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1801por Barbagallo, M, Aberle, O, Alcayne, V, Andrzejewski, J, Audouin, L, Bécares, V, Babiano-Suarez, V, Bacak, M, Benedikt, Th, Bennett, S, Berthoumieux, E, Billowes, J, Bosnar, D, Brown, A, Busso, M, Caamaño, M, Caballero-Ontanaya, L, Calviño, F, Calviani, M, Cano-Ott, D, Casanovas, A, Cerutti, F, Chiaveri, E, Colonna, N, Cortes, G, Cortés-Giraldo, M A, Consentino, L, Cristallo, S, Damone, L A, Davies, P J, Dietz, M, Domingo-Pardo, C, Dressler, R, Ducasse, Q, Dupont, E, Duran, I, Eleme, Z, Fernández-Domínguez, B, Ferrari, A, Finocchiaro, P, Furman,V, Göbel, K, Gawlik, A, Gilardoni, S, Gonçalves, I F, González-Romero, E, Guerrero, C, Gunsing, F, Heinitz, S, Heyse, J, Jenkins, D G, Junghans, A, Käppeler, F, Kadi, Y, Kimura, A, Knapova, I, Kokkoris, M, Kopatch, Y, Krtička, M, Kurtulgil, D, Ladarescu, I, Lederer-Woods, C, Lonsdale, S J, Macina, D, Manna, A, Martínez, T, Masi, A, Massimi, C, Mastinu, P, Mastromarco, M, Maugeri, E A, Mazzone, A, Mendoza, E, Mengoni, A, Michalopoulou, V, Milazzo, P M, Mingrone, F, Moreno-Soto, J, Musumarra, A, Negret, A, Ogállar, F, Oprea, A, Patronis, N, Pavlik, A, Perkowski, J, Persanti, L, Petrone, C, Pirovano, E, Porras, I, Praena, J, Quesada, J M, Ramos-Doval, D, Rauscher, T, Reifarth, R, Rochman, D, Sabaté-Gilarte, M, Saxena, A, Shillebeeckx, P, Schumann, D, Sekhar, A, Smith, A G, Sosnin, N V, Sprung, P, Stamatopoulos, A, Tagliente, G, Tain, J L, Tarifeño-Saldivia, A, Tassan-Got, L, Tsinganis, A, Ulrich, J, Urlass, S, Valenta, S, Vannini, G, Variale, V, Vaz, P, Ventura, A, Vescovi, D, Vlachoudis, V, Vlastou, R, Wallner,A, Woods, P J, Wright, T, Žugec, P, the n_TOF Collaboration“…This discrepancy has been referred since several decades as Cosmological Lithium Problem. In one last attempt to find nuclear solutions to this longstanding conundrum, the $^{7}$Be(n,α)$^{4}$He and $^7}$Be(n,p)$^{7}$Li reactions, that affect predominantly the production of 7Li via the destruction of his parent nucleus 7Be, have been studied. …”
Publicado 2019
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1802por UEDA, Yoshihiro“…We review the current understanding of the cosmological evolution of supermassive black holes in galactic centers elucidated by X-ray surveys of active galactic nuclei (AGNs). …”
Publicado 2015
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1803Measuring the 2D baryon acoustic oscillation signal of galaxies in WiggleZ: cosmological constraintspor Hinton, Samuel R., Kazin, Eyal, Davis, Tamara M., Blake, Chris, Brough, Sarah, Colless, Matthew, Couch, Warrick J., Drinkwater, Michael J., Glazebrook, Karl, Jurek, Russell J., Parkinson, David, Pimbblet, Kevin A., Poole, Gregory B., Pracy, Michael, Woods, David“…Within these bins and methodologies, we recover constraints between 5 and 22 per cent error. Our cosmological constraints are consistent with flat ΛCDM cosmology and agree with results from the Baryon Oscillation Spectroscopic Survey.…”
Publicado 2016
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1804“…In this paper, we have studied Bianchi type-I string cosmological model by combining Kaluza-Klein (KK) theory and [Formula: see text] theory of gravity which is an extension of 5-dimensional KK string cosmological models. …”
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1809por Palanque-Delabrouille, Nathalie, Yèche, Christophe, Lesgourgues, Julien, Rossi, Graziano, Borde, Arnaud, Viel, Matteo, Aubourg, Eric, Kirkby, David, LeGoff, Jean-Marc, Rich, James, Roe, Natalie, Ross, Nicholas P., Schneider, Donald P., Weinberg, David“…We present constraints on the parameters of the $\Lambda$CDM cosmological model in the presence of massive neutrinos, using the one-dimensional Ly$\alpha$ forest power spectrum obtained with the Baryon Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky Survey (SDSS) by Palanque-Delabrouille et al. (2013), complemented by additional cosmological probes. …”
Publicado 2014
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1810por Ellis, John, Garcia, Marcos A.G., Nagata, Natsumi, Nanopoulos, Dimitri V., Olive, Keith A.“…We propose a complete cosmological scenario based on a flipped SU(5)×U(1) GUT model that incorporates Starobinsky-like inflation, taking the subsequent cosmological evolution carefully into account. …”
Publicado 2019
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1813“…We study two possible cosmological consequences of a first-order phase transition in the temperature range of $1$ GeV to $10^3$ TeV: the generation of a stochastic gravitational wave background (SGWB) within the sensitivity of the Laser Interferometer Space Antenna (LISA) and, simultaneously, primordial magnetic fields that would evolve through the Universe's history and could be compatible with the lower bound from $\gamma$-ray telescopes on intergalactic magnetic fields (IGMF) at present time. …”
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