236 research outputs found
On the Mechanism of Townsend Avalanche for Negative Molecular Ions
Time projection chambers drifting negative ions (NITPC) instead of electrons
have several advantages. A NITPC can operate at very high reduced drift fields
without diffusion runaway, and the readout digitization sampling rate
requirement is considerably relaxed due to the low drift speed of negative
ions. The initiation of Townsend avalanches to allow gas gain in these devices
has not been understood until now. It is shown here that the avalanche in low
pressure CS vapor is most likely initiated by collisional detachment of the
electron from the negative molecular ion. In mixtures of Nitromethane vapor
with CO the mechanism appears to be more complex
A benign, low Z electron capture agent for negative ion TPCs
We have identified nitromethane (CHNO) as an effective electron
capture agent for negative ion TPCs (NITPCs).
We present drift velocity and longitudinal diffusion measurements for
negative ion gas mixtures using nitromethane as the capture agent.
Not only is nitromethane substantially more benign than the only other
identified capture agent, CS, but its low atomic number will enable the use
of the NITPC as a photoelectric X{}-ray polarimeter in the 1{}-10 keV band
Low Pressure Negative Ion Drift Chamber for Dark Matter Search
Weakly Interacting Massive Particles (WIMPs) are an attractive candidate for
the dark matter thought to make up the bulk of the mass of our universe. We
explore here the possibility of using a low pressure negative ion drift chamber
to search for WIMPs. The innovation of drifting ions, instead of electrons,
allows the design of a detector with exceptional sensitivity to, background
rejection from, and signature of WIMPs.Comment: 5 pages submitted to PR
The DRIFT Project: Searching for WIMPS with a Directional Detector
A low pressure time projection chamber for the detection of WIMPs is
discussed. Discrimination against Compton electron background in such a device
should be very good, and directional information about the recoil atoms would
be obtainable. If a full 3-D reconstruction of the recoil tracks can be
achieved, Monte Carlo studies indicate that a WIMP signal could be identified
with high confidence from as few as 30 detected WIMP-nucleus scattering events.Comment: 5 pages, 3 figures. Presented at Dark 98, Heidelberg, July 1998, and
to appear in conference proceeding
Energy Deposition of Energetic Silicon Atoms Within a Silicon Lattice
The energy dependence of the ionization produced in silicon by recoiling silicon atoms was measured in the 4–54-keV energy interval. It is found that the fraction of the recoil energy that is dissipated as ionization follows an E1/2 dependence which agrees well with the predictions of the theory of Lindhard et al. [Mat. Fys. Medd. 33, 10 (1963)]
Gaseous Dark Matter Detectors
Dark Matter detectors with directional sensitivity have the potential of
yielding an unambiguous positive observation of WIMPs as well as discriminating
between galactic Dark Matter halo models. In this article, we introduce the
motivation for directional detectors, discuss the experimental techniques that
make directional detection possible, and review the status of the experimental
effort in this field.Comment: 19 pages, review on gaseous directional dark matter detectors
submitted to New Journal of Physic
Directional recoil rates for WIMP direct detection
New techniques for the laboratory direct detection of dark matter weakly
interacting massive particles (WIMPs) are sensitive to the recoil direction of
the struck nuclei. We compute and compare the directional recoil rates
(where is the angle measured from a reference
direction in the sky) for several WIMP velocity distributions including the
standard dark halo and anisotropic models such as Sikivie's late-infall halo
model and logarithmic-ellipsoidal models. Since some detectors may be unable to
distinguish the beginning of the recoil track from its end (lack of head-tail
discrimination), we introduce a ``folded'' directional recoil rate
, where does not distinguish the head from
the tail of the track. We compute the CS and CF exposures required to
distinguish a signal from an isotropic background noise, and find that
is effective for the standard dark halo and some but not
all anisotropic models.Comment: 39 pages, 15 figure
Muon Catalyzed Fusion in 3 K Solid Deuterium
Muon catalyzed fusion in deuterium has traditionally been studied in gaseous
and liquid targets. The TRIUMF solid-hydrogen-layer target system has been used
to study the fusion reaction rates in the solid phase of D_2 at a target
temperature of 3 K. Products of two distinct branches of the reaction were
observed; neutrons by a liquid organic scintillator, and protons by a silicon
detector located inside the target system. The effective molecular formation
rate from the upper hyperfine state of and the hyperfine transition
rate have been measured: , and .
The molecular formation rate is consistent with other recent measurements, but
not with the theory for isolated molecules. The discrepancy may be due to
incomplete thermalization, an effect which was investigated by Monte Carlo
calculations. Information on branching ratio parameters for the s and p wave
d+d nuclear interaction has been extracted.Comment: 19 pages, 11 figures, submitted to PRA Feb 20, 199
A Study of the Residual 39Ar Content in Argon from Underground Sources
The discovery of argon from underground sources with significantly less 39Ar
than atmospheric argon was an important step in the development of
direct-detection dark matter experiments using argon as the active target. We
report on the design and operation of a low background detector with a single
phase liquid argon target that was built to study the 39Ar content of the
underground argon. Underground argon from the Kinder Morgan CO2 plant in
Cortez, Colorado was determined to have less than 0.65% of the 39Ar activity in
atmospheric argon.Comment: 21 pages, 10 figure
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