DMTPC-10L: Direction-Sensitive Dark Matter Detector Prototype
| dc.creator | Dujmic, D. | |
| dc.creator | Fisher, P. | |
| dc.creator | Lanza, R. | |
| dc.creator | Lopez, J. | |
| dc.creator | Kaboth, A. | |
| dc.creator | Kohse, G. | |
| dc.creator | Monroe, J. | |
| dc.creator | Vanderspek, R. | |
| dc.creator | Sciolla, G. | |
| dc.creator | Yamamoto, R. | |
| dc.creator | Ahlen, S. | |
| dc.creator | Otis, K. | |
| dc.creator | Roccaro, A. | |
| dc.creator | Tomita, H. | |
| dc.creator | Skvorodnev, N. | |
| dc.creator | Wellenstein, H. | |
| dc.date | 2008-10-15 | |
| dc.date.accessioned | 2026-07-07T10:10:27Z | |
| dc.date.available | 2026-07-07T10:10:27Z | |
| dc.description | The known direction of motion of dark matter particles relative to the Earth may be a key for their unambiguous identification even in the presence of backgrounds. We describe a prototype detector that is able to reconstruct direction vectors of weakly interacting massive particles that may the dominant constituent of the dark matter in our galaxy. The detector uses a low-density gas (CF4) in a 10liter time-projection chamber with mesh-based electrodes and optical and charge readout. Initial results confirm good performance in the reconstruction of direction angle and sense ('head-tail') for low-momentum nuclear recoils. | |
| dc.description | Presented at the 34th International Conference on High Energy Physics, Philadelphia, 2008 | |
| dc.identifier | https://arxiv.org/abs/0810.2769 | |
| dc.identifier | http://arxiv.org/abs/0810.2769 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/171606 | |
| dc.subject | Instrumentation and Detectors | |
| dc.title | DMTPC-10L: Direction-Sensitive Dark Matter Detector Prototype | |
| dc.type | text |