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5481por Cini, Michele“…These include: discrete quantum models and lattices (periodic and not), Casimir effect, Anyons, Fano Resonances, the Hanbury Brown and Twiss effect, the Aharonov-Bohm effect, the Meitner-Auger effect, Squeezed Light, the Rabi model, neutrino oscillations, aspects of Quantum Transport, Quantum Pumping, and Berry phases, black holes and cosmological problems.…”
Publicado 2018
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5482“…We find model parameters that give rise to the correct cosmological dark matter density while evading the latest direct detection searches for dark matter scattering produced by the XENON1T experiment, including the effects of Z-Z' mixing. …”
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5483“…Nell’ultimo decennio, questi fenomeni sono diventati strumenti molto efficaci nello studio dell’origine e dell’evoluzione dell’Universo. I cosmologi li utilizzano come "fari" cosmici che illuminano i loro immediati dintorni e anche come sonde per ricostruire la dinamica dell’espansione dell’Universo. …”
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5484por Dippel, Anne“…The first one points towards CERN as place where a cosmological game of probability is played with the help of Monte-Carlo simulations. …”
Publicado 2017
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5485por Baldini, W., Balla, A., Bernhard, J., Calcaterra, A., Cafaro, V., Ceccucci, A., Cicero, V., Ciambrone, P., Danielsson, H., D'Alessandro, G., Felici, G., Gatignon, L., Gerbershagen, A., Giordano, V., Lanfranchi, G., Montanari, A., Paoloni, A., Papalino, G., Rovelli, T., Saputi, A., Schuchmann, S., Stummer, F., Tosi, N.“…SHADOWS can accumulate up to a ~2 x10^19 protons on target per year and expand the exploration for a large variety of FIPs well beyond the state-of-the-art in the mass range of MeV-GeV in a parameter space that is allowed by cosmological and astrophysical observations. So far the strongest bounds on the interaction strength of new feebly-interacting light particles with Standard Model particles exist up to the kaon mass; above this threshold the bounds weaken significantly. …”
Publicado 2021
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5486por Baldini, W, Balla, A, Bernhard, J, Calcaterra, A, Cafaro, V, Charitonidis, N, Ceccucci, A, Cicero, V, Ciambrone, P, Danielsson, H, De Roeck, A, Duval, F, D’Alessandro, G, Felici, G, Foggetta, L, Gatignon, L, Gerbershagen, A, Giordano, V, Lanfranchi, G, Lax, I, Montanari, A, Murphy, R, Paoloni, A, Papalino, G, Rovelli, T, Saputi, A, Schuchmann, S, Stummer, F, Torromeo, G, Tosi, N, Vannozzi, A“…SHADOWS can accumulate up to a $\sim (1-2) \cdot 10^{19}$ protons on target per year and expand the exploration for a large variety of FIPs well beyond the state-of-the-art in the mass range of MeV-GeV in a parameter space that is allowed by cosmological and astrophysical observations. So far the strongest bounds on the interaction strength of new feebly-interacting light particles with Standard Model particles exist up to the kaon mass; above this threshold the bounds weaken significantly. …”
Publicado 2022
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5487por Marsicano, Luca“…Despite the various astrophysical and cosmological observations proving its existence, its elementary properties remain to date unknown. …”
Publicado 2022
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5488“…In combination with related ideas and general constraints in S-theory, we are led to a cosmological scenario in which, after a phase transition, the extra timelike dimension becomes part of the compactified universe residing inside microscopic matter. …”
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5489por Totani, T“…This suggests a possibility that GRBs are most energetic in TeV range and such TeV gamma-rays may be detectable from GRBs even at cosmological distances, i.e., z gives a quantitative explanation for the famous long-duration GeV photons detected from GRB940217. …”
Publicado 1998
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5490“…Finally, we show that under certain circumstances, the presence of an infinite tower of Kaluza-Klein axion modes can significantly accelerate the dissipation of the energy associated with cosmological relic axion oscillations, thereby enabling the Peccei-Quinn symmetry-breaking scale to exceed the usual four-dimensional relic oscillation bounds. …”
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5491“…We then combinethis cosmological constraint with neutralino production with light sfermions tofurther reduce the parameter space that precludes observability of the Higgs atthe LHC. …”
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5492ESSnuSB: a Project for Leptonic CP Violation Discovery based on the European Spallation Source Linacpor Wildner, E“…The detector would also be used to measure the proton lifetime, detect cosmological neutrinos and neutrinos from supernova explosions. …”
Publicado 2015
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5493por Di Mascolo, Luca, Saro, Alexandro, Mroczkowski, Tony, Borgani, Stefano, Churazov, Eugene, Rasia, Elena, Tozzi, Paolo, Dannerbauer, Helmut, Basu, Kaustuv, Carilli, Christopher L., Ginolfi, Michele, Miley, George, Nonino, Mario, Pannella, Maurilio, Pentericci, Laura, Rizzo, Francesca“…In fact, the SZ signal reveals the ICM thermal energy in a way that is insensitive to cosmological dimming, making it ideal for tracing the thermal history of cosmic structures(3). …”
Publicado 2023
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5494por Anderson, E. K., Baker, C. J., Bertsche, W., Bhatt, N. M., Bonomi, G., Capra, A., Carli, I., Cesar, C. L., Charlton, M., Christensen, A., Collister, R., Cridland Mathad, A., Duque Quiceno, D., Eriksson, S., Evans, A., Evetts, N., Fabbri, S., Fajans, J., Ferwerda, A., Friesen, T., Fujiwara, M. C., Gill, D. R., Golino, L. M., Gomes Gonçalves, M. B., Grandemange, P., Granum, P., Hangst, J. S., Hayden, M. E., Hodgkinson, D., Hunter, E. D., Isaac, C. A., Jimenez, A. J. U., Johnson, M. A., Jones, J. M., Jones, S. A., Jonsell, S., Khramov, A., Madsen, N., Martin, L., Massacret, N., Maxwell, D., McKenna, J. T. K., Menary, S., Momose, T., Mostamand, M., Mullan, P. S., Nauta, J., Olchanski, K., Oliveira, A. N., Peszka, J., Powell, A., Rasmussen, C. Ø., Robicheaux, F., Sacramento, R. L., Sameed, M., Sarid, E., Schoonwater, J., Silveira, D. M., Singh, J., Smith, G., So, C., Stracka, S., Stutter, G., Tharp, T. D., Thompson, K. A., Thompson, R. I., Thorpe-Woods, E., Torkzaban, C., Urioni, M., Woosaree, P., Wurtele, J. S.“…The theoretical consensus is that any laboratory mass must be attracted(6) by the Earth, although some authors have considered the cosmological consequences if antimatter should be repelled by matter(7–10). …”
Publicado 2023
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5495“…We then show that many of these puzzling observations are predicted by one single relation — Milgrom’s law — involving an acceleration constant a(0) (or a characteristic surface density Σ(†) = a(0)/G) on the order of the square-root of the cosmological constant in natural units. This relation can at present most easily be interpreted as the effect of a single universal force law resulting from a modification of Newtonian dynamics (MOND) on galactic scales. …”
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5496“…In this context, the f(R) setting to the consensus cosmological model, the [Formula: see text] CDM model, can be written as a polynomial including just a constant and a third-order term. …”
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5497“…The theoretical framework is provided by the theory of manifestly covariant quantum gravity and the related prediction of an exclusively quantum-produced stochastic cosmological constant. The specific example case of the Schwarzschild–deSitter geometry is looked at, analyzing the consequent stochastic modifications of the Einstein field equations. …”
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5498“…However, the IPCC has faced criticism for its different organizational and functional biases which include a geographical bias favoring experts from the global north, a gender bias in favor of men, a disciplinary bias in favor of the natural sciences over the social sciences and humanities, and finally, a cosmological bias favoring western science over indigenous knowledges. …”
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5499por Westoby, Ross, Clissold, Rachel, McNamara, Karen E., Latai-Niusulu, Anita, Chandra, Alvin“…According to participants, Pacific Islander worldviews, knowledge systems and cosmologies often make it difficult to separate and evaluate NELD independently, challenging the nomenclature of NELD categories developed through international mechanisms. …”
Publicado 2021
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5500por Volovik, G. E.“…Finally, we considered the application of the gravitational tetrads for the solution of the cosmological constant problem.…”
Publicado 2021
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