Zobrazeno 1 - 10
of 633
pro vyhledávání: '"Barranco, J"'
Autor:
Garnica, Yadir, Barranco, J.
It is well known that the coupling of the axion-like particle with the photon modifies Maxwell equations. One of the main consequences of these modifications is the conversion of axions into photons. Little has been said about the effect of the modif
Externí odkaz:
http://arxiv.org/abs/2409.04648
Autor:
Velázquez-Ibarra, L., Barranco, J.
In this work we compute the resonant wavelength of whispering gallery modes for bulk-fused silica microspheres including chromatic dispersion. This is done following two methods: by solving the exact characteristic equation and, on the other hand, by
Externí odkaz:
http://arxiv.org/abs/2403.00589
Autor:
Lesur, G., Ercolano, B., Flock, M., Lin, M. -K., Yang, C. -C., Barranco, J. A., Benitez-Llambay, P., Goodman, J., Johansen, A., Klahr, H., Laibe, G., Lyra, W., Marcus, P., Nelson, R. P., Squire, J., Simon, J. B., Turner, N., Umurhan, O. M., Youdin, A. N.
The building of planetary systems is controlled by the gas and dust dynamics of protoplanetary disks. While the gas is simultaneously accreted onto the central star and dissipated away by winds, dust grains aggregate and collapse to form planetesimal
Externí odkaz:
http://arxiv.org/abs/2203.09821
Autor:
Roque, Armando A., Barranco, J.
Publikováno v:
Phys. Rev. D 102, 104010 (2020)
Cold Dark Stars made of self-gravitating fermions in the degenerate limit are constructed in General Relativity and in R-square gravity, $f(R)=R+\alpha R^2$. The properties of the resulting Cold Dark Stars in both theories of gravity are studied. It
Externí odkaz:
http://arxiv.org/abs/1912.09222
Autor:
López-Machado, M.A., Rodriguez, D Alonso, Basulto-Puig, J.C., Martin-Hernandez, T., Sánchez-Miranda, D., Agüero-Betancourt, C.M., Besú-García, B., Rodríguez-Fernández, Y., Guerrero-Vega, L., GómezFonseca, I., Ramos-Pérez, O., Acosta-Domínguez, I., Ronquillo-Ramirez, D., Díaz-Fernández, Y., Aguilar-Soto, L., Reíd-Montejo, J., Palomo-Leyva, Y., LandinFaria, M.R., Rosendo-Domínguez, R.M., Alonso-Manresa, C., Marín-Pérez, D.M., Malo-Lantigua, Y., Rodríguez-Florat, M.C., Delgado-Laborit, Y., RodriguezGuevara, Y., Peláez-González, M., Torres-Mora, Y., Cabrera-Hernández, O.S., Gimarais-Varona, F.J., Hormigot-Hernández, M., Artola-Gutiérrez, L.V., Gallardo-Martí, L., Porro-Verdecia, J., Castro-Bistorte, R., RobertsDandie, E., Berenguer-Pedroso, S., Manso-García, Yudith, Mora-García, C.V., Lastre-Muñoz, Y., Duran-Rivero, O., Hernández-García, B., Escobar-Escobar, K., CarmenatesGutiérrez, M.K., Conde-Bello, B., Olazabal-Linares, E.L., Bringas-Labrada, I., Noy-León, M., Velazco-González, N., Bursosa-Moreno, B., Morell-Padrón, Y., Rodríguez-Matos, Y., Treto-Torguet, Y.M., Comas-Díaz, L., Miranda, F., FigueredoGonzález, Y., Quiñones-Juan, A., Mursuli-García, I., Giménez-Velásquez, V.M., Hernández-Ávila, A., Hernández-Cabrera, T., García-Zulueta, T., Parra-Pérez, A., Cintra-Jacob, D., Mendoza-Jiménez, M., de la Fuente-Carbonell, S.M., Hernández-Eduard, B., Ochoa-García, M., Garcia-Iglesias, E., Álvarez-Acosta, A., Martínez-Rosales, R.U., Ávila-Díaz, L., Santana-Vázquez, Z., Mila-Cáceres, L., Guillén-Nieto, G.E., Fuentes-Aguilar, F., Nordelo-Valdivia, A., GonzálezFernández, N., González-Sarmientos, M., Rubio-Salinas, A., Domínguez-Rabilero, L.C., Espinosa-Peña, R.A., Ramírez-Núñez, Y., Junco-Barranco, J., Díaz-González, O., Fragas-Quintero, A., Pérez-Guevara, M.T., Enriquez-Puertas, J.M., Infante-Hernández, Y., Cruz-Sui, O., NoaRomero, E., López, Yizel Hernández, Sánchez-García, J.E., Rodríguez-Martínez, E., Pimentel-Vázquez, E., Martínez-Díaz, E., Cinza-Estévez, Zurina, Resik-Aguirre, Sonia, Figueroa-Baile, Nelvis L., Oquendo-Martínez, Rachel, Campa-Legrá, Ivan, Tejeda-Fuentes, Alina, Rivero-Caballero, Marila, González-García, Gloria, Chávez-Chong, Cristina O., Alonso-Valdés, Marel, Hernández-Bernal, Francisco, Lemos-Pérez, Gilda, Campal-Espinosa, Ana, Freyre-Corrales, Giselle, Benítez-Gordillo, Delia, Gato-Orozco, Evelyn, Pérez Bartutis, Greter Susana, Mesa-Pedroso, Iliana, Bueno-Alemani, Nilda, Infante-Aguilar, Elizabeth, Rodríguez Reinoso, José Luis, Melo-Suarez, Grettel, Limonta-Fernández, Miladys, Ayala-Ávila, Marta, Muzio-González, Verena L.
Publikováno v:
In eClinicalMedicine September 2023 63
Akademický článek
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The equation of state for a degenerate gas of fermions at zero temperature in the non relativistic case is a polytrope, i.e. $p=\gamma \rho^{5/3}/m_F^{8/3}$. If dark matter is modelled by such non interacting fermion, this dependence in the mass of t
Externí odkaz:
http://arxiv.org/abs/1811.11125
The future detection and measurement of the diffuse neutrino supernova background will shed light on the rate of supernovae events in the Universe, the star formation rate and the neutrino spectrum from each supernova. Little has been said about what
Externí odkaz:
http://arxiv.org/abs/1706.03834
Autor:
Angal-Kalinin, D., Appleby, R., Arduini, G., Banfi, D., Barranco, J., Biancacci, N., Brett, D., Bruce, R., Bruening, O., Buffat, X., Burov, A., Cai, Y., Calaga, R., Chancé, A., Crouch, M., Dalena, B., Day, H., de Maria, R., Muller, J. Esteban, Fartoukh, S., Fitterer, M., Frasciello, O., Giovannozzi, M., Herr, W., Höfle, W., Holzer, B., Iadarola, G., Jowett, J. M., Korostelev, M., Li, K., McIntosh, E., Métral, E., Mostacci, A., Mounet, N., Muratori, B., Nosochkov, Y., Ohmi, K., Papaphilippou, Y., Paret, S., Payet, J., Pieloni, T., Qiang, J., Rijoff, T., Rossi, L., Rumolo, G., Salvant, B., Schaumann, M., Shaposhnikova, E., Shatilov, D., Tambasco, C., Tomás, R., Valishev, A., Wang, M. -H., Wanzenberg, R., White, S., Wolski, A., Zagorodnova, O., Zannini, C., Zimmermann, F., Zobov, M.
Publikováno v:
CERN Yellow Report CERN 2015-005, pp. 21-60
Chapter 2 in High-Luminosity Large Hadron Collider (HL-LHC) : Preliminary Design Report. The Large Hadron Collider (LHC) is one of the largest scientific instruments ever built. Since opening up a new energy frontier for exploration in 2010, it has g
Externí odkaz:
http://arxiv.org/abs/1705.09447
Massive neutrinos can have helicity $s_{\parallel}\neq -1$. Neutrino helicity changes when the neutrino interacts with an external magnetic field and it is possible that the left-handed neutrinos born inside the Sun or a supernova could leave their s
Externí odkaz:
http://arxiv.org/abs/1704.01549