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Artículos de revistas sobre el tema "CRESST"

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Publicado: 11 de marzo de 2023

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1

Angloher, G., M. Bauer, I. Bavykina, A. Bento, A. Brown, C. Bucci, C. Ciemniak et al. "CRESST". EAS Publications Series 36 (2009): 231–36. http://dx.doi.org/10.1051/eas/0936032.

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2

Kraus, H., G. Angloher, M. Bauer, I. Bavykina, C. Bucci, P. Christ, C. Ciemniak et al. "CRESST – status and future". Nuclear Physics B - Proceedings Supplements 173 (noviembre de 2007): 104–7. http://dx.doi.org/10.1016/j.nuclphysbps.2007.08.156.

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3

Seidel, W., M. Bravin, M. Bruckmayer, C. Bucci, S. Cooper, P. DiStefano, F. V. Feilitzsch et al. "The CRESST dark matter search". Physics of Atomic Nuclei 63, n.º 7 (julio de 2000): 1242–48. http://dx.doi.org/10.1134/1.855777.

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4

Bravin, M., M. Bruckmayer, C. Bucci, S. Cooper, S. Giordano, F. von Feilitzsch, J. Höhne et al. "The CRESST dark matter search". Astroparticle Physics 12, n.º 1-2 (octubre de 1999): 107–14. http://dx.doi.org/10.1016/s0927-6505(99)00073-0.

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5

Cozzini, C., G. Angloher, C. Bucci, F. von Feilitzsch, T. Frank, D. Hauff, S. Henry et al. "CRESST cryogenic dark matter search". New Astronomy Reviews 49, n.º 2-6 (mayo de 2005): 255–58. http://dx.doi.org/10.1016/j.newar.2005.01.016.

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6

Zerle, L., C. Bucci, M. Bühler, S. Cooper, F. v. Feilitzsch, J. Höhne, V. Jörgens et al. "The CRESST dark matter search". Nuclear Physics B - Proceedings Supplements 70, n.º 1-3 (enero de 1999): 85–89. http://dx.doi.org/10.1016/s0920-5632(98)00393-4.

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7

Jochum, J., G. Angloher, M. Bauer, I. Bavykina, A. Brown, C. Bucci, C. Ciemniak et al. "The CRESST dark matter search". Progress in Particle and Nuclear Physics 66, n.º 2 (abril de 2011): 202–7. http://dx.doi.org/10.1016/j.ppnp.2011.01.007.

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8

Jochum, J., M. Bravin, M. Bruckmayer, C. Bucci, S. Cooper, S. Giordano, F. v. Feilitzsch et al. "The CRESST dark matter search". Nuclear Physics B - Proceedings Supplements 87, n.º 1-3 (junio de 2000): 70–73. http://dx.doi.org/10.1016/s0920-5632(00)00634-4.

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9

Pröbst, F., G. Angloher, M. Bruckmayer, C. Bucci, S. Cooper, P. Di Stefano, F. von Feilitzsch et al. "Results of CRESST phase I". Nuclear Physics B - Proceedings Supplements 110 (julio de 2002): 67–69. http://dx.doi.org/10.1016/s0920-5632(02)01453-6.

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10

Pröbst, F. "Results of CRESST phase I". Nuclear Physics B - Proceedings Supplements 110, n.º 2 (julio de 2002): 67–69. http://dx.doi.org/10.1016/s0920-5632(02)80096-2.

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11

Westphal, W., C. Coppi, F. v. Feilitzsch, C. Isaila, T. Jagemann, J. Jochum, J. König et al. "Detector calibration measurements in CRESST". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 559, n.º 2 (abril de 2006): 372–74. http://dx.doi.org/10.1016/j.nima.2005.12.013.

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12

Åström, J., F. Pröbst, P. C. F. Di Stefano, L. Stodolsky, J. Timonen, C. Bucci, S. Cooper et al. "Fracture processes studied in CRESST". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 559, n.º 2 (abril de 2006): 754–56. http://dx.doi.org/10.1016/j.nima.2005.12.127.

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13

Seidel, W., G. Angloher, M. Bauer, I. Bavykina, A. Bento, A. Brown, C. Bucci et al. "The CRESST dark matter search". Journal of Physics: Conference Series 120, n.º 4 (1 de julio de 2008): 042020. http://dx.doi.org/10.1088/1742-6596/120/4/042020.

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14

Westphal, W., C. Coppi, F. von Feilitzsch, C. Isaila, J. König, W. Potzel, W. Rau et al. "Dark-matter search with CRESST". Czechoslovak Journal of Physics 56, n.º 5 (mayo de 2006): 535–42. http://dx.doi.org/10.1007/s10582-006-0118-2.

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15

Stodolsky, Leo, G. Angloher, M. Bauer, I. Bavykina, A. Bento, C. Bucci, C. Ciemniak et al. "The CRESST II Dark Matter Search". Journal of Physics: Conference Series 384 (13 de septiembre de 2012): 012013. http://dx.doi.org/10.1088/1742-6596/384/1/012013.

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16

Angloher, G., P. Bauer, N. Ferreiro, D. Hauff, A. Tanzke, R. Strauss, M. Kiefer et al. "Quasiparticle Diffusion in CRESST Light Detectors". Journal of Low Temperature Physics 184, n.º 1-2 (4 de febrero de 2016): 323–29. http://dx.doi.org/10.1007/s10909-016-1512-1.

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17

Petricca, F., G. Angloher, C. Cozzini, T. Frank, D. Hauff, J. Ninković, F. Pröbst, W. Seidel y S. Uchaikin. "Light detector development for CRESST II". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 520, n.º 1-3 (marzo de 2004): 193–96. http://dx.doi.org/10.1016/j.nima.2003.11.291.

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18

Henry, S., H. Kraus, B. Majorovits y Y. Ramachers. "Multichannel SQUID readout for CRESST II". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 520, n.º 1-3 (marzo de 2004): 588–91. http://dx.doi.org/10.1016/j.nima.2003.11.322.

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19

Lang, Rafael F. y Wolfgang Seidel. "Search for dark matter with CRESST". New Journal of Physics 11, n.º 10 (16 de octubre de 2009): 105017. http://dx.doi.org/10.1088/1367-2630/11/10/105017.

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20

Wulandari, H., F. Von Feilitzsch, M. Huber, Th Jagemann, J. Jochum, T. Lachenmaier, J. C. Lanfranchi et al. "Study on Neutron-induced Background in the CRESST Experiment". Symposium - International Astronomical Union 220 (2004): 491–92. http://dx.doi.org/10.1017/s0074180900183895.

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CRESST II is an experiment for direct WIMP search, using cryogenic detectors. the ratio of the two signals (temperature rise and scintillation light) measured for each interaction is an excellent parameter for discrimination of the radioactive background. the main remaining background is the neutron flux present at the experimental site, since neutrons produce the same signals as WIMPs do. Based on Monte Carlo simulations the present work shows how neutrons from different origins affect CRESST and which measures have to be taken into account to reach the sensitivity goal.
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21

Strauss, R., G. Angloher, A. Bento, C. Bucci, L. Canonica, X. Defay, A. Erb et al. "The CRESST-III low-mass WIMP detector". Journal of Physics: Conference Series 718 (mayo de 2016): 042048. http://dx.doi.org/10.1088/1742-6596/718/4/042048.

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22

Angloher, G., M. Altmann, M. Bruckmayer, C. Bucci, S. Cooper, C. Cozzini, P. Di Stefano et al. "Dark matter search with CRESST cryogenic detectors". Physics of Atomic Nuclei 66, n.º 3 (marzo de 2003): 494–96. http://dx.doi.org/10.1134/1.1563712.

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23

Rau, W., G. Angloher, I. Bavykina, M. Bauer, C. Bucci, P. Christ, C. Coppi et al. "Results and status of the CRESST experiment". Journal of Physics: Conference Series 39 (1 de mayo de 2006): 75–81. http://dx.doi.org/10.1088/1742-6596/39/1/016.

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24

Kiefer, Michael, Franz Pröbst, Godehard Angloher, Irina Bavykina, Dieter Hauff y Wolfgang Seidel. "Glued detectors for the CRESST-II experiment". Optical Materials 31, n.º 10 (agosto de 2009): 1410–14. http://dx.doi.org/10.1016/j.optmat.2008.09.019.

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25

Strauss, R., G. Angloher, A. Bento, C. Bucci, L. Canonica, X. Defay, A. Erb et al. "Exploring Low-Mass Dark Matter with CRESST". Journal of Low Temperature Physics 184, n.º 3-4 (28 de enero de 2016): 866–72. http://dx.doi.org/10.1007/s10909-016-1492-1.

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26

Lang, R. F., G. Angloher, M. Bauer, I. Bavykina, A. Bento, A. Brown, C. Bucci et al. "Electron and gamma background in CRESST detectors". Astroparticle Physics 32, n.º 6 (enero de 2010): 318–24. http://dx.doi.org/10.1016/j.astropartphys.2009.09.009.

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27

Jagemann, Thomas. "CRESST Detectors for Nonbaryonic Cold Dark Matter Particles". Symposium - International Astronomical Union 220 (2004): 493–94. http://dx.doi.org/10.1017/s0074180900183901.

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The CRESST experiment is set up for the direct detection of Weakly Interacting Massive Particles (WIMPs) which our Galactic dark matter halo possibly consists of. the employed detection method is elastic scattering by nuclei. the recoiling nucleus deposits most of its energy in the form of lattice vibrations in the detector. Cooling the detector to very low temperatures (mK) enhances the temperature rise due to the energy deposition. the crucial parameter for direct WIMP searches is the sensitivity to the WIMP interaction cross section in a certain range of possible WIMP masses. CRESST is now sensitive enough to explore the parameter space predicted by supersymmetric models.
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28

Henry, S., N. Bazin, H. Kraus, B. Majorovits, M. Malek, R. McGowan, V. B. Mikhailik, Y. Ramachers y A. J. B. Tolhurst. "The 66-channel SQUID readout for CRESST II". Journal of Instrumentation 2, n.º 11 (12 de noviembre de 2007): P11003. http://dx.doi.org/10.1088/1748-0221/2/11/p11003.

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29

Scholl, S. y J. Jochum. "Neutron background simulation for the CRESST–II experiment". Journal of Physics: Conference Series 375, n.º 1 (30 de julio de 2012): 012020. http://dx.doi.org/10.1088/1742-6596/375/1/012020.

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30

Angloher, G., C. Bucci, C. Cozzini, F. von Feilitzsch, T. Frank, D. Hauff, S. Henry et al. "CRESST-II: dark matter search with scintillating absorbers". Nuclear Physics B - Proceedings Supplements 138 (enero de 2005): 153–55. http://dx.doi.org/10.1016/j.nuclphysbps.2004.11.035.

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31

Pantić, Emilija, Antonio Bento, Dieter Hauff, Federica Petricca, Franz Pröbst y Wolfgang Seidel. "Development of superconducting absorbers for CRESST light detectors". Optical Materials 31, n.º 10 (agosto de 2009): 1398–404. http://dx.doi.org/10.1016/j.optmat.2008.09.017.

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32

Jochum, J. "CRESST direct Dark Matter search with cryogenic detectors". Progress in Particle and Nuclear Physics 57, n.º 1 (julio de 2006): 357–65. http://dx.doi.org/10.1016/j.ppnp.2005.11.023.

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33

Roth, S., G. Angloher, M. Bauer, I. Bavykina, A. Bento, A. Brown, C. Bucci, C. Ciemniak, C. Coppi y G. Deuter. "Direct dark matter search with CRESST and EURECA". Progress in Particle and Nuclear Physics 64, n.º 2 (abril de 2010): 457–59. http://dx.doi.org/10.1016/j.ppnp.2009.12.075.

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34

Sisti, M., M. Bravin, M. Bruckmayer, C. Bucci, S. Cooper, P. Di Stefano, S. Giordano et al. "The CRESST dark matter experiment: status and perspectives". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 444, n.º 1-2 (abril de 2000): 312–14. http://dx.doi.org/10.1016/s0168-9002(99)01405-9.

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35

Kuźniak, M., M. G. Boulay y T. Pollmann. "Surface roughness interpretation of 730kgdays CRESST-II results". Astroparticle Physics 36, n.º 1 (agosto de 2012): 77–82. http://dx.doi.org/10.1016/j.astropartphys.2012.05.005.

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36

Angloher, G., C. Bucci, C. Cozzini, F. von Feilitzsch, T. Frank, D. Hauff, S. Henry et al. "Cresst-II: dark matter search with scintillating absorbers". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 520, n.º 1-3 (marzo de 2004): 108–11. http://dx.doi.org/10.1016/j.nima.2003.11.254.

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37

Petricca, F., G. Angloher, C. Bucci, P. Christ, C. Cozzini, F. von Feilitzsch, D. Hauff et al. "CRESST: First results with the phonon-light technique". Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 559, n.º 2 (abril de 2006): 375–77. http://dx.doi.org/10.1016/j.nima.2005.12.014.

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38

DRUKIER, A. K. y S. NUSSINOV. "TOWARDS DETECTION OF LOW MASS WIMPs (MWIMP<10GeV/c2): MINI-REVIEW". International Journal of Modern Physics A 28, n.º 26 (20 de octubre de 2013): 1330033. http://dx.doi.org/10.1142/s0217751x13300330.

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Weakly Interacting Massive Particles (WIMPs) may constitute most of the matter in the Universe. There are intriguing results from DAMA/LIBRA, CoGeNT and CRESST-II, and more recently CDMS-Si suggesting a relatively light dark matter candidate of mass <10 GeV /c2. At the same time, experiments using heavy nuclear targets such as CDMS-Ge and XENON detectors suggest that there is no DM candidates with MW>15 GeV /c2. We review the existing experiments and the problems associated with light mass WIMP detection. We find that all six experiments considered (DAMA, CoGeNT, CRESST, CDMS-Si, CDMS-Ge, XENON) are consistent if one assumes that the mass of WIMP is lower than expected: 3.4<MW<6.8 GeV /c2. This is followed by a discussion of the properties of "new" detectors, which may enable more reliable detection of low mass WIMPs.
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39

Petricca, F., G. Angloher, M. Bauer, I. Bavykina, A. Bento, C. Bucci, C. Ciemniak et al. "Latest results from the CRESST-II Dark Matter Search". Journal of Physics: Conference Series 375, n.º 1 (30 de julio de 2012): 012003. http://dx.doi.org/10.1088/1742-6596/375/1/012003.

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40

Schäffner, K., F. Pröbst, W. Seidel, F. Petricca, D. Hauff y R. Kleindienst. "Alternative Scintillating Materials for the CRESST Dark Matter Search". Journal of Low Temperature Physics 167, n.º 5-6 (25 de enero de 2012): 1075–80. http://dx.doi.org/10.1007/s10909-012-0488-8.

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41

Angloher, G., M. Bauer, I. Bavykina, A. Bento, A. Brown, C. Bucci, C. Ciemniak, C. Coppi, G. Deuter y F. von Feilitzsch. "Commissioning run of the CRESST-II dark matter search". Astroparticle Physics 31, n.º 4 (mayo de 2009): 270–76. http://dx.doi.org/10.1016/j.astropartphys.2009.02.007.

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42

Bikit, I., D. Mrđa, I. Aničin y M. Vesković. "Comment on “Electron and gamma background in CRESST detectors”". Astroparticle Physics 34, n.º 2 (septiembre de 2010): 139–41. http://dx.doi.org/10.1016/j.astropartphys.2010.05.002.

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43

Kopp, Joachim, Thomas Schwetz y Jure Zupan. "Light dark matter in the light of CRESST-II". Journal of Cosmology and Astroparticle Physics 2012, n.º 03 (2 de marzo de 2012): 001. http://dx.doi.org/10.1088/1475-7516/2012/03/001.

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44

Strauss, R., G. Angloher, A. Bento, C. Bucci, L. Canonica, A. Erb, F. v. Feilitzsch et al. "Beta/gamma and alpha backgrounds in CRESST-II Phase 2". Journal of Cosmology and Astroparticle Physics 2015, n.º 06 (16 de junio de 2015): 030. http://dx.doi.org/10.1088/1475-7516/2015/06/030.

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45

Mancuso, M., A. H. Abdelhameed, G. Angloher, R. Breier, P. Bauer, A. Bento, E. Bertoldo et al. "Searches for Light Dark Matter with the CRESST-III Experiment". Journal of Low Temperature Physics 199, n.º 1-2 (1 de febrero de 2020): 547–55. http://dx.doi.org/10.1007/s10909-020-02343-3.

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46

Coppi, C., C. Ciemniak, F. von Feilitzsch, A. Gütlein, H. Hagn, C. Isaila, J. Jochum et al. "Characterization of the CRESST detectors by neutron induced nuclear recoils". EAS Publications Series 36 (2009): 315–17. http://dx.doi.org/10.1051/eas/0936045.

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47

Catena, Riccardo y Vanessa Zema. "Prospects for dark matter signal discovery and model selection via timing information in a low-threshold experiment". Journal of Cosmology and Astroparticle Physics 2022, n.º 02 (1 de febrero de 2022): 022. http://dx.doi.org/10.1088/1475-7516/2022/02/022.

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Abstract In the recent years, many low-threshold dark matter (DM) direct detection experiments have reported the observation of unexplained excesses of events at low energies. Exemplary for these, the experiment CRESST has detected unidentified events below an energy of about 200 eV — a result hampering the detector performance in the search for GeV-scale DM. In this work, we test the impact of nuclear recoil timing information on the potential for DM signal discovery and model selection on a low-threshold experiment limited by the presence of an unidentified background resembling this population of low-energy events. Among the different targets explored by the CRESST collaboration, here we focus on Al2O3, as a sapphire detector was shown to reach an energy threshold as low as 19.7 eV [1]. We test the ability of a low-threshold experiment to discover a signal above a given background, or to reject the spin-independent interaction in favour of a magnetic dipole coupling in terms of p-values. We perform our p-value calculations: 1) taking timing information into account; and 2) assuming that the latter is not available. By comparing the two approaches, we find that under our assumptions timing information has a marginal impact on the potential for DM signal discovery, while provides more significant results for the selection between the two models considered. For the model parameters explored here, we find that the p-value for rejecting spin-independent interactions in favour of a magnetic dipole coupling is about 0.11 when the experimental exposure is 460 g×year and smaller (about 0.06) if timing information is available. The conclusion on the role of timing information remains qualitatively unchanged for exposures as large as 1 kg×5 year. At the same time, our results show that a 90% C.L. rejection of spin-independent interactions in favour of a magnetic dipole coupling is within reach of an upgrade of the CRESST experiment [2].
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48

Gütlein, A., G. Angloher, A. Bento, C. Bucci, L. Canonica, X. Defay, A. Erb et al. "Search for dark photons using data from CRESST-II Phase 2". Journal of Physics: Conference Series 888 (septiembre de 2017): 012208. http://dx.doi.org/10.1088/1742-6596/888/1/012208.

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49

Roth, S., C. Ciemniak, C. Coppi, F. v. Feilitzsch, A. Gütlein, C. Isaila, J. C. Lanfranchi, S. Pfister, W. Potzel y W. Westphal. "Cryogenic composite detectors for the dark matter experiments CRESST and EURECA". Optical Materials 31, n.º 10 (agosto de 2009): 1415–20. http://dx.doi.org/10.1016/j.optmat.2008.09.013.

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50

Rothe, J., G. Angloher, P. Bauer, A. Bento, C. Bucci, L. Canonica, A. D’Addabbo et al. "TES-Based Light Detectors for the CRESST Direct Dark Matter Search". Journal of Low Temperature Physics 193, n.º 5-6 (10 de mayo de 2018): 1160–66. http://dx.doi.org/10.1007/s10909-018-1944-x.

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