Results from the ZEPLIN-III dark matter search experiment
dc.contributor.advisor
Murphy, Alex
en
dc.contributor.advisor
Ghag, Chamkaur
en
dc.contributor.author
Scovell, Paul Robert
en
dc.contributor.sponsor
Science and Technology Facilities Council (STFC)
en
dc.date.accessioned
2014-10-22T15:06:54Z
dc.date.available
2014-10-22T15:06:54Z
dc.date.issued
2011-06-27
dc.description.abstract
The existence of a significant non-baryonic component to the Universe is
widely accepted, with worldwide efforts underway trying to detect this so-called
dark matter. The ZEPLIN-III detector utilises liquid xenon (Xe) as a target
medium in the search for the expected rare interactions of Weakly Interacting
Massive Particles, or WIMPs, with ordinary baryonic matter. The neutralino,
arising in supersymmetric extensions to the standard model of particle physics,
provides a particularly well-motivated candidate. The ZEPLIN-III experiment,
operating in two-phase (liquid/gas) mode, measures both the scintillation and
ionisation signatures produced during an interaction.
The first science run (FSR) of ZEPLIN-III was performed during three months
in 2008. The run culminated in a published result which excluded a WIMP-nucleon
interaction cross-section above 8:1 x 10-8 pb for a 60 GeVc-2 WIMP at
the 90% confidence level.
ZEPLIN-III then entered an upgrade period where the photomultiplier tube
(PMT) array, previously the dominant source of background, was replaced with
new, ultra-low background, PMTs. The radio-contamination of components used
to make these PMTs has been thoroughly studied and their impact on the background
rates in ZEPLIN-III characterised. Additionally, a new 1.5 tonne plastic
scintillator veto detector was constructed, increasing the ability to reject WIMPlike
signals caused by neutron induced nuclear recoil events and improving the γ-ray discrimination capability of ZEPLIN-III.
The second science run (SSR) of ZEPLIN-III began in June 2010 and continued
for 6 months, with a projected upper limit for the interaction cross-section
of 1:52 x 10-8 pb for a 55 GeVc-2 WIMP at the 90% confidence level.
en
dc.identifier.uri
http://hdl.handle.net/1842/9592
dc.language.iso
en
dc.publisher
The University of Edinburgh
en
dc.subject
ZEPLIN-III
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dc.subject
dark matter
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dc.subject
liquid xenon
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dc.title
Results from the ZEPLIN-III dark matter search experiment
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dc.type
Thesis or Dissertation
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dc.type.qualificationlevel
Doctoral
en
dc.type.qualificationname
PhD Doctor of Philosophy
en
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