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L. Becerra

4 papers hereh-index 13480 citations47 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • L. Becerra — 4 papers, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20242026
collaborators

4 papers

astro-ph.HE2026

GRB 220101A: a most energetic 1054 erg long GRB triggered by two supernovae 3.5 seconds apart

R. Ruffini, Y. Aimuratov, L. M. Becerra +10

GRB 220101A is a long GRB, with a total energy exceeding 1054 erg with a redshift z=4.61 and one of the largest ever high-quality multi-wavelength observational coverage,…

astro-ph.HE2025

On the formation of strange quark stars from supernova in compact binaries

L. M. Becerra, F. Cipolletta, A. Drago +4

Strange quark stars (SQSs), namely compact stars entirely composed of deconfined quark matter, are characterized by similar masses and compactness to neutron stars (NSs) and have b…

astro-ph.HE2024

The long-short GRB connection

J. A. Rueda, L. Becerra, C. L. Bianco +4

Long and short gamma-ray bursts (GRBs) are thought to arise from different and unrelated astrophysical progenitors. The association of long GRBs with supernovae (SNe) and the diffe…

astro-ph.HE2024

Occurrence of gravitational collapse in the accreting neutron stars of binary-driven hypernovae

L. M. Becerra, F. Cipolletta, C. L. Fryer +4

The binary-driven hypernova (BdHN) model proposes long gamma-ray bursts (GRBs) originate in binaries composed of a carbon-oxygen (CO) star and a neutron star (NS) companion. The CO…

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