168 research outputs found
Dynamics and Radiation of Young Type-Ia Supernova Remnants: Important Physical Processes
We examine and analyze the physical processes that should be taken into
account when modeling young type-Ia SNRs, with ages of several hundred years.
It is shown, that energy losses in the metal-rich ejecta can be essential for
remnants already at this stage of evolution. The influence of electron thermal
conduction and the rate of the energy exchange between electrons and ions on
the temperature distribution and the X-radiation from such remnants is studied.
The data for Tycho SNR from the XMM-Newton X-ray telescope have been employed
for the comparison of calculations with observations.Comment: 19 pages, 8 figure
Search for Pauli Exclusion Principle Violating Atomic Transitions and Electron Decay with a P-type Point Contact Germanium Detector
A search for Pauli-exclusion-principle-violating K-alpha electron transitions
was performed using 89.5 kg-d of data collected with a p-type point contact
high-purity germanium detector operated at the Kimballton Underground Research
Facility. A lower limit on the transition lifetime of 5.8x10^30 seconds at 90%
C.L. was set by looking for a peak at 10.6 keV resulting from the x-ray and
Auger electrons present following the transition. A similar analysis was done
to look for the decay of atomic K-shell electrons into neutrinos, resulting in
a lower limit of 6.8x10^30 seconds at 90 C.L. It is estimated that the MAJORANA
DEMONSTRATOR, a 44 kg array of p-type point contact detectors that will search
for the neutrinoless double-beta decay of 76-Ge, could improve upon these
exclusion limits by an order of magnitude after three years of operation
Low Background Signal Readout Electronics for the MAJORANA DEMONSTRATOR
The MAJORANA DEMONSTRATOR is a planned 40 kg array of Germanium detectors
intended to demonstrate the feasibility of constructing a tonne-scale
experiment that will seek neutrinoless double beta decay () in
. Such an experiment would require backgrounds of less than 1
count/tonne-year in the 4 keV region of interest around the 2039 keV Q-value of
the decay. Designing low-noise electronics, which must be placed
in close proximity to the detectors, presents a challenge to reaching this
background target. This paper will discuss the MAJORANA collaboration's
solutions to some of these challenges
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