Zobrazeno 1 - 10
of 102
pro vyhledávání: '"Santos, F. D."'
Offshore wind structures are subject to deterioration mechanisms throughout their operational lifetime. Even if the deterioration evolution of structural elements can be estimated through physics-based deterioration models, the uncertainties involved
Externí odkaz:
http://arxiv.org/abs/2211.00642
Autor:
Santos, F. D. R., Dias, R. G.
Publikováno v:
Scientific Reports volume 10, 4532 (2020)
Adding interactions to many-body Hamiltonians of geometrically frustrated lattices often leads to diminished subspaces of localized states. In this paper, we show how to construct interacting many-body Hamiltonians, starting from the non-interacting
Externí odkaz:
http://arxiv.org/abs/2004.00596
Publikováno v:
Supercond. Sci. Technol. 29 095008 (2016)
We present a numerical study of quasi-1D frustrated Josephson junction ladders with diagonal couplings and open boundary conditions, in the large capacitance limit. We derive a correspondence between the energy of this Josephson junction ladder and t
Externí odkaz:
http://arxiv.org/abs/1607.08201
Publikováno v:
2015 Supercond. Sci. Technol. 28 045021
Motivated by the recent discovery of iron-based superconductors, with high critical temperatures and multiple bands crossing the Fermi level, we address the conditions for the presence of chiral superconducting phases configurations in the in-plane m
Externí odkaz:
http://arxiv.org/abs/1411.0937
Autor:
Longmore, Steven N., Rathborne, Jill, Bastian, Nate, Alves, Joao, Ascenso, Joana, Bally, John, Testi, Leonardo, Longmore, Andy, Battersby, Cara, Bressert, Eli, Purcell, Cormac, Walsh, Andrew, Jackson, James, Foster, Jonathan, Molinari, Sergio, Meingast, Stefan, Amorim, A., Lima, J., Marques, R., Moitinho, A., Pinhao, J., Rebordao, J., Santos, F. D.
Young massive clusters (YMCs) with stellar masses of 10^4 - 10^5 Msun and core stellar densities of 10^4 - 10^5 stars per cubic pc are thought to be the `missing link' between open clusters and extreme extragalactic super star clusters and globular c
Externí odkaz:
http://arxiv.org/abs/1111.3199
Autor:
Kainulainen, J. T., Alves, J. F., Beletsky, Y., Ascenso, J., Kainulainen, J. M., Amorim, A., Lima, J., Marques, R., Pinhao, J., Rebordao, J., Santos, F. D.
We reveal the stellar light emerging from the kiloparsec-scale, ring-like structure of the NGC5128 (Centaurus A) galaxy in unprecedented detail. We use arcsecond-scale resolution near infrared images to create a "dust-free" view of the central region
Externí odkaz:
http://arxiv.org/abs/0906.3521
Autor:
Kowalski, M., Rubin, D., Aldering, G., Agostinho, R. J., Amadon, A., Amanullah, R., Balland, C., Barbary, K., Blanc, G., Challis, P. J., Conley, A., Connolly, N. V., Covarrubias, R., Dawson, K. S., Deustua, S. E., Ellis, R., Fabbro, S., Fadeyev, V., Fan, X., Farris, B., Folatelli, G., Frye, B. L., Garavini, G., Gates, E. L., Germany, L., Goldhaber, G., Goldman, B., Goobar, A., Groom, D. E., Haissinski, J., Hardin, D., Hook, I., Kent, S., Kim, A. G., Knop, R. A., Lidman, C., Linder, E. V., Mendez, J., Meyers, J., Miller, G. J., Moniez, M., Mourao, A. M., Newberg, H., Nobili, S., Nugent, P. E., Pain, R., Perdereau, O., Perlmutter, S., Phillips, M. M., Prasad, V., Quimby, R., Regnault, N., Rich, J., Rubenstein, E. P., Ruiz-Lapuente, P., Santos, F. D., Schaefer, B. E., Schommer, R. A., Smith, R. C., Soderberg, A. M., Spadafora, A. L., Strolger, L. -G., Strovink, M., Suntzeff, N. B., Suzuki, N., Thomas, R. C., Walton, N. A., Wang, L., Wood-Vasey, W. M., Yun, J. L.
Publikováno v:
Astrophys.J.686:749-778,2008
We present a new compilation of Type Ia supernovae (SNe Ia), a new dataset of low-redshift nearby-Hubble-flow SNe and new analysis procedures to work with these heterogeneous compilations. This ``Union'' compilation of 414 SN Ia, which reduces to 307
Externí odkaz:
http://arxiv.org/abs/0804.4142
Autor:
Teixeira, P. S, Fernandes, S. R., Alves, J. F., Correia, J. C., Santos, F. D., Lada, E. A., Lada, C. J.
Publikováno v:
Astron.Astrophys. 413 (2004) L1-L4
In the present paper we present JHK photometric results of the young embedded cluster NGC 2316. We construct the cluster radial profile from which we determine a radius of 0.63 pc. We find 189 $\pm$ 29 cluster members in an extinction limited sub-sam
Externí odkaz:
http://arxiv.org/abs/astro-ph/0311492
Publikováno v:
Europhys.Lett.46:668-674,1999
The deuteron deep inelastic unpolarized structure function F_2^D is calculated using the Wilson operator product expansion method. The long distance behaviour, related to the deuteron bound state properties, is evaluated using the Bethe-Salpeter equa
Externí odkaz:
http://arxiv.org/abs/nucl-th/9711041