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1.
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Latest results of the CAST axion search
/ Irastorza, I G (DAPNIA, Saclay ; Zaragoza U.) ; Arik, E (Dogus U., Kadikoy) ; Aune, S (DAPNIA, Saclay) ; Autiero, D (CERN) ; Barth, K (CERN) ; Belov, A (Moscow, INR) ; Beltran, B (Zaragoza U.) ; Borghi, S (CERN) ; Bourlis, G (Hellenic Open U., Patras) ; Boydag, F S (Dogus U., Kadikoy) et al.
/CAST
2007 - 9 p.
- Published in : , pp. 301-310
Fulltext: PDF;
In : 42nd Rencontres de Moriond, La Thuile, Italy, 10 - 17 Mar 2007, pp.301-310
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2.
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Solar axion search with the CAST experiment
/ Borghi, S (CERN ; Glasgow U.) ; Arik, E (Dogus U., Kadikoy ; Bogazici U.) ; Aune, S (IRFU, Saclay) ; Autiero, D (CERN ; Lyon, IPN) ; Barth, K (CERN) ; Belov, A (Moscow, INR) ; Beltrán, B (Zaragoza U.) ; Bourlis, G (Hellenic Open U., Patras) ; Boydag, F S (Dogus U., Kadikoy ; Bogazici U.) ; Bräuninger, H (Garching, Max Planck Inst., MPE) et al.
/CAST
The CAST (CERN Axion Solar Telescope) experiment is searching for solar axions by their conversion into photons inside the magnet pipe of a LHC prototype dipole. In the phase II, CAST is operating with a buffer gas inside the magnet bore apertures in order to extent the sensitivity of the experiment to larger axion masses. [...]
Paris, France : Moriond, 2008 - 8 p.
- Published in : , pp. 465-472
Fulltext: PDF;
In : 43rd Rencontres de Moriond, La Thuile, Italy, 01 - 08 Mar 2008, pp.465-472
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3.
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An update on the Axion Helioscopes front: current activities at CAST and the IAXO project
/ Dafni, T (Zaragoza U.) ; Arik, M (Dogus U., Kadikoy) ; Armengaud, E (IRFU, SPhN, Saclay) ; Aune, S (IRFU, Saclay) ; Avignone, F T (South Carolina U.) ; Barth, K (CERN) ; Belov, A (Moscow, INR) ; Betz, M (CERN) ; Bräuninger, H (Garching, Max Planck Inst., MPE) ; Brax, P (CERN) et al.
Although they have not yet been detected, axions and axion-like particles (ALPs) continue to maintain the interest (even increasingly so) of the rare-event searches community as viable candidates for the Dark Matter of the Universe but also as a solution for several other puzzles of astrophysics. Their property of coupling to photons has inspired different experimental methods for their detection, one of which is the helioscope technique. [...]
2016 - 6 p.
- Published in : Nucl. Part. Phys. Proc. 273-275 (2016) 244-249
In : 37th International Conference on High Energy Physics, Valencia, Spain, 2 - 9 Jul 2014, pp.244-249
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4.
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EURECA – setting the scene for scintillators
/ Kraus, H (Oxford U.) ; Armengau, E. (IRFU, Saclay) ; Bauer, M. (Tubingen U.) ; Bavykina, I. (Munich, Max Planck Inst.) ; Benoit, A. (Grenoble, CRTBT) ; Bento, A. (Munich, Max Planck Inst.) ; Blumer, J. (Karlsruhe U., EKP ; Karlsruhe, Forschungszentrum) ; Bornschein, L. (Karlsruhe U., EKP) ; Broniatowski, A. (CSNSM, Orsay) ; Burghart, G. (CERN) et al.
EURECA (European Underground Rare Event Calorimeter Array) will be an astro-particle physics facility aiming to directly detect galactic dark matter. The Laboratoire Souterrain de Modane has been selected as host laboratory. [...]
2009
In : 1st International Workshop on Radiopure Scintillators for EURECA, Kiev, Ukraine, 9 - 10 Sep 2008, pp.7-11
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5.
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The CERN Axion Solar Telescope
/ Hasinoff, M D (CERN ; British Columbia U.) ; Andriamonje, S (DAPNIA, Saclay) ; Arik, E (Bogazici U.) ; Autiero, D (CERN) ; Avignone, F (South Carolina U.) ; Barth, K (CERN) ; Bingol, E (Darmstadt, Tech. Hochsch.) ; Brauninger, H (Garching, Max Planck Inst., MPE) ; Brodzinski, R (PNL, Richland) ; Carmona, J (U. Zaragoza (main)) et al.
The CAST experiment at CERN is using a decommissioned LHC prototype magnet to search for solar axions through their Primakoff conversion into x-ray photons. The magnet (B = 9.0 Tesla, L = 10 m) can track the sun each day for a total exposure time of ~180 minutes (sunrise + sunset). [...]
2003 - 7 p.
- Published in : 10.1142/9789812791160_0009
In : 4th International Workshop on New Worlds in Astroparticle Physics, Faro, Portugal, 5 - 7 Sep 2002, pp.103-109
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6.
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The IAXO Helioscope
/ Ferrer Ribas, E. (IRFU, Saclay) ; Armengaud, E. (IRFU, Saclay) ; Avignone, F.T. (South Carolina U.) ; Betz, M. (CERN) ; Brax, P. (IPhT, Saclay) ; Brun, P. (IRFU, Saclay) ; Cantatore, G. (INFN, Trieste ; Trieste U.) ; Carmona, J.M. (Zaragoza U.) ; Carosi, G.P. (LLNL, Livermore) ; Caspers, F. (CERN) et al.
The IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 10(4) better than CAST phase-I, resulting in sensitivity on g(a)(γ) one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm(2) spots coupled to ultra-low background Micromegas X-ray detectors. [...]
2015 - 8 p.
- Published in : J. Phys.: Conf. Ser. 650 (2015) 012009
IOP Open Access article: PDF;
In : 7th Symposium on large TPCs for low-energy rare event detection, Paris, France, 15 - 17 Dec 2014, pp.012009
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7.
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Sensitivity of NEXT-100 to neutrinoless double beta decay
/ NEXT Collaboration
NEXT-100 is an electroluminescent high-pressure xenon gas time projection chamber that will search for the neutrinoless double beta decay of Xe-136. The detector possesses two features of great value in neutrinoless double beta decay searches: very good energy resolution (better than 1% FWHM at the Q value of Xe-136) and track reconstruction for the discrimination of signal and background events. [...]
arXiv:1511.09246; FERMILAB-PUB-16-669-CD-ND.-
2016-05-26 - 30 p.
- Published in : JHEP 05 (2016) 159
Article from SCOAP3: PDF; Fulltext: PDF; Springer Open Access article: PDF; External link: Fermilab Library Server (fulltext available)
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8.
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The Next Generation of Axion Helioscopes: The International Axion Observatory (IAXO)
/ Vogel, J K (LLNL, Livermore) ; Armengaud, E (IRFU, Saclay) ; Avignone, F T (South Carolina U.) ; Betz, M (CERN) ; Brax, P (IRFU, Saclay) ; Brun, P (IRFU, Saclay) ; Cantatore, G (INFN, Trieste ; Trieste U.) ; Carmona, J M (Zaragoza U.) ; Carosi, G P (LLNL, Livermore) ; Caspers, F (CERN) et al.
The International Axion Observatory (IAXO) is a proposed 4 th -generation axion helioscope with the primary physics research goal to search for solar axions via their Primakoff conversion into photons of 1 – 10 keV energies in a strong magnetic field. IAXO will achieve a sensitivity to the axion-photon coupling g aγ down to a few ×10 −12 GeV −1 for a wide range of axion masses up to ∼ 0 . [...]
2015 - 8 p.
- Published in : Phys. Procedia 61 (2015) 193-200
Elsevier Open Access article: PDF;
In : 13th International Conference on Topics in Astroparticle and Underground Physics, Asilomar, CA, USA, 8 - 13 Sep 2013, pp.193-200
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