Published August 18, 2011 | Version v1
Journal article Metadata-only

A Model for Simulating Realistic Profiles of Pulsars

Creators

  • 1. National Centre for Radio Astrophysics, Pune (India)
  • 2. Indian Institute of Astrophysics, Bangalore (India)

Description

We devise an accurate method to compute the emission profile corresponding to a given set of pulsar emission parameters, for eg. inclination angle α, impact angle β, frequency of emission ω, Lorentz factor γ, and pulsar spin-period P. The intensity of emission is simulated, and compared with the observed profiles.

Additional details

Identifiers

DOI
10.1063/1.3615140;

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1357
Journal Issue
1
Journal Page Range
p. 297-298
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
An astrophysical key to unlock the secrets of the Universe
Acronym
Conference on radio pulsars
Dates
10-15 Oct 2010
Place
Chia, Sardinia (Italy)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
43083717
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ASTROPHYSICS; COMPUTERIZED SIMULATION; INCLINATION; PHOTON EMISSION; PROMPT GAMMA RADIATION; PULSARS; ROTATION; SPIN
Descriptors DEC
ANGULAR MOMENTUM; COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; EMISSION; GAMMA RADIATION; IONIZING RADIATIONS; MOTION; PARTICLE PROPERTIES; PHYSICS; RADIATIONS; SIMULATION

Optional Information

Notes
(c) 2011 American Institute of Physics