Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • harvard1
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Studies of neutron background rejection in the PoGOLite polarimeter
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0001-5191-9306
2010 (English)In: X-ray Polarimetry: A New Window in Astrophysics / [ed] Ronaldo Bellazzini, Enrico Costa, Giorgio Matt, Gianpiero Tagliaferri, Cambridge University Press, 2010, 299-304 p.Conference paper, Published paper (Refereed)
Abstract [en]

The Polarized Gamma-ray Observer (PoGOLite) is a balloon-borne polarimeter based on measuring anisotropy in the azimuthal scattering angle distribution of photons in the energy range 25-80 keV. This is achieved through coincident detection of Compton scattering and photoelectric absorption within a close-packed array of phoswich detector cells (PDCs). Each PDC contains a plastic scintillator rod (main detector component), a plastic scintillator tube (active collimator) and a BGO crystal (anticoincidence shield).

A significant in-flight background is expected from atmospheric neutrons as well as from neutrons produced by interactions of cosmic rays with mechanical structures surrounding the instrument. Although this background can be reduced by introducing suitable shielding materials such as polyethylene, the shield geometry must be optimized through simulations in order to yield sufficient shielding with an acceptable increase in weight.

Geant4-based Monte Carlo simulations have shown that a 10 cm thick polyethylene shield surrounding the PoGOLite instrument is required to sufficiently reduce the background, i.e. fake polarization events, from atmospheric neutrons. In order to validate these simulations, a beam test was carried out, at which 14 MeV neutrons were used to irradiate a simple detector array with four plastic scintillators and three BGO crystals. The array was configured to mimic the PoGOLite detector geometry and also featured a polyethylene neutron shield. Here, we present details of the neutron beam test and our simulation thereof, which demonstrate that the treatment of neutron interactions within the Geant4 framework is reliable. Such simulations can therefore be used to assess in-flight neutron background in balloon-borne instruments, such as the PoGOLite polarimeter.

Place, publisher, year, edition, pages
Cambridge University Press, 2010. 299-304 p.
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-79874ISBN: 978-0-521-19184-5 (print)OAI: oai:DiVA.org:kth-79874DiVA: diva2:495827
Conference
The Coming of Age of X-Ray Polarimetry, Rome, Italy, April 27-30 2009
Note
Publication written by M. Kiss (sole credited author) on behalf of the PoGOLite collaboration. QC 20120210Available from: 2012-02-10 Created: 2012-02-09 Last updated: 2012-02-10Bibliographically approved

Open Access in DiVA

No full text

Other links

Cambridge Books OnlineConference homepage

Authority records BETA

Kiss, Mózsi

Search in DiVA

By author/editor
Kiss, Mózsi
By organisation
Particle and Astroparticle Physics
Astronomy, Astrophysics and Cosmology

Search outside of DiVA

GoogleGoogle Scholar

isbn
urn-nbn

Altmetric score

isbn
urn-nbn
Total: 42 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • harvard1
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf