Zobrazeno 1 - 10
of 681
pro vyhledávání: '"GRAZIANI, C."'
Autor:
Bertuccio, G., Ahangarianabhari, M., Graziani, C., Macera, D., Shi, Y., Gandola, M., Rachevski, A., Rashevskaya, I., Vacchi, A., Zampa, G., Zampa, N., Bellutti, P., Giacomini, G., Picciotto, A., Piemonte, C., Zorzi, N.
Publikováno v:
IEEE TRANSACTIONS ON NUCLEAR SCIENCE, VOL. 63, NO. 1, FEBRUARY 2016, pp. 400-406
We present a spectroscopic system constituted by a Silicon Drift Detector (SDD) coupled to a CMOS charge sensitive preamplifier, named SIRIO, specifically designed to reach ultimate low noise levels. The SDD, with an active area of 13 mm , has been m
Externí odkaz:
http://arxiv.org/abs/2201.01698
Autor:
Bott, A. F. A., Tzeferacos, P., Chen, L., Palmer, C. A. J., Rigby, A., Bell, A., Bingham, R., Birkel, A., Graziani, C., Froula, D. H., Katz, J., Koenig, M., Kunz, M. W., Li, C. K., Meinecke, J., Miniati, F., Petrasso, R., Park, H. -S., Remington, B. A., Reville, B., Ross, J. S., Ryu, D., Ryutov, D., Séguin, F., White, T. G., Schekochihin, A. A., Lamb, D. Q., Gregori, G.
Understanding magnetic-field generation and amplification in turbulent plasma is essential to account for observations of magnetic fields in the universe. A theoretical framework attributing the origin and sustainment of these fields to the so-called
Externí odkaz:
http://arxiv.org/abs/2007.12837
Autor:
Chen, L. E., Bott, A. F. A., Tzeferacos, P., Rigby, A., Bell, A., Bingham, R., Graziani, C., Katz, J., Koenig, M., Li, C. K., Petrasso, R., Park, H. -S., Ross, J. S., Ryu, D., White, T. G., Reville, B., Matthews, J., Meinecke, J., Miniati, F., Zweibel, E. G., Sarkar, S., Schekochihin, A. A., Lamb, D. Q., Froula, D. H., Gregori, G.
Publikováno v:
Astrophys. J. 892:114, 2020
Identifying the sources of the highest energy cosmic rays requires understanding how they are deflected by the stochastic, spatially intermittent intergalactic magnetic field. Here we report measurements of energetic charged-particle propagation thro
Externí odkaz:
http://arxiv.org/abs/1808.04430
Autor:
Bott, A. F. A., Graziani, C., Tzeferacos, P., White, T. G., Lamb, D. Q., Gregori, G., Schekochihin, A. A.
Recent laser-plasma experiments report the existence of dynamically significant magnetic fields, whose statistical characterisation is essential for understanding the physical processes these experiments are attempting to investigate. In this paper,
Externí odkaz:
http://arxiv.org/abs/1708.01738
Autor:
Tzeferacos, P., Rigby, A., Bott, A., Bell, A. R., Bingham, R., Casner, A., Cattaneo, F., Churazov, E. M., Emig, J., Flocke, N., Fiuza, F., Forest, C. B., Foster, J., Graziani, C., Katz, J., Koenig, M., Li, C. -K., Meinecke, J., Petrasso, R., Park, H. -S., Remington, B. A., Ross, J. S., Ryu, D., Ryutov, D., Weide, K., White, T. G., Reville, B., Miniati, F., Schekochihin, A. A., Froula, D. H., Gregori, G., Lamb, D. Q.
The universe is permeated by magnetic fields, with strengths ranging from a femtogauss in the voids between the filaments of galaxy clusters to several teragauss in black holes and neutron stars. The standard model behind cosmological magnetic fields
Externí odkaz:
http://arxiv.org/abs/1702.03015
Autor:
Tzeferacos, P., Rigby, A., Bott, A., Bell, A. R., Bingham, R., Casner, A., Cattaneo, F., Churazov, E. M., Emig, J., Fiuza, F., Forest, C. B., Foster, J., Graziani, C., Katz, J., Koenig, M., Li, C. -K., Meinecke, J., Petrasso, R., Park, H. -S., Remington, B. A., Ross, J. S., Ryu, D., Ryutov, D., White, T. G., Reville, B., Miniati, F., Schekochihin, A. A., Lamb, D. Q., Froula, D. H., Gregori, G.
Magnetic fields are ubiquitous in the Universe. Extragalactic disks, halos and clusters have consistently been shown, via diffuse radio-synchrotron emission and Faraday rotation measurements, to exhibit magnetic field strengths ranging from a few nG
Externí odkaz:
http://arxiv.org/abs/1702.03016
Autor:
Jordan IV, G. C., Graziani, C., Fisher, R. T., Townsley, D. M., Meakin, C., Weide, K., Reid, L. B., Norris, J., Hudson, R., Lamb, D. Q.
We describe the detonation mechanism comprising the "Pulsationally Assisted" Gravitationally Confined Detonation (GCD) model of Type Ia supernovae SNe Ia. This model is analogous to the previous GCD model reported in Jordan et al.(2008); however, the
Externí odkaz:
http://arxiv.org/abs/1202.3997
Autor:
Arimoto, M., Kawai, N., Asano, K., Hurley, K., Suzuki, M., Nakagawa, Y. E., Shimokawabe, T., Pazmino, N. V., Sato, R., Matsuoka, M., Yoshida, A., Tamagawa, T., Shirasaki, Y., Sugita, S., Takahashi, I., Atteia, J. -L., Pelangeon, A., Vanderspek, R., Graziani, C., Prigozhin, G., Villasenor, J., Jernigan, J. G., Crew, G. B., Sakamoto, T., Ricker, G. R., Woosley, S. E., Butler, N., Levine, A., Doty, J. P., Donaghy, T. Q., Lamb, D. Q., Fenimore, E., Galassi, M., Boer, M., Dezalay, J. -P., Olive, J. -F., Braga, J., Manchanda, R., Pizzichini, G.
Using a pulse-fit method, we investigate the spectral lags between the traditional gamma-ray band (50-400 keV) and the X-ray band (6-25 keV) for 8 GRBs with known redshifts (GRB 010921, GRB 020124, GRB 020127, GRB 021211, GRB 030528, GRB 040924, GRB
Externí odkaz:
http://arxiv.org/abs/1002.3849
Autor:
Pélangeon, A., Atteia, J. -L., Nakagawa, Y. E., Hurley, K., Yoshida, A., Vanderspek, R., Suzuki, M., Kawai, N., Pizzichini, G., Boër, M., Braga, J., Crew, G., Donaghy, T. Q., Dezalay, J. P., Doty, J., Fenimore, E. E., Galassi, M., Graziani, C., Jernigan, J. G., Lamb, D. Q., Levine, A., Manchanda, J., Martel, F., Matsuoka, M., Olive, J. -F., Prigozhin, G., Ricker, G. R., Sakamoto, T., Shirasaki, Y., Sugita, S., Takagishi, K., Tamagawa, T., Villasenor, J., Woosley, S. E., Yamauchi, M.
Publikováno v:
Astron.Astrophys.491:157-171,2008
Aims: Taking advantage of the forthcoming Catalog of the HETE-2 mission, the aim of this paper is to evaluate the main properties of HETE-2 GRBs - the E_peak, the T_90 and the E_iso - in their source frames and to derive their unbiased distribution.
Externí odkaz:
http://arxiv.org/abs/0811.3304
Autor:
Jordan IV, G C, Fisher, R T, Townsley, D M, Calder, A C, Graziani, C, Asida, S, Lamb, D Q, Truran, J W
Publikováno v:
Astrophys.J.681:1448-1457,2008
We report the results of a series of three-dimensional (3-D) simulations of the deflagration phase of the gravitationally confined detonation mechanism for Type Ia supernovae. In this mechanism, ignition occurs at one or several off-center points, re
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703573