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4461por Esposito, Giampiero“…In the second part, a number of relevant physical applications are studied: non-local boundary conditions for massless spin-1/2 fields, massless spin-3/2 potentials on manifolds with boundary, geometric theory of massive spin-3/2 potentials, local boundary conditions in quantum supergravity, quark boundary conditions, one-loop quantum cosmology, conformally covariant operators and Euclidean quantum gravity.…”
Publicado 1998
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4462“…We find that the branching ratio for decay of the heavier neutralino chi_2 to chi + tau mu is enhanced when the LSP mass m_chi = m_stau_1, including the region of CMSSM parameter space where coannihilation keeps the relic chi density within the range preferred by cosmology. Thus chi_2 to chi + tau mu decay may provide a physics opportunity for observing the violation of tau lepton number at the LHC that is complementary to tau to mu + gamma decay. …”
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4463por Sikivie, P“…Constraints from laboratory searches, astrophysics and cosmology require the axion mass to be in the range $10^{-6} \lesssim m_a < 3\cdot 10^{-3}$eV. …”
Publicado 2002
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4464por Goswami, S, Rangarajan, R, Agashe, K, Bandyopadhyay, A, Bhattacharya, K K, Brahmachari, B, Burgess, C, Chun, E J, Choudhury, D, Das-Prasanta, Kumar, Dighe, Amol S, Godbole, Rohini M, Gupta, N, Kaplinghat, M, Indumathi, D, Forshaw, J, Keum, Yu Y, Layek, B, Majumdar, D, Mahajan, N, Mehta, P, Mohapatra, Rabindra N, Mondal, N K, More, S, Nir, Y, Pakvasa, S, Parida, M K, Ravikumar, M, Rajasekaran, G, Ramadevi, P, Rindani, S D, Roy, D P, Roy, P, Sahu, N, Samanta, A, Shadmi, Y, Srivastava, A M, Sankar, S U, Vaidya, R, Yajnik, U“…The astroparticle physics subgroup focused on how various particle physics inputs affect the CMBR fluctuation spectrum, and on brane cosmology. This report also contains an introduction on how to use the publicly available code CMBFAST to calculate the CMBR fluctuations.…”
Publicado 2004
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4465“…Studies have shown however that rather large Dark Matter-photon or Dark Matter-baryon interactions could be allowed by cosmology. Here we address the question of the role of the Dark Matter interactions in more detail to determine at which extent Dark Matter has to be necessarily weakly interacting. …”
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4466por Longair, Malcolm“…The gravitational bending of electromagnetic waves by massive bodies is a subject of the greatest importance for contemporary and future astronomy, astrophysics and cosmology. Examples of the potential impact of this key tool of modern observational astronomy are presented. …”
Publicado 2015
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4467“…The ‘standard’ model of cosmology is founded on the basis that the expansion rate of the universe is accelerating at present — as was inferred originally from the Hubble diagram of Type Ia supernovae. …”
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4468“…Detectors of microwave photons find applications in different fields ranging from security to cosmology. Due to the intrinsic difficulties related to the detection of vanishingly small energy quanta [Formula: see text] , significant portions of the microwave electromagnetic spectrum are still uncovered by suitable techniques. …”
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4469“…Theoretical implications for cosmology and field theories are pointed out.…”
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4470por Bormashenko, Edward“…The fundamental role of the temperature of the cosmic microwave background in modern cosmology is discussed. The range of problems and controversies related to the negative absolute temperature is treated.…”
Publicado 2020
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4471“…Professor Henry Tye (戴自海) is a world-renowned expert in theoretical particle physics, string theory and cosmology. He was recently the IAS Professor at the Jockey Club Institute for Advanced Study (IAS) and the Hong Kong University of Science and Technology (HKUST), and is the Horace White Professor of Physics (Emeritus) at Cornell University. …”
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4472por Patrignani, C, Agashe, K, Aielli, G, Amsler, C, Antonelli, M, Asner, D M, Baer, H, Banerjee, Sw, Barnett, R M, Basaglia, T, Bauer, C W, Beatty, J J, Belousov, V I, Beringer, J, Bethke, S, Bichsel, H, Biebel, O, Blucher, E, Brooijmans, G, Buchmueller, O, Burkert, V, Bychkov, M A, Cahn, R N, Carena, M, Ceccucci, A, Cerri, A, Chakraborty, D, Chen, M -C, Chivukula, R S, Copic, K, Cowan, G, Dahl, O, D'Ambrosio, G, Damour, T, de Florian, D, de Gouvea, A, DeGrand, T, de Jong, P, Dissertori, G, Dobrescu, B A, D'Onofrio, M, Doser, M, Drees, M, Dreiner, H K, Dwyer, D A, Eerola, P, Eidelman, S, Ellis, J, Erler, J, Ezhela, V V, Fetscher, W, Fields, B D, Foster, B, Freitas, A, Gallagher, H, Garren, L, Gerber, H -J, Gerbier, G, Gershon, T, Gherghetta, T, Godizov, A A, Goodman, M, Grab, C, Gritsan, A V, Grojean, C, Groom, D E, Grünewald, M, Gurtu, A, Gutsche, T, Haber, H E, Hagiwara, K, Hanhart, C, Hashimoto, S, Hayato, Y, Hayes, K G, Hebecker, A, Heltsley, B, Hernández-Rey, J J, Hikasa, K, Hisano, J, Höcker, A, Holder, J, Holtkamp, A, Huston, J, Hyodo, T, Irwin, K, Jackson, J D, Johnson, K F, Kado, M, Karliner, M, Katz, U F, Klein, S R, Klempt, E, Kowalewski, R V, Krauss, F, Kreps, M, Krusche, B, Kuyanov, Yu V, Kwon, Y, Lahav, O, Laiho, J, Langacker, P, Liddle, A, Ligeti, Z, Lin, C -J, Lippmann, C, Liss, T M, Littenberg, L, Lugovsky, K S, Lugovsky, S B, Lusiani, A, Makida, Y, Maltoni, F, Mannel, T, Manohar, A V, Marciano, W J, Martin, A D, Masoni, A, Matthews, J, Meißner, U -G, Milstead, D, Mitchell, R E, Molaro, P, Mönig, K, Moortgat, F, Mortonson, M J, Murayama, H, Nakamura, K, Narain, M, Nason, P, Navas, S, Neubert, M, Nevski, P, Nir, Y, Olive, K A, Pagan Griso, S, Parsons, J, Peacock, J A, Pennington, M, Petcov, S T, Petrov, V A, Piepke, A, Pomarol, A, Quadt, A, Raby, S, Rademacker, J, Raffelt, G, Ratcliff, B N, Richardson, P, Ringwald, A, Roesler, S, Rolli, S, Romaniouk, A, Rosenberg, L J, Rosner, J L, Rybka, G, Ryutin, R A, Sachrajda, C T, Sakai, Y, Salam, G P, Sarkar, S, Sauli, F, Schneider, O, Scholberg, K, Schwartz, A J, Scott, D, Sharma, V, Sharpe, S R, Shutt, T, Silari, M, Sjöstrand, T, Skands, P, Skwarnicki, T, Smith, J G, Smoot, G F, Spanier, S, Spieler, H, Spiering, C, Stahl, A, Stone, S L, Sumino, Y, Sumiyoshi, T, Syphers, M J, Takahashi, F, Tanabashi, M, Terashi, K, Terning, J, Thorne, R S, Tiator, L, Titov, M, Tkachenko, N P, Törnqvist, N A, Tovey, D, Valencia, G, van de Water, R, Varelas, N, Venanzoni, G, Vincter, M G, Vogel, P, Vogt, A, Wakely, S P, Walkowiak, W, Walter, C W, Wands, D, Ward, D R, Wascko, M O, Weiglein, G, Weinberg, D H, Weinberg, E J, White, M, Wiencke, L R, Willocq, S, Wohl, C G, Wolfenstein, L, Womersley, J, Woody, C L, Workman, R L, Yao, W -M, Zeller, G P, Zenin, O V, Zhu, R -Y, Zimmermann, F, Zyla, P A“…The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,062 new measurements from 721 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. …”
Publicado 2016
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4473“…We model the space-time foam as a gas of D-particles in the bulk space-time of a higher-dimensional cosmology where the observable Universe is a D3-brane. …”
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4474“…A section on neutrino oscillations and one on nuclear matter at high temperatures bridge the field of "nuclear and particle physics" and "modern astrophysics and cosmology". The new edition incorporates a large amount of new experimental results on deep inelastic scattering (obtained at the Electron-Proton Collider HERA at DESY in Hamburg) into chapters 7 and 8. …”
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4475por Hamber, Herbert W“…The book ends with a discussion of contemporary issues in quantum cosmology such as scale dependent gravitational constants and quantum effects in the early universe.…”
Publicado 2009
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4476por Cremonesi, Oliviero“…Complementary measurements to assess the absolute neutrino mass scale (cosmology and single beta decays) are also discussed.…”
Publicado 2010
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4477“…This type of behavior is in principle perturbative in the string coupling, persists after compactification, could have trapped scalar fields inside potential wells as a result of the cosmological evolution and could have also injected the inflationary phase of our Universe.…”
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4478“…A section on neutrino oscillations and one on nuclear matter at high temperatures bridge the field of "nuclear and particle physics" and "modern astrophysics and cosmology". New developments are covered, e. g. in sections on the double beta decay including a discussion of the possibility for a neutrinoless decay and its implications for the standard model. …”
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4479por Shaviv, Giora“…Beginning with generally accepted science, the book ends in today’s terra incognita of nuclear physics, astrophysics and cosmology. A monumental work that will fascinate scientists, philosophers, historians and lay readers alike.…”
Publicado 2012
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4480Publicado 2014“…The topics of the conference will include: Cosmic Rays Dark Matter in Cosmology Direct Dark Matter Searches Indirect Dark Matter Searches High Energy Particle Physics Neutrinos High Energy Astrophysics The conference will be held at the Tuschinski Theatre, an extraordinary landmark built in 1921 in the heart of Amsterdam in a spectacular mix of Amsterdam School, Jugendstil, Art Nouveau and Art Deco. …”
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