti, C, Gras, P, Gros, M, Guerard, E, Gutierrez, T, Han, K, Hansen, E, Heeger, K, Helis, D, Huang, H, Huang, R, Ianni, A, Imbert, L, Johnston, J, Juillard, A, Karapetrov, G, Keppel, G, Khalife, H, Kobychev, V, Kolomensky, Y, Konovalov, S, Liu, Y, Loaiza, P, Ma, L, Madhukuttan, M, Mancarella, F, Mariam, R, Marini, L, Marnieros, S, Martinez, M, Maruyama, R, Mauri, B, Mayer, D, Mei, Y, Milana, S, Misiak, D, Napolitano, T, Nastasi, M, Navick, X, Nikkel, J, Nipoti, R, Nisi, S, Nones, C, Norman, E, Novosad, V, Nutini, I, O'Donnell, T, Olivier, G, Olivieri, E, Oriol, C, Ouellet, J, Pagan, S, Pagliarone, C, Pagnanini, L, Pari, P, Pattavina, L, Paul, B, Pavan, M, Peng, H, Pessina, G, Pettinacci, V, Pira, C, Pirro, S, Poda, D, Polakovic, T, Polischuk, O, Pozzi, S, Previtali, E, Puiu, A, Ressa, A, Reynet, D, Rizzoli, R, Rosenfeld, C, Sanglard, V, Scarpaci, J, Schmidt, B, Sharma, V, Shlegel, V, Singh, V, Sisti, M, Speller, D, Surukuchi, P, Taffarello, L, Tellier, O, Tomei, C, Tretyak, V, Tsymbaliuk, A, Velazquez, M, Vetter, K, Wagaarachchi, S, Wang, G, Wang, L, Welliver, B, Wilson, J, Wilson, K, Winslow, L, Xue, M, Yan, L, Yang, J, Yefremenko, V, Yumatov, V, Zarytskyy, M, Zhang, J, Zolotarova, A, and Zucchelli, S
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gas and liquid scintillators) ,Physics - Instrumentation and Detectors ,Accurate estimation ,Physics::Instrumentation and Detectors ,Bolometer ,Analytical chemistry ,Double-beta decay ,FOS: Physical sciences ,Cryogenic detector ,Radiopurity ,01 natural sciences ,030218 nuclear medicine & medical imaging ,law.invention ,Particle identification ,Particle identification methods ,03 medical and health sciences ,Particle identification method ,0302 clinical medicine ,CUORE ,law ,0103 physical sciences ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Detector array ,Instrumentation ,Mathematical Physics ,Event triggered ,Physics ,Lithium molybdate ,010308 nuclear & particles physics ,Astrophysics::Instrumentation and Methods for Astrophysics ,Instrumentation and Detectors (physics.ins-det) ,Scintillators, scintillation and light emission processes (solid, gas and liquid scintillators) ,Double-beta decay detectors ,scintillation and light emission processes (solid ,Double-beta decay detector ,Cryogenic detectors ,Scintillators ,Crystal scintillator ,Energy (signal processing) - Abstract
A scintillating bolometer based on a large cubic Li$_{2}$$^{100}$MoO$_4$ crystal (45 mm side) and a Ge wafer (scintillation detector) has been operated in the CROSS cryogenic facility at the Canfranc underground laboratory in Spain. The dual-readout detector is a prototype of the technology that will be used in the next-generation $0\nu2\beta$ experiment CUPID. The measurements were performed at 18 and 12 mK temperature in a pulse tube dilution refrigerator. This setup utilizes the same technology as the CUORE cryostat that will host CUPID and so represents an accurate estimation of the expected performance. The Li$_{2}$$^{100}$MoO$_4$ bolometer shows a high energy resolution of 6 keV FWHM at the 2615 keV $\gamma$ line. The detection of scintillation light for each event triggered by the Li$_{2}$$^{100}$MoO$_4$ bolometer allowed for a full separation ($\sim$8$\sigma$) between $\gamma$($\beta$) and $\alpha$ events above 2 MeV. The Li$_{2}$$^{100}$MoO$_4$ crystal also shows a high internal radiopurity with $^{228}$Th and $^{226}$Ra activities of less than 3 and 8 $\mu$Bq/kg, respectively. Taking also into account the advantage of a more compact and massive detector array, which can be made of cubic-shaped crystals (compared to the cylindrical ones), this test demonstrates the great potential of cubic Li$_{2}$$^{100}$MoO$_4$ scintillating bolometers for high-sensitivity searches for the $^{100}$Mo $0\nu2\beta$ decay in CROSS and CUPID projects., Comment: 19 pages, 7 figures, 1 table
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- 2021
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247. Measurement of the 2νββ Decay Rate and Spectral Shape of ^{100}Mo from the CUPID-Mo Experiment.
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Augier C, Barabash AS, Bellini F, Benato G, Beretta M, Bergé L, Billard J, Borovlev YA, Cardani L, Casali N, Cazes A, Celi E, Chapellier M, Chiesa D, Dafinei I, Danevich FA, De Jesus M, Dixon T, Dumoulin L, Eitel K, Ferri F, Fujikawa BK, Gascon J, Gironi L, Giuliani A, Grigorieva VD, Gros M, Helis DL, Huang HZ, Huang R, Imbert L, Johnston J, Juillard A, Khalife H, Kleifges M, Kobychev VV, Kolomensky YG, Konovalov SI, Kotila J, Loaiza P, Ma L, Makarov EP, de Marcillac P, Mariam R, Marini L, Marnieros S, Navick XF, Nones C, Norman EB, Olivieri E, Ouellet JL, Pagnanini L, Pattavina L, Paul B, Pavan M, Peng H, Pessina G, Pirro S, Poda DV, Polischuk OG, Pozzi S, Previtali E, Redon T, Rojas A, Rozov S, Sanglard V, Scarpaci JA, Schmidt B, Shen Y, Shlegel VN, Šimkovic F, Singh V, Tomei C, Tretyak VI, Umatov VI, Vagneron L, Velázquez M, Ware B, Welliver B, Winslow L, Xue M, Yakushev E, Zarytskyy M, and Zolotarova AS
- Abstract
Neutrinoless double beta decay (0νββ) is a yet unobserved nuclear process that would demonstrate Lepton number violation, a clear evidence of beyond standard model physics. The process two neutrino double beta decay (2νββ) is allowed by the standard model and has been measured in numerous experiments. In this Letter, we report a measurement of 2νββ decay half-life of ^{100}Mo to the ground state of ^{100}Ru of [7.07±0.02(stat)±0.11(syst)]×10^{18} yr by the CUPID-Mo experiment. With a relative precision of ±1.6% this is the most precise measurement to date of a 2νββ decay rate in ^{100}Mo. In addition, we constrain higher-order corrections to the spectral shape, which provides complementary nuclear structure information. We report a novel measurement of the shape factor ξ_{3,1}=0.45±0.03(stat)±0.05(syst) based on a constraint on the ratio of higher-order terms from theory, which can be reliably calculated. This is compared to theoretical predictions for different nuclear models. We also extract the first value for the effective axial vector coupling constant obtained from a spectral shape study of 2νββ decay.
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- 2023
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248. New Limit for Neutrinoless Double-Beta Decay of ^{100}Mo from the CUPID-Mo Experiment.
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Armengaud E, Augier C, Barabash AS, Bellini F, Benato G, Benoît A, Beretta M, Bergé L, Billard J, Borovlev YA, Bourgeois C, Brudanin VB, Camus P, Cardani L, Casali N, Cazes A, Chapellier M, Charlieux F, Chiesa D, de Combarieu M, Dafinei I, Danevich FA, De Jesus M, Dixon T, Dumoulin L, Eitel K, Ferri F, Fujikawa BK, Gascon J, Gironi L, Giuliani A, Grigorieva VD, Gros M, Guerard E, Helis DL, Huang HZ, Huang R, Johnston J, Juillard A, Khalife H, Kleifges M, Kobychev VV, Kolomensky YG, Konovalov SI, Leder A, Loaiza P, Ma L, Makarov EP, de Marcillac P, Mariam R, Marini L, Marnieros S, Misiak D, Navick XF, Nones C, Norman EB, Novati V, Olivieri E, Ouellet JL, Pagnanini L, Pari P, Pattavina L, Paul B, Pavan M, Peng H, Pessina G, Pirro S, Poda DV, Polischuk OG, Pozzi S, Previtali E, Redon T, Rojas A, Rozov S, Rusconi C, Sanglard V, Scarpaci JA, Schäffner K, Schmidt B, Shen Y, Shlegel VN, Siebenborn B, Singh V, Tomei C, Tretyak VI, Umatov VI, Vagneron L, Velázquez M, Welliver B, Winslow L, Xue M, Yakushev E, Zarytskyy M, and Zolotarova AS
- Abstract
The CUPID-Mo experiment at the Laboratoire Souterrain de Modane (France) is a demonstrator for CUPID, the next-generation ton-scale bolometric 0νββ experiment. It consists of a 4.2 kg array of 20 enriched Li_{2}^{100}MoO_{4} scintillating bolometers to search for the lepton-number-violating process of 0νββ decay in ^{100}Mo. With more than one year of operation (^{100}Mo exposure of 1.17 kg×yr for physics data), no event in the region of interest and, hence, no evidence for 0νββ is observed. We report a new limit on the half-life of 0νββ decay in ^{100}Mo of T_{1/2}>1.5×10^{24} yr at 90% C.I. The limit corresponds to an effective Majorana neutrino mass ⟨m_{ββ}⟩<(0.31-0.54) eV, dependent on the nuclear matrix element in the light Majorana neutrino exchange interpretation.
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- 2021
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249. First Germanium-Based Constraints on Sub-MeV Dark Matter with the EDELWEISS Experiment.
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Arnaud Q, Armengaud E, Augier C, Benoît A, Bergé L, Billard J, Broniatowski A, Camus P, Cazes A, Chapellier M, Charlieux F, De Jésus M, Dumoulin L, Eitel K, Elkhoury E, Fillipini JB, Filosofov D, Gascon J, Giuliani A, Gros M, Jin Y, Juillard A, Kleifges M, Lattaud H, Marnieros S, Misiak D, Navick XF, Nones C, Olivieri E, Oriol C, Pari P, Paul B, Poda D, Rozov S, Salagnac T, Sanglard V, Siebenborn B, Vagneron L, Weber M, Yakushev E, and Zolotarova A
- Abstract
We present the first Ge-based constraints on sub-MeV/c^{2} dark matter (DM) particles interacting with electrons using a 33.4 g Ge cryogenic detector with a 0.53 electron-hole pair (rms) resolution, operated underground at the Laboratoire Souterrain de Modane. Competitive constraints are set on the DM-electron scattering cross section, as well as on the kinetic mixing parameter of dark photons down to 1 eV/c^{2}. In particular, the most stringent limits are set for dark photon DM in the 6 to 9 eV/c^{2} range. These results demonstrate the high relevance of Ge cryogenic detectors for the search of DM-induced eV-scale electron signals.
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- 2020
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250. Development of 100 Mo -containing scintillating bolometers for a high-sensitivity neutrinoless double-beta decay search.
- Author
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Armengaud E, Augier C, Barabash AS, Beeman JW, Bekker TB, Bellini F, Benoît A, Bergé L, Bergmann T, Billard J, Boiko RS, Broniatowski A, Brudanin V, Camus P, Capelli S, Cardani L, Casali N, Cazes A, Chapellier M, Charlieux F, Chernyak DM, de Combarieu M, Coron N, Danevich FA, Dafinei I, Jesus M, Devoyon L, Domizio SD, Dumoulin L, Eitel K, Enss C, Ferroni F, Fleischmann A, Foerster N, Gascon J, Gastaldo L, Gironi L, Giuliani A, Grigorieva VD, Gros M, Hehn L, Hervé S, Humbert V, Ivannikova NV, Ivanov IM, Jin Y, Juillard A, Kleifges M, Kobychev VV, Konovalov SI, Koskas F, Kozlov V, Kraus H, Kudryavtsev VA, Laubenstein M, Sueur HL, Loidl M, Magnier P, Makarov EP, Mancuso M, de Marcillac P, Marnieros S, Marrache-Kikuchi C, Nagorny S, Navick XF, Nikolaichuk MO, Nones C, Novati V, Olivieri E, Pagnanini L, Pari P, Pattavina L, Pavan M, Paul B, Penichot Y, Pessina G, Piperno G, Pirro S, Plantevin O, Poda DV, Queguiner E, Redon T, Rodrigues M, Rozov S, Rusconi C, Sanglard V, Schäffner K, Scorza S, Shlegel VN, Siebenborn B, Strazzer O, Tcherniakhovski D, Tomei C, Tretyak VI, Umatov VI, Vagneron L, Vasiliev YV, Velázquez M, Vignati M, Weber M, Yakushev E, and Zolotarova AS
- Abstract
This paper reports on the development of a technology involving 100 Mo -enriched scintillating bolometers, compatible with the goals of CUPID, a proposed next-generation bolometric experiment to search for neutrinoless double-beta decay. Large mass ( ∼ 1 kg ), high optical quality, radiopure 100 Mo -containing zinc and lithium molybdate crystals have been produced and used to develop high performance single detector modules based on 0.2-0.4 kg scintillating bolometers. In particular, the energy resolution of the lithium molybdate detectors near the Q -value of the double-beta transition of 100 Mo (3034 keV) is 4-6 keV FWHM. The rejection of the α -induced dominant background above 2.6 MeV is better than 8 σ . Less than 10 μ Bq/kg activity of 232 Th ( 228 Th ) and 226 Ra in the crystals is ensured by boule recrystallization. The potential of 100 Mo -enriched scintillating bolometers to perform high sensitivity double-beta decay searches has been demonstrated with only 10 kg × d exposure: the two neutrino double-beta decay half-life of 100 Mo has been measured with the up-to-date highest accuracy as T 1 / 2 = [6.90 ± 0.15(stat.) ± 0.37(syst.)] × 10 18 years . Both crystallization and detector technologies favor lithium molybdate, which has been selected for the ongoing construction of the CUPID-0/Mo demonstrator, containing several kg of 100 Mo ., (© The Author(s) 2017.)
- Published
- 2017
- Full Text
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