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Nikolai Tyurin (Institute for High Energy Physics (RU))26/06/2013, 09:30
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Rosy Nikolaidou (CEA/IRFU,Centre d'etude de Saclay Gif-sur-Yvette (FR))26/06/2013, 09:40Higgs boson
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Gregorio bernardi (LPNHE University of Paris 6 & 7)26/06/2013, 10:10Higgs boson
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Francesco Riva (Ecole Polytechnique Federale de Lausanne (CH))26/06/2013, 11:00Higgs boson
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Boris ARBUZOV (SINP MSU, Moscow)26/06/2013, 11:30Higgs boson
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Alexander KNOCHEL (ITTK RWTH, Aachen, Germany)26/06/2013, 12:00Higgs boson
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Valery Kiselev (IHEP, Protvino, Russia)26/06/2013, 12:30Higgs bosonModerator: V. Kiselev Panelists: B. Arbuzov A. Knochel R. Nikolaidou G. Bernardi F. Riva Questions: • If the SM with elementary Higgs field is completely confirmed with the discovery of a heavy scalar boson at LHC and Tevatron? • Does the Higgs mass value of 126 GeV point to the need of new physics below the Planck scale? • Do we need the next Higgs factory to solve...Go to contribution page
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Sonja Kabana (Laboratoire de Physique Subatomique et des Technologies Associe)26/06/2013, 14:15Structure of fundamental particles
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Olga Evdokimov (Physics Department-University of Illinois at Chicago)26/06/2013, 14:45Structure of fundamental particles
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Ekaterina POZDEEVA (SINP MSU, Moscow)26/06/2013, 15:15Black holesIn holographic approach the Quark Gluon Plasma (QGP) formation in 4D space is related with Black Hole (BH) creation in 5D Anti de Sitter space (AdS) and multiplicity in heavy-ion collisions is determined by entropy of 5D BH. Using the general relativity technique the entropy of formed BH can be estimate by the trapped surface area. We simulate energy dependence of entropy considering ...Go to contribution page
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Valentin ZAKHAROV (ITEP, Moscow)26/06/2013, 15:30Structure of fundamental particles
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Bernardo Adeva (Universidade de Santiago de Compostela (ES))26/06/2013, 16:20What did we learn from the LHC?
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Cristina Ferro (National Central University (TW))26/06/2013, 16:50What did we learn from the LHC?
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Fedor Ratnikov (KIT - Karlsruhe Institute of Technology (DE))26/06/2013, 17:20What did we learn from the LHC?
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Khristian Kotov (Ohio State University (US))26/06/2013, 17:50What did we learn from the LHC?
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Valentin Zakharov (ITEP, Moscow, Russia)26/06/2013, 18:20Structure of fundamental particlesModerator: V. Zakharov Panelists: S. Kabana O. Evdokimov K. Kotov S. Troshin S. Sadovsky Questions: • In which case experiment could unambiguously (dis)prove the existence of Quark-Gluon Plasma? • If the investigations of HI collisions can clarify the confinement problem? • Is there time enough for establishing the local thermodynamic equilibrium in the course of the HI...Go to contribution page
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Mr Andrey Sheshukov (JINR)27/06/2013, 09:30Neutrino in labs & cosmosThis talk is focused on a general description of the OPERA experiment, which is designed to observe directly the appearance of nu-tau produced by neutrino oscillations in an almost pure nu_mu beam. The neutrino beam is produced at CERN and detected 730 km away in an underground hall of the National Laboratory of Gran Sasso. OPERA detector is a hybrid structure, containing nuclear emulsion...Go to contribution page
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Timur Dzhatdoev (PNPI MSU, Moscow, Russia)27/06/2013, 09:55The present talk highlights the data analysis status of the OPERA experiment. The experiment exploited the CNGS beam from CERN to Gran Sasso, at the average L/E ratio of 43 km/GeV, optimized to search for ν_μ→ν_τ oscillation in appearance mode, and also allowing to perform a ν_e appearance search. Profiting of the sub-micrometer spatial resolution of nuclear emulsions, employed in the OPERA...Go to contribution page
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Michael Smy (UCI)27/06/2013, 10:15Neutrino in labs & cosmos
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Nikita Titov (INR RAS, Moscow)27/06/2013, 11:10KATRIN project has a goal to set electron antineutrino mass upper limit at 0.2 eV level. Installation construction at Karlsruhe Institute of Technology (KIT) proceeds to it final stage. Inner electrodes are installed inside the main spectrometer and first background tests are launched. Windowless gaseous tritium source (WGTS) temperature stabilization was proven to provide 20 mK temperature...Go to contribution page
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Alexey Lubashevskiy (MPIK)27/06/2013, 11:30Neutrino in labs & cosmosThe study of neutrinoless double beta decay ($0\nu\beta\beta$) is a powerful approach to investigate fundamental properties of neutrinos. The observation of $0\nu\beta\beta$ would demonstrate lepton number violation in nature and prove that neutrinos have a Majorana component. It will also give an access to the neutrino mass hierarchy and to the information on the absolute values of the...Go to contribution page
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Dr Marat Khabibullin (INR RAS, Troitsk), Prof. Yury Kudenko (Russian Academy of Sciences (RU))27/06/2013, 11:55Neutrino in labs & cosmos
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Vladimir Obraztsov (Institute for High Energy Physics (RU))27/06/2013, 12:35Neutrino in labs & cosmosModerator: V. Obraztsov Panelists: M. Smy M. Khabibullin N. Titov S. Gershtein Questions: • How well do we need to know the standard neutrino sector parameters? • Neutrino and the lepton/baryon asymmetry in the Universe. • Are there new species of neutrino (e.g. the "sterile"one)? • What are the most important problems of neutrino physics? • Perspectives of...Go to contribution page
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Oleg Zenin (Institute for High Energy Physics (RU))27/06/2013, 14:40What did we learn from the LHC?
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Alexander Bylinkin (ITEP)27/06/2013, 15:10Structure of fundamental particles
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Damian PSZCZEL (NCNR, Warsaw, Poland; Uppsala University)27/06/2013, 15:30Structure of fundamental particles
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Prof. Anatoly Petrukhin (MEPhI, Moscow)27/06/2013, 15:50The discovery of Higgs boson completed the first (and main) stage of experiments on p-p-interactions at LHC. Attempts to search new physics effects in these experiments did not give positive results. At that time, many interesting and not described by modern theories and models phenomena were observed in cosmic ray experiments in the energy region 1015 – 1017 eV, which corresponds to the LHC...Go to contribution page
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Vladimir Petrov (Institute for High Energy Physics (RU))27/06/2013, 16:30Structure of fundamental particles
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Alexander Bazilevsky (B)27/06/2013, 17:00Structure of fundamental particles
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Alexey PROKUDIN (JLAB, Newport News, USA)27/06/2013, 17:30Structure of fundamental particles
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Alexey Prokudin (JLAB, Newport News)27/06/2013, 18:00Structure of fundamental particlesModerator: A. Prokudin Panelists: O. Zenin B. Adeva C. Ferro A. Likhoded Questions: Panel Discussion IV. • Does QCD help us to understand strong interactions? • Does the SM theory with Kobayashi-Maskawa (CKM) quark-mixing matrix describe all CP-violation and rare decays phenomena observed in the heavy quark sector? • Can quantum loop corrections reveal new physics mass...Go to contribution page
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TRIO ELEGIA27/06/2013, 19:00
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Prof. Anatoly CHEREPASHCHUK (SAI MSU, Moscow)28/06/2013, 09:30Black holes
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Alexander ZAKHAROV (ITEP, Moscow)28/06/2013, 10:00Black holes
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Mikhail Katanaev (Steklov Mathematical Institute, Moscow)28/06/2013, 10:30Black holesIt is well known that the Schwarzschild solution describes the gravitational field outside compact spherically symmetric mass distribution in General Relativity. In particular, it describes the gravitational field outside a point particle. Nevertheless, what is the exact solution of Einstein's equations with \delta-type source corresponding to a point particle is not known. In the...Go to contribution page
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Abhas MITRA (BARC, Mumbai, India)28/06/2013, 11:15Black holesEven if one would assume existence of Black Holes (BHs), High Energy Astrophysics observations cannot be explained because no free charge, no current can emerge from central singularities. In other words, even supposed charged BHs cannot have any electromagnetic property. In fact gravitational effects too should not propagate out of Event Horizons! Several authors try to resolve the BH...Go to contribution page
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Stephen CROTHERS (AIAS, USA)28/06/2013, 11:45Black holesAll alleged black hole solutions pertain to a universe that is spatially infinite, is eternal, contains only one mass, is not expanding, and is asymptotically flat. But the alleged big bang cosmology pertains to a universe that is spatially finite, is of finite age, contains radiation and many masses including multiple black holes (some of which are primordial), is expanding, and is not...Go to contribution page
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Skiff Sokolov (IHEP, Protvino, Russia)28/06/2013, 12:15Black holesModerator: S. Sokolov Panelists: A. Cherepashchuk A. Mitra S. Crothers A. Zakharov Questions: • Is there a definitive observational/experimental proof of the existence of black holes? • Are there theoretical problems with black holes? • Are any understanding of mass gap between the supermassive black holes in centers of spiral galaxies and star-range black holes ascribed...Go to contribution page
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Edward ANDERSON (APC, Paris/Cambridge Univ., DAMTP, UK)28/06/2013, 14:30Dark matter & dark energy
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Abhas Mitra (BARC, Mumbai, India)28/06/2013, 15:00Dark matter & dark energyNewtonian Cosmology was apparently plagued with the problem of infinite gravitational force, and Einstein’s General Relativity apparently ushered in the revolutionary concept of a closed finite non-singular static universe. Later, Big Bang model (BBM) essentially incorporated non-static versions of similar relativistic model. Simultaneously the concept of a Cosmological Constant or a repulsive...Go to contribution page
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Vladimir Sokolov (SAO RAS, Nizhnij Arkhyz, Russia)28/06/2013, 15:30Dark matter & dark energyThe brief review and discussion of statement of some observational problems of gamma-ray bursts (GRB), GRB host galaxies and star forming at small and large redshifts: Are there similarities and differences between GRB hosts and the typical galaxy population - this is currently the main question for the study of GRB host galaxies. The direct connection between long-duration GRBs and...Go to contribution page
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Alexander Dolgov28/06/2013, 16:20Dark matter & dark energy
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Prof. Valery RUBAKOV (INR RAS, Moscow)28/06/2013, 16:50Dark matter & dark energy
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Edward Anderson (Cambridge Univ., DAMTP, UK)28/06/2013, 17:20Dark matter & dark energyModerator: E. Anderson Panelists: A. Mitra V. Rubakov A. Dolgov S. Crothers A. Zakharov Questions: Discussion VI. • To what extent Dark Matter and Dark Energy are necessary to explain the observed properties of the Universe? • Why the Dark matter profiles so universal at the galactic scales? • Are there viable candidates of modified gravitational dynamics to exclude the...Go to contribution page
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Vladimir Petrov (Institute for High Energy Physics (RU))28/06/2013, 18:20
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