Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
-
321por Lederer, C., Massimi, C., Altstadt, S., Andrzejewski, J., Audouin, L., Barbagallo, M., Bécares, V., Bečvář, F., Belloni, F., Berthoumieux, E., Billowes, J., Boccone, V., Bosnar, D., Brugger, M., Calviani, M., Calviño, F., Cano-Ott, D., Carrapiço, C., Cerutti, F., Chiaveri, E., Chin, M., Colonna, N., Cortés, G., Cortés-Giraldo, M.A., Diakaki, M., Domingo-Pardo, C., Duran, I., Dressler, R., Dzysiuk, N., Eleftheriadis, C., Ferrari, A., Fraval, K., Ganesan, S., García, A.R., Giubrone, G., Gómez-Hornillos, M.B., Gonçalves, I.F., González-Romero, E., Griesmayer, E., Guerrero, C., Gunsing, F., Gurusamy, P., Jenkins, D.G., Jericha, E., Kadi, Y., Käppeler, F., Karadimos, D., Kivel, N., Koehler, P., Kokkoris, M., Korschinek, G., Krtička, M., Kroll, J., Langer, C., Leeb, H., Leong, L.S., Losito, R., Manousos, A., Marganiec, J., Martínez, T., Mastinu, P.F., Mastromarco, M., Meaze, M., Mendoza, E., Mengoni, A., Milazzo, P.M., Mingrone, F., Mirea, M., Mondelaers, W., Paradela, C., Pavlik, A., Perkowski, J., Pignatari, M., Plompen, A., Praena, J., Quesada, J.M., Rauscher, T., Reifarth, R., Riego, A., Roman, F., Rubbia, C., Sarmento, R., Schillebeeckx, P., Schmidt, S., Schumann, D., Tagliente, G., Tain, J.L., Tarrío, D., Tassan-Got, L., Tsinganis, A., Valenta, S., Vannini, G., Variale, V., Vaz, P., Ventura, A., Versaci, R., Vermeulen, M.J., Vlachoudis, V., Vlastou, R., Wallner, A., Ware, T., Weigand, M., Weiß, C., Wright, T.J., Žugec, P.“…Stellar model calculations for a 25 M$_\odot$ star show that the new data have a significant effect on the $s$-process production of $^{63}$Cu, $^{64}$Ni, and $^{64}$Zn in massive stars, allowing stronger constraints on the Cu yields from explosive nucleosynthesis in the subsequent supernova.…”
Publicado 2013
Enlace del recurso
Enlace del recurso
-
322por Volpe, Cristina“…We discuss that the availability of neutrino beams in the 100 MeV energy range offers a unique opportunity to perform neutrino scattering experiments of interest for nuclear physics, for the study of fundamental interactions and of core-collapse supernova physics.…”
Publicado 2009
Enlace del recurso
Enlace del recurso
-
323“…Neutrinos play an important role in supernova nucleosynthesis. To obtain more information about these processes, cross sections are folded with a Fermi-Dirac distribution with temperatures of approximately 10 9 K.…”
Enlace del recurso
-
324por Bettini, A“…The physics program at the Gran Sasso Laboratory that we are defining will be focussed on the next phase of neutrino physics with a complementary set of experiments on the muon-neutrino beam from CERN (CNGS project), on solar neutrinos, on atmospheric neutrinos and on neutrinos from supernova explosion. The relevant thermonuclear cross-sections will be measured. …”
Publicado 2001
Enlace del recurso
Enlace del recurso
-
325“…We conduct a comprehensive study of the detectability of primordial black holes with non-negligible spin, via the searches for the neutrinos and positrons in the MeV energy range. Diffuse supernova neutrino background searches and observation of the 511 keV gamma-ray line from positrons in the Galactic center set competitive constraints. …”
Enlace del recurso
Enlace del recurso
-
326por Martin Camalich, Jorge, Pospelov, Maxim, Vuong, Pham Ngoc Hoa, Ziegler, Robert, Zupan, Jure“…For instance, a strong limit on the Λ→na transition can be derived from the supernova SN 1987A. In the near future, dedicated searches for q→q′a decays at ongoing experiments could potentially test Peccei-Quinn breaking scales up to 1012 GeV at NA62 or KOTO and up to 109 GeV at Belle II or BES III.…”
Publicado 2020
Enlace del recurso
Enlace del recurso
-
327“…Recent observations suggest that gamma-ray bursts (GRBs) and their afterglows are produced by jets of highly relativistic cannonballs (CBs), emitted in supernova explosions. The fully ionized CBs cool to a temperature below 4500 K within a day or two, at which point electron-proton recombination produces an intense Lyman-$\alpha$ emission. …”
Enlace del recurso
-
328“…Phosphorus is thought to be created by neutron capture on (29)Si and (30)Si in massive stars(20,21), and released into the interstellar medium by Type II supernova explosions(2,22). However, models of galactic chemical evolution must arbitrarily increase the supernovae production(23) to match observed abundances. …”
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
329“…Fundamental astrophysical phenomena, such as charged particle acceleration and magnetic field generation, are presented along with spectacular phenomena, such as stellar winds (including ultra-relativistic pulsar wind), supernova explosions and evolution of its remnants, and solar flares.…”
Enlace del recurso
Enlace del recurso
-
330“…Neutrinos play an important role in supernova nucleosynthesis. To obtain more information about these processes, cross sections are folded with a Fermi-Dirac distribution with temperatures of approximately 10$^9$ K.…”
Enlace del recurso
Enlace del recurso
-
331“…Astrophysical data on the Supernova luminosity-distance - redshift relations, recalculated in terms of relative measurement standards, is utilized as a justification of conformal-invariant unified theory, where all masses, including masses of the Planck and Higgs, become the present- day values of dynamic variable of evolution of the universe in a regime of the dominances of a free scalar field. …”
Enlace del recurso
-
332“…As an application we consider the case n = –3 important for oscillations of supernova neutrinos.…”
Enlace del recurso
-
333por Sakharov, Alexander, Ellis, John, Harries, Nicholas, Meregaglia, Anselmo, Rubbia, André“…We consider the limits that may be set on a linear or quadratic violation of Lorentz invariance in the propagation of energetic neutrinos, v/c=[1 +- (E/M_\nuQG1)] or [1 +- (E/M_\nu QG2}^2], using data from supernova explosions and the OPERA long-baseline neutrino experiment.…”
Publicado 2009
Enlace del recurso
Enlace del recurso
-
334por Acciarri, R., Adams, C., Asaadi, J., Baller, B., Bolton, T., Bromberg, C., Cavanna, F., Church, E., Edmunds, D., Ereditato, A., Farooq, S., Ferrari, A., Fitzpatrick, R.S., Fleming, B., Hackenburg, A., Horton-Smith, G., James, C., Lang, K., Lantz, M., Lepetic, I., Littlejohn, B.R., Luo, X., Mehdiyev, R., Page, B., Palamara, O., Rebel, B., Sala, P.R., Scanavini, G., Schukraft, A., Smirnov, G., Soderberg, M., Spitz, J., Szelc, A.M., Weber, M., Wu, W., Yang, T., Zeller, G.P.“…This study represents a successful reconstruction of physics at the MeV scale in a LArTPC, a capability of crucial importance for detection and reconstruction of supernova and solar neutrino interactions in future large LArTPCs.…”
Publicado 2018
Enlace del recurso
Enlace del recurso
-
335“…Explaining the XENON1T excess with transition magnetic moments is marginally possible if very conservative assumptions are adopted regarding the supernova 1987 A and CMB constraints. Finally, we discuss model-building challenges that arise in scenarios that feature large magnetic moments while keeping neutrino masses well below 1 eV. …”
Enlace del recurso
Enlace del recurso
-
336por Goobar, Ariel, Johansson, Joel, Schulze, Steve, Arendse, Nikki, Carracedo, Ana Sagués, Dhawan, Suhail, Mörtsell, Edvard, Fremling, Christoffer, Yan, Lin, Perley, Daniel, Sollerman, Jesper, Joseph, Rémy, Hinds, K-Ryan, Meynardie, William, Andreoni, Igor, Bellm, Eric, Bloom, Josh, Collett, Thomas E., Drake, Andrew, Graham, Matthew, Kasliwal, Mansi, Kulkarni, Shri R., Lemon, Cameron, Miller, Adam A., Neill, James D., Nordin, Jakob, Pierel, Justin, Richard, Johan, Riddle, Reed, Rigault, Mickael, Rusholme, Ben, Sharma, Yashvi, Stein, Robert, Stewart, Gabrielle, Townsend, Alice, Vinko, Jozsef, Wheeler, J. Craig, Wold, Avery“…Detecting gravitationally lensed supernovae is among the biggest challenges in astronomy. …”
Publicado 2023
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
337por Westfall, Aundrea K, Telemeco, Rory S, Grizante, Mariana B, Waits, Damien S, Clark, Amanda D, Simpson, Dasia Y, Klabacka, Randy L, Sullivan, Alexis P, Perry, George H, Sears, Michael W, Cox, Christian L, Cox, Robert M, Gifford, Matthew E, John-Alder, Henry B, Langkilde, Tracy, Angilletta, Michael J, Leaché, Adam D, Tollis, Marc, Kusumi, Kenro, Schwartz, Tonia S“…We found that the Supernova Assembly contained the full genome and was a suitable reference for RNAseq and single-nucleotide polymorphism calling, but the chromosome-level scaffolds provided by the addition of HiC data allowed synteny and whole-genome association mapping analyses. …”
Publicado 2021
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
338por Nguyen, Duong Hoang, Herrmann, Thomas, Härtl, Barbara, Draganov, Dobrin, Minev, Ivelina, Neuharth, Forrest, Gomez, Alberto, Alamillo, Ashley, Schneider, Laura Edith, Kleinholz, Daniela, Minev, Boris, Santidrian, Antonio F.“…Here, we describe how the Supernova (SNV) cell-based oncolytic platform can be utilized to generate off-the-shelf products for cancer treatments. …”
Publicado 2022
Enlace del recurso
Enlace del recurso
Enlace del recurso
Online Artículo Texto -
339por Ridpath, Ian“…World-wide coverage of observatories and telescopes, and major entries on supernova, Big Bang theory, and stellar evolution, make this an invaluable reference source for students, professionals, and amateur astronomers. …”
Publicado 2003
Enlace del recurso
-
340“…The CB-model fit to the AG clearly shows the presence of an associated supernova akin to SN1998bw, and allows even for the determination of the broad-band spectrum of the host galaxy. …”
Enlace del recurso
Enlace del recurso