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The first minutes of a binary-driven hypernova
L. M. Becerra, R. Moradi, J. A. Rueda +2
We simulate the first minutes of the evolution of a binary-driven hypernova (BdHN) event, with a special focus on the associated accretion processes of supernova (SN) ejecta onto t…
The structure of the ultrarelativistic prompt emission phase and the properties of the black hole in GRB 180720B
F. Rastegarnia, R. Moradi, J. A. Rueda +5
In analogy with GRB 190114C, we here analyze the ultrarelativistic prompt emission (UPE) of GRB 180720B observed in the rest-frame time interval --~s by Fer…
GRB 171205A: Hypernova and Newborn Neutron Star
Yu Wang, L. M. Becerra, C. L. Fryer +2
GRB 171205A is a low-luminosity, long-duration gamma-ray burst (GRB) associated with SN 2017iuk, a broad-line type Ic supernova (SN). It is consistent with being formed in the core…
Orbital decay of double white dwarfs: beyond gravitational wave radiation effects
G. A. Carvalho, R. C. dos Anjos, J. G. Coelho +6
The traditional description of the orbital evolution of compact-object binaries, like double white dwarfs (DWDs), assumes that the system is driven only by gravitational wave (GW)…
GRB 190829A -- A Showcase of Binary Late Evolution
Yu Wang, J. A. Rueda, R. Ruffini +7
GRB 190829A is the fourth closest gamma-ray burst (GRB) to date (). Owing to its wide range of radio, optical, X-ray, and the very-high-energy (VHE) observations by H.E.S…
On the X-ray, optical and radio afterglows of the BdHN I GRB 180720B generated by the synchrotron emission
J. A. Rueda, Liang Li, R. Moradi +3
Gamma-ray bursts (GRBs) are systems of unprecedented complexity across all the electromagnetic spectrum, including the radio, optical, X-rays, gamma-rays in the megaelectronvolt (M…