Zobrazeno 1 - 10
of 1 245
pro vyhledávání: '"Pisani G"'
Autor:
Rueda J. A., Ruffini R., Rodriguez J. F., Muccino M., Aimuratov Y., Barres de Almeida U., Becerra L., Bianco C. L., Cherubini C., Filippi S., Kovacevic M., Moradi R., Pisani G. B., Wang Y.
Publikováno v:
EPJ Web of Conferences, Vol 168, p 01006 (2018)
We have sub-classified short and long-duration gamma-ray bursts (GRBs) into seven families according to the binary nature of their progenitors. Short GRBs are produced in mergers of neutron-star binaries (NS-NS) or neutron star-black hole binaries (N
Externí odkaz:
https://doaj.org/article/6cd305397a404b749bdeb04cfdf29e3c
Autor:
Pisani G. B., Ruffini R., Aimuratov Y., Bianco C. L., Karlica M., Kovacevic M., Moradi R., Muccino M., Penacchioni A. V., Primorac D., Rueda J. A., Wang Y.
Publikováno v:
EPJ Web of Conferences, Vol 168, p 04002 (2018)
In a series of recent publications, scientists from ICRANet, led by professor Remo Ruffini, have reached a novel comprehensive picture of gamma-ray bursts (GRBs) thanks to their development of a series of new theoretical approaches. Among those, the
Externí odkaz:
https://doaj.org/article/23476396d400435789c97db07bf3aab5
Autor:
Ruffini, R., Moradi, R., Rueda, J. A., Li, L., Sahakyan, N., Chen, Y. -C., Wang, Y., Aimuratov, Y., Becerra, L., Bianco, C. L., Cherubini, C., Filippi, S., Karlica, M., Mathews, G. J., Muccino, M., Pisani, G. B., Xue, S. S.
We recall evidence that long gamma-ray bursts (GRBs) have binary progenitors and give new examples. Binary-driven hypernovae (BdHNe) consist of a carbon-oxygen core (CO$_{\rm core}$) and a neutron star (NS) companion. For binary periods $\sim 5$ min,
Externí odkaz:
http://arxiv.org/abs/2103.09142
Autor:
Muccino, M., Izzo, L., Luongo, O., Boshkayev, K., Amati, L., Della Valle, M., Pisani, G. B., Zaninoni, E.
Observations of gamma-ray bursts up to $z\sim 9$ are best suited to study the possible evolution of the Universe equation of state at intermediate redshifts. We apply the Combo-relation to a sample of 174 gamma ray bursts to investigate possible evid
Externí odkaz:
http://arxiv.org/abs/2012.03392
Autor:
Ruffini, R., Moradi, R., Rueda, J. A., Wang, Y., Aimuratov, Y., Becerra, L., Bianco, C. L., Chen, Y. -C., Cherubini, C., Filippi, S., Karlica, M., Mathews, G. J., Muccino, M., Pisani, G. B., Primorac, D., Xue, S. -S.
X-ray Flashes (XRFs), binary-driven hypernovae (BdHNe) are long GRB subclasses with progenitor a CO$_{\rm core}$, undergoing a supernova (SN) explosion and hypercritically accreting in a tight binary system onto a companion neutron star (NS) or black
Externí odkaz:
http://arxiv.org/abs/1803.05476
Autor:
Ruffini, R., Muccino, M., Aimuratov, Y., Amiri, M., Bianco, C. L., Chen, Y. -C., Panah, B. Eslam, Mathews, G. J., Moradi, R., Pisani, G. B., Primorac, D., Rueda, J. A., Wang, Y.
It has recently become clear that in both short and long gamma-ray bursts (GRBs) it coexists a sequence of different events, each characterized by specific physical processes and corresponding values of the Lorentz gamma factors. The ultra-relativist
Externí odkaz:
http://arxiv.org/abs/1802.07552
Autor:
Ruffini, R., Becerra, L., Bianco, C. L., Chen, Y. C., Karlica, M., Kovacevic, M., Fuksman, J. D. Melon, Moradi, R., Muccino, M., Pisani, G. B., Primorac, D., Rueda, J. A., Vereshchagin, G. V., Wang, Y., Xue, S. -S.
We analyze GRB 151027A within the binary-driven hypernova (BdHN) approach, with progenitor a carbon-oxygen core on the verge of a supernova (SN) explosion and a binary companion neutron star (NS). The hypercritical accretion of the SN ejecta onto the
Externí odkaz:
http://arxiv.org/abs/1712.05001
Autor:
Aimuratov, Y., Ruffini, R., Muccino, M., Bianco, C. L., Penacchioni, A. V., Pisani, G. B., Primorac, D., Rueda, J. A., Wang, Y.
Publikováno v:
ApJ, 844 (2017) 83
Theoretical and observational evidences have been recently gained for a two-fold classification of short bursts: 1) short gamma-ray flashes (S-GRFs), with isotropic energy $E_{iso}<10^{52}$~erg and no BH formation, and 2) the authentic short gamma-ra
Externí odkaz:
http://arxiv.org/abs/1704.08179
Autor:
Ruffini, R., Wang, Y., Aimuratov, Y., de Almeida, U. Barres, Becerra, L., Bianco, C. L., Chen, Y. C., Karlica, M., Kovacevic, M., Li, L., Fuksman, J. D. Melon, Moradi, R., Muccino, M., Penacchioni, A. V., Pisani, G. B., Primorac, D., Rueda, J. A., Shakeri, S., Vereshchagin, G. V., Xue, S. -S.
We analyze the early X-ray flares in the GRB "flare-plateau-afterglow" (FPA) phase observed by Swift-XRT. The FPA occurs only in one of the seven GRB subclasses: the binary-driven hypernovae (BdHNe). This subclass consists of long GRBs with a carbon-
Externí odkaz:
http://arxiv.org/abs/1704.03821
Autor:
Pisani, G. B., Ruffini, R., Aimuratov, Y., Bianco, C. L., Kovacevic, M., Moradi, R., Muccino, M., Penacchioni, A. V., Rueda, J. A., Shakeri, S., Wang, Y.
It has previously been discovered that there is a universal power law behavior exhibited by the late X-ray emission (LXRE) of a "golden sample" (GS) of six long energetic GRBs, when observed in the rest-frame of the source. This remarkable feature, i
Externí odkaz:
http://arxiv.org/abs/1610.05619