Published April 1, 2020 | Version v1
Journal article

Structured Jets and X-Ray Plateaus in Gamma-Ray Burst Phenomena

  • 1. Gran Sasso Science Institute, Viale F. Crispi 7, I-67100, L'Aquila (AQ) (Italy)
  • 2. INAF—Osservatorio Astronomico di Brera, via Emilio Bianchi 46, I-23807 Merate (Italy)

Description

The first multi-messenger detection of a binary neutron star merger, GW170817, brought to the forefront the structured jet model as a way to explain multiwavelength observations taken more than a year after the event. Here, we show that the high-latitude emission from a structured jet can naturally produce an X-ray plateau in gamma-ray burst (GRB) light curves, independent of the radiation from an external shock. We calculate the radiation from a switched-off shell featuring an angular structure in both its relativistic bulk motion and intrinsic brightness. Our model is able to explain the shallow decay phase (plateau) often observed in GRB X-ray light curves. We discuss the possible contribution of the structured jet high-latitude emission to other distinctive features of GRB X-ray light curves, and its capability to explain the chromatic optical/X-ray light-curve properties.

Availability note (English)

Available from http://dx.doi.org/10.3847/1538-4357/ab8221

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
893
Journal Issue
2
Journal Page Range
[10 p.]
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United Kingdom
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
52057090
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BINARY STARS; COSMIC GAMMA BURSTS; DETECTION; EMISSION; JET MODEL; NEUTRON STARS; RELATIVISTIC RANGE; X RADIATION
Descriptors DEC
COSMIC RADIATION; ELECTROMAGNETIC RADIATION; ENERGY RANGE; IONIZING RADIATIONS; MATHEMATICAL MODELS; PARTICLE MODELS; PRIMARY COSMIC RADIATION; RADIATIONS; STARS