activity
20022026
most citedSecond Order Scalar Invariants of the Riemann Tensor: Applications to Black Hole Spacetimes

112 citations · 1.2k across the 49 of their papers we have counts for

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Showing astro-ph.HEShow all

10 papers · 1 filter

astro-ph.HE2023★ 18 cited

GRB-SN Association within the Binary-Driven Hypernova Model

Y. Aimuratov, L. M. Becerra, C. L. Bianco +11

The observations of supernovae (SNe) Ic occurring after the prompt emission of long gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model where GRBs…

astro-ph.HE2021★ 22 cited

Nature of the ultrarelativistic prompt emission phase of GRB 190114C

R. Moradi, J. A. Rueda, R. Ruffini +7

We address the physical origin of the ultrarelativistic prompt emission (UPE) phase of GRB 190114C observed in the interval 1.9-3.99 s, by the Fermi-GBM in 10 keV-10 MeV . Thanks t…

astro-ph.HE2021★ 24 cited

The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs

R. Ruffini, R. Moradi, J. A. Rueda +14

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}…

astro-ph.HE2019★ 6 cited

Self-similarity and power-laws in GRB 190114C

R. Ruffini, Liang Li, R. Moradi +10

Following Fermi and NOT observations, Ruffini et al. (2019b) soon identified GRB 190114C as BdHN I at z=0.424, it has been observed since, with unprecedented accuracy, [...] all th…

astro-ph.HE2018★ 47 cited

On the GeV emission of the type I BdHN GRB 130427A

R. Ruffini, R. Moradi, J. A. Rueda +9

We propose that the "inner engine" of a type I binary-driven hypernova (BdHN) is composed of a Kerr black hole (BH) in a non-stationary state, embedded in a uniform magnetic field…

astro-ph.HE2018★ 6 cited

The inner engine of GeV-radiation-emitting gamma-ray bursts

R. Ruffini, J. A. Rueda, R. Moradi +12

We motivate how the most recent progress in the understanding the nature of the GeV radiation in most energetic gamma-ray bursts (GRBs), the binary-driven hypernovae (BdHNe), has l…

astro-ph.HE2016★ 26 cited

On the last stable orbit around rapidly rotating neutron stars

Federico Cipolletta, Christian Cherubini, Simonetta Filippi +2

We compute the binding energy and angular momentum of a test-particle at the last stable circular orbit (LSO) on the equatorial plane around a general relativistic, rotating neutro…

astro-ph.HE2016★ 23 cited

GRB 090510: a genuine short-GRB from a binary neutron star coalescing into a Kerr-Newman black hole

R. Ruffini, M. Muccino, Y. Aimuratov +9

In a new classification of merging binary neutron stars (NSs) we separate short gamma-ray bursts (GRBs) in two sub-classes. The ones with erg coalesce to f…

astro-ph.HE2016★ 20 cited

On the rate and on the gravitational wave emission of short and long GRBs

R. Ruffini, J. Rodriguez, M. Muccino +13

On the ground of the large number of gamma-ray bursts (GRBs) detected with cosmological redshift, we classified GRBs in seven subclasses, all with binary progenitors originating gr…

astro-ph.HE2009★ 32 cited

pair creation by vacuum polarization around electromagnetic black holes

C. Cherubini, A. Geralico, J. Rueda +1

The concept of "dyadotorus" was recently introduced to identify in the Kerr-Newman geometry the region where vacuum polarization processes may occur, leading to the creation of $e^…