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Start Over Author "Cerdonio M" Journal physical review letters
10 results on '"Cerdonio M"'

1. Nonequilibrium Steady-State Fluctuations in Actively Cooled Resonators

Author

Bonaldi, M., primary, Conti, L., additional, De Gregorio, P., additional, Rondoni, L., additional, Vedovato, G., additional, Vinante, A., additional, Bignotto, M., additional, Cerdonio, M., additional, Falferi, P., additional, Liguori, N., additional, Longo, S., additional, Mezzena, R., additional, Ortolan, A., additional, Prodi, G. A., additional, Salemi, F., additional, Taffarello, L., additional, Vitale, S., additional, and Zendri, J.-P., additional

Published
2009
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2. Feedback Cooling of the Normal Modes of a Massive Electromechanical System to Submillikelvin Temperature

Author

Vinante, A., primary, Bignotto, M., additional, Bonaldi, M., additional, Cerdonio, M., additional, Conti, L., additional, Falferi, P., additional, Liguori, N., additional, Longo, S., additional, Mezzena, R., additional, Ortolan, A., additional, Prodi, G. A., additional, Salemi, F., additional, Taffarello, L., additional, Vedovato, G., additional, Vitale, S., additional, and Zendri, J.-P., additional

Published
2008
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3. Erratum: Upper Limits on Gravitational-Wave Emission in Association with the 27 Dec 2004 Giant Flare of SGR1806-20 [Phys. Rev. Lett.95, 081103 (2005)]

Author

Baggio, L., primary, Bignotto, M., additional, Bonaldi, M., additional, Cerdonio, M., additional, Conti, L., additional, De Rosa, M., additional, Falferi, P., additional, Fortini, P., additional, Inguscio, M., additional, Liguori, N., additional, Marin, F., additional, Mezzena, R., additional, Mion, A., additional, Ortolan, A., additional, Prodi, G. A., additional, Poggi, S., additional, Salemi, F., additional, Soranzo, G., additional, Taffarello, L., additional, Vedovato, G., additional, Vinante, A., additional, Vitale, S., additional, and Zendri, J. P., additional

Published
2005
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4. Upper Limits on Gravitational-Wave Emission in Association with the 27 Dec 2004 Giant Flare of SGR1806-20

Author

Baggio, L., primary, Bignotto, M., additional, Bonaldi, M., additional, Cerdonio, M., additional, Conti, L., additional, De Rosa, M., additional, Falferi, P., additional, Fortini, P., additional, Inguscio, M., additional, Liguori, N., additional, Marin, F., additional, Mezzena, R., additional, Mion, A., additional, Ortolan, A., additional, Prodi, G. A., additional, Poggi, S., additional, Salemi, F., additional, Soranzo, G., additional, Taffarello, L., additional, Vedovato, G., additional, Vinante, A., additional, Vitale, S., additional, and Zendri, J. P., additional

Published
2005
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5. 3-Mode Detection for Widening the Bandwidth of Resonant Gravitational Wave Detectors

Author

Baggio, L., primary, Bignotto, M., additional, Bonaldi, M., additional, Cerdonio, M., additional, Conti, L., additional, Falferi, P., additional, Liguori, N., additional, Marin, A., additional, Mezzena, R., additional, Ortolan, A., additional, Poggi, S., additional, Prodi, G. A., additional, Salemi, F., additional, Soranzo, G., additional, Taffarello, L., additional, Vedovato, G., additional, Vinante, A., additional, Vitale, S., additional, and Zendri, J. P., additional

Published
2005
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8. First Search for Gravitational Wave Bursts with a Network of Detectors

Author

Allen, Z. A., primary, Astone, P., additional, Baggio, L., additional, Busby, D., additional, Bassan, M., additional, Blair, D. G., additional, Bonaldi, M., additional, Bonifazi, P., additional, Carelli, P., additional, Cerdonio, M., additional, Coccia, E., additional, Conti, L., additional, Cosmelli, C., additional, Crivelli Visconti, V., additional, D'Antonio, S., additional, Fafone, V., additional, Falferi, P., additional, Fortini, P., additional, Frasca, S., additional, Hamilton, W. O., additional, Heng, I. S., additional, Ivanov, E. N., additional, Johnson, W. W., additional, Kingham, M., additional, Locke, C. R., additional, Marini, A., additional, Martinucci, V., additional, Mauceli, E., additional, McHugh, M. P., additional, Mezzena, R., additional, Minenkov, Y., additional, Modena, I., additional, Modestino, G., additional, Moleti, A., additional, Ortolan, A., additional, Pallottino, G. V., additional, Pizzella, G., additional, Prodi, G. A., additional, Rocco, E., additional, Ronga, F., additional, Salemi, F., additional, Santostasi, G., additional, Taffarello, L., additional, Terenzi, R., additional, Tobar, M. E., additional, Vedovato, G., additional, Vinante, A., additional, Visco, M., additional, Vitale, S., additional, Votano, L., additional, and Zendri, J. P., additional

Published
2000
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9. Search for an Ultralight Scalar Dark Matter Candidate with the AURIGA Detector.

Author

Branca A, Bonaldi M, Cerdonio M, Conti L, Falferi P, Marin F, Mezzena R, Ortolan A, Prodi GA, Taffarello L, Vedovato G, Vinante A, Vitale S, and Zendri JP

Abstract

A search for a new scalar field, called moduli, has been performed using the cryogenic resonant-mass AURIGA detector. Predicted by string theory, moduli may provide a significant contribution to the dark matter (DM) component of our Universe. If this is the case, the interaction of ordinary matter with the local DM moduli, forming the Galaxy halo, will cause an oscillation of solid bodies with a frequency corresponding to the mass of moduli. In the sensitive band of AURIGA, some 100 Hz at around 1 kHz, the expected signal, with Q=△f/f∼10^{6}, is a narrow peak, △f∼1  mHz. Here the detector strain sensitivity is h_{s}∼2×10^{-21}  Hz^{-1/2}, within a factor of 2. These numbers translate to upper limits at 95% C.L. on the moduli coupling to ordinary matter (d_{e}+d_{m_{e}})≲10^{-5} around masses m_{ϕ}=3.6×10^{-12}  eV, for the standard DM halo model with ρ_{DM}=0.3  GeV/cm^{3}.

Published
2017
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