DARK MATTER IN COSMOLOGY QUANTUM MEASUREMENTS EXPERIMENTAL GRAV ITA Tl ON Matiere Noire et Cosmologie - Mesures Quantiques Gravitation Experimentale XVlth Moriond Worshop Les Arcs, Savoie, France -January 20-27, 1996 Dark Matter in Cosmology -Quantum Measurements Experimental Gravitation Series : Moriond Workshops ISBN 2-86332-203-6 ©Copyright 1996 by Editions Frontieres righrtess erved. All Thisb ooko,r p arttsh eremoaf,y n otb er eproduceidna nyf ormo rb ya nym eanse,l ectroonri c mechanical, inpchlotuodcionpgy riencgo,r dionrga nyi nformatsitoonra ge retsryisvtieanmlo w knowno rt ob ei nventweidt,h owurti ttpeenr missfiroomnt heP ublisher. EDITIONS FRONTIERES B.P. 33 Gif-sur-Yvette Cedex - France 91192 Printed in Singapore Proceedings of the XXXlst RENCONTRES DE MORIOND Series : Moriond Workshops Les Arcs, Savoie, France January 1996 20-27, DARK MATTER IN COSMOLOGY QUANTUM MEASUREMENTS EXPERIMENTAL GRAVITATION edited by R. Ansari (' Y. Giraud-Heraud c,� J. Tran Thanh Van � � j) 0 � r "<'l'o f'I 91 EDITIONS FRONTIERES IV XVlth Moriond Workshop Dark Matter in Cosmology - Quantum Measurements Experimental Gravitation was organized by J. Tran Thanh Van (Orsay) with the active collaboration of : Adelberger (Seattle) E. R. Ansari (Orsay) G. Chardin (Saclay) T. Damour (/HESB,u res/Yvette) Fackler (Livermore) 0. G. Fontaine (Paris) G. Gerbier (Sac/ay) Y. Giraud-Heraud (Paris) G. Greene (LoAsl amos) Guiderdoni (Paris) B. S. Haroche (Paris) Hinds (Cambridge) E. J. Kaplan (Paris) J.-M. Raimond (Paris) Sadoulet (Berkeley) B. v 96' RENCONTRES DE MORIOND The XXXIst Rencontres de Moriond were held in 1996 in Les Arcs 1800, Savoie, France. The first meeting took place at Moriond in the French Alps in 1966. There, experimental as well as theoretical physicists not only shared their scientific preoccupations but also the household chores. The participants in the first meeting were mainly French physicists interested in electromagnetic interactions. In the following years, a session on high energy strong interactions was also added. The main purpose of these meetings is to discuss recent developments in contemporary physics and also to promote effective collaboration between experimentalists and theorists in the field of elementary particle physics. By bringing together a relatively small number of participants, the meeting helps to develop better human relations as well as a more thorough and detailed discussion of the contributions. This concern of research and experimentation of new channels of communication and dialogue which from the start animated the Moriond meetings, inspired us to organize a simultaneous meeting of biologists on Cell Differenciation (1970) and to create the Moriond Astrophysics Meeting (1981). In the same spirit, we have started a new series on Condensed Matter Physics in January 1994. Common meetings between biologists, astrophysicists, condensed matter physicists and high energy physicists are organized to study the implications of the advances from one field into the others. I hope that these conferences and lively discussions may give birth to new analytical methods or new mathematical languages. At the XXXIst Rencontres de Moriond in 1996, four physics sessions, one astrophysics session and one biology session were held : *January 20-27 "Dark matter in cosmology, Quantum measurements and Experimental gravitation. "Correlated fermions and transport in mesoscopic systems" *March "Electroweak Interactions and Unified Theories" 16-23 "Microwave background Anisotropies" * March 23-30 "QCD and High Energy Hadronic Interactions" " Rencontre de Biologie -Meribel " Vl I thank the organizers of the XXXIst Rencontres de Moriond : -E. Adelberger, R. Ansari, G. Chardin, T. Damour, 0. Fackler, G. Fontaine, G. Gerbier, Giraud-Heraud, G. Greene , B. Guiderdoni, S. Haroche, E. Hinds, J. Y. Kaplan, J-M. Raimond, B. Sadoulet for the session Dark matter in cosmology, Quantum measurements and Experimental gravitation, -T. Jolicoeur, T. Martin, G. Montambaux, B. Pannetier for the session Correlated fermions and transport in mesoscopic systems -P. Binetruy, A. Blonde!, R. Cahn, G. Coignet, L. Fayard, P. Fayet, J.-M. Frere, H. Frisch, L. Krauss, L. Okun, S. Loucatos, C. Savoy and G. Una! for the Electroweak Interaction session, -M. Bersanelli, F.R. Bouchet, M. Giard, R. Gispert, B. Guiderdoni, J.-M. Lamarre, N. Mandolesi, J.-L. Puget, J. Tauber for the Microwave background Anisotropies session, -E. Auge, P. Aurenche, E. Berger, A. Capella, D. Denegri, B. Klima, L. Kluberg, L. McLerran, L. Montanet, B. Pietrzyck, D. Schiff, and C. Voltolini for the QCD and Hadronic Interaction session, - F. Fabre, M. Fellous, P.-M. Guyon, I. Oliveri and K. Tran Thanh Van for the Biology meeting. and the conference secretaries: G. Ambonati, C. Andrews, N. Bachala, J.M. Ballocchi, C. Barthelemy, L. Besson, R. Bilhaut, C. Cohas-Bogey, Gattignon, D. Larcher, D. Y. Levaillant, H. Mauger, F. N. Osswald,, J. Raguideau, A. M. Renault-Perrin, J. Schmitt and F. Warin. I am also grateful to Mr. E. Rocca-Serra, Ms. C. Dufourny, Ms. S. Kovalevsky who contributed through their hospitality and cooperation to the well-being of the participants enabling them to work in a relaxed atmosphere. These Rencontres were sponsored by the European Union Human Capital and Mobility Programme, the Centre National de la Recherche Scientifique (INSU, SPM and FP), the Institut National de Physique Nucleaire et de Physique des Particules (IN2P3), the Commissariat l'Energie Atomique (DAPNIA, DRECAM), the Ministere a de l'Enseignement Superieur et de la Recherche (programme ACCESS) and the International Science Foundation. I would like to express my thanks for their encouraging support. I sincerely wish that a fruitful exchange and an efficient collaboration between the physicists, the astrophysicists and the biologists will arise from these Rencontres as from the previous ones. Tran Thanh Van J. vii CONTENTS '96 Rencontres de Moriond v I. DARK MATTER Why do we need non baryonic dark matter? A. Olive 3 K. Weak lensing as a probe of dark matter. L. Van Waerbeke 25 Particle dark matter review. G. fungman 33 Phenomenological introduction to direct dark matter detection. P. Gondola 41 Particle dark matter direct detection. L. Mosca 53 Dark matter search with a 24 G sapphire bolometer and neutron background measurements in the underground laboratory of Modane. V. Chazal 65 Status of the CRESST dark matter search. L. Zerle 73 WIMPS search with Te02 thermal detectors : first results of the Milano-Gran Sasso experiment. M. Pavan 77 Search for spin-coupled dark matter by means of large volume scintillators. K. Fushimi 81 New limits to interaction rates from the UK dark matter experiment. T. Ali 85 Indirect detection of supersymmetric dark matter. L. Bergstrom 91 WIMP annihilations in the sun and in the earth. J. Edsjo 101 The NESTOR experiment. Y. Sacquin 105 Status of the projects BAIKAL and AMANDA. C. H. Spiering 109 Can atmospheric Cerenkov telescopes resolve the dark matter problem? E. Pare 117 Indirect detection of WIMPs with cosmic ray positrons and antiprotons : current status and future prospects. G. Tarle 125 HERON as a dark matter detector? R.E.Lanou 131 Dark matter in early-type galaxies. W. Forman 137 SUSY SM and SUSY GUT axions as dark matter. J.L u 143 Recent results from the LEP 1.5 run at CERN. E.L anr;on 149 II. STRUCTURE FORMATION AND COSMOLOGY Observational constraints on Q and H0• f. S. Bag/a 157 Galaxy formation : the linear theory. M.L achieze-Rey 163 The distribution of matter around luminous galaxies. W. H. Zurek 177 Large-scale structure formation in the quasi-linear regime. F. Bernardeau 187 The strongly non-linear regime and N-body simulations. S. Colombi 199 Hydrodynamic simulations of galaxy formation. G. Tormen 207 viii The SLOAN digital sky survey : status and prospects. /.Loveday 215 The DENIS and 2MASS near infrared surveys and their applications in cosmology. G. Mamon 225 The COBRAS/SAMBA space project. N. Mandolesi 233 What can we still learn from the cosmic background radiation? f. Delabrouille 241 Measurement of q0 with Type Ia Supernovae. R. Pain 247 On physically self-consistent basis for large scale structure formation theory. M. Y. Khlopov 255 III. QUANTUM MEASUREMENT A precision test of decoherence. W. H. Zurek 263 Propensities : Measuring quantum states with quantum rulers. P.L . Knight 271 Quantum measurement and regeneration of a single superposition state. Y. Yamamoto 281 A macroscopic mechanical oscillator at the quantum limit level : a practical scheme. F. Ricci 289 New aspects of neutron optics. R. Golub 293 Quantum error correction. A. M. Steane 305 Clock synchronisation with quantum fields. S. Reynaud 309 Motion induced radiation from a vibrating cavity. A. Lambrecht 317 Measurement of the Casimir force in an optical cavity with a resonant transduction scheme. P. Puppo 325 Data security and quantum mechanics. A. Ekert 329 Dissipation and quantum mechanics with trapped ions. f. Cirac 333 I. Quantum computing : dream or nightmare. f. M. Raimond S. Haroche 341 & IV. EXPERIMENTAL GRAVITATION VIRGO -A laser interferometer for the detection of gravitational waves. H. Heitmann 347 UGO project : an overview. A. Lazzarini 355 Laser interferometer space antenna (LISA). Y. fafry 363 Triaxial neutron stars -A possible source of gravitational radiation. f. Frieben 369 Some new concepts for laser interferometer gravitational wave detectors. R.W .P. Drever 375 Theoretical motivations for equivalence principle tests and searches for new long-range forces. P. Fayet 379 Reducing systematic errors in LLR and Viking radar ranging data. K. Nordtvedt 397 A lower bound on neutrino mass? E. Fischbach 405 Prospects for gravitational physics experiments with cryogenic torsion balances. R. D. Newman 409 Search for anomalous coupling of spin to hypothetical non baryonic dark matter in our galaxy. R. Ritter 417 C. ix Precision measurements of small forces. M. Moore 423 W. Plans for a redetermination of G. M. Bantel 429 A rotating torsion balance experiment to measure Newtons constant G. f. H. Gundlach 435 V. SPECIAL LECTURES Ten years of the fifth force. E. Fischbach 443 Desperately seeking the source of ultra high energy cosmic rays. L. M. Celnikier 453 Resumes en Fran�ais 465 List of Participants 475
Description: