Simulation of the Directional Dark Matter Detector (D3) and Directional Neutron Observer (DiNO)

H. Feng; I. Jaegle; J. Yamaoka; S.E. Vahsen; S. Ross

REVIEW

Simulation of the Directional Dark Matter Detector (D3) and Directional Neutron Observer (DiNO)

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1110.3444 v1 pith:MNNTNH5J submitted 2011-10-16 astro-ph.IM

I. Jaegle , H. Feng , S. Ross , J. Yamaoka , S.E. Vahsen This is my paper

classification astro-ph.IM

keywords directionalneutrondarkdetectormatterobserversimulationstudies

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

Preliminary simulation and optimization studies of the Directional Dark Matter Detector and the Directional Neutron Observer are presented. These studies show that the neutron interaction with the gas-target in these detectors is treated correctly by GEANT4 and that by lowering the pressure, the sensitivity to low-mass WIMP candidates is increased. The use of negative ion drift might allow us to search the WIMP mass region suggested by the results of the non-directional experiments DAMA/LIBRA, CoGeNT and CRESST-II.

Discussion (0). Sign in to comment.

Pith tools