XENON

E. Aprile; K. L. Giboni; M. E. Monzani; G. Plante; M. Yamashita; R. J. Gaitskell; S. Fiorucci; P. Sorensen; L. DeViveiros; A. Bernstein; N. Madden; C. Winant; T. Shutt; J. Kwong; A. Bolozdynya; E. Dahl; U. Oberlack; P. Shagin; R. Gomez; D. McKinsey; A. Manzur; R. Hasty; K. Ni; F. Arneodo; A. Ferella; L. Baudis; J. Angle; J. Orboeck; A. Manalaysay; J. A.M. Lopes; L. Coelho; L. Fernandes; J. Santos

doi:10.1016/j.nuclphysbps.2007.08.142

XENON

E. Aprile, K. L. Giboni, M. E. Monzani, G. Plante, M. Yamashita, R. J. Gaitskell, S. Fiorucci, P. Sorensen, L. DeViveiros, A. Bernstein, N. Madden, C. Winant, T. Shutt, J. Kwong, A. Bolozdynya, E. Dahl, U. Oberlack, P. Shagin, R. Gomez, D. McKinseyA. Manzur, R. Hasty, K. Ni, F. Arneodo, A. Ferella, L. Baudis, J. Angle, J. Orboeck, A. Manalaysay, J. A.M. Lopes, L. Coelho, L. Fernandes, J. Santos

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Abstract

The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xenon nuclei. With 1 ton of LXe distributed in ten identical modules, the proposed XENON1T experiment will achieve a sensitivity more than a factor of thousand beyond current limits.The detectors are time projection chambers operated in dual (liquid/gas) phase, to detect simultaneously the ionization, through secondary scintillation in the gas, and primary scintillation in the liquid produced by low energy recoils. We review some of the results from the prototype XENON3 detector and briefly discuss about the status of current XENON10 at Gran Sasso Laboratory in Italy.

Original language	English (US)
Pages (from-to)	113-116
Number of pages	4
Journal	Nuclear Physics B - Proceedings Supplements
Volume	173
DOIs	https://doi.org/10.1016/j.nuclphysbps.2007.08.142
State	Published - Nov 2007

All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics
Nuclear and High Energy Physics

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10.1016/j.nuclphysbps.2007.08.142

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Aprile, E., Giboni, K. L., Monzani, M. E., Plante, G., Yamashita, M., Gaitskell, R. J., Fiorucci, S., Sorensen, P., DeViveiros, L., Bernstein, A., Madden, N., Winant, C., Shutt, T., Kwong, J., Bolozdynya, A., Dahl, E., Oberlack, U., Shagin, P., Gomez, R., ... Santos, J. (2007). XENON. Nuclear Physics B - Proceedings Supplements, 173, 113-116. https://doi.org/10.1016/j.nuclphysbps.2007.08.142

@article{9e79e079e99a425fac0e7e279ec2888f,

title = "XENON",

abstract = "The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xenon nuclei. With 1 ton of LXe distributed in ten identical modules, the proposed XENON1T experiment will achieve a sensitivity more than a factor of thousand beyond current limits.The detectors are time projection chambers operated in dual (liquid/gas) phase, to detect simultaneously the ionization, through secondary scintillation in the gas, and primary scintillation in the liquid produced by low energy recoils. We review some of the results from the prototype XENON3 detector and briefly discuss about the status of current XENON10 at Gran Sasso Laboratory in Italy.",

author = "E. Aprile and Giboni, {K. L.} and Monzani, {M. E.} and G. Plante and M. Yamashita and Gaitskell, {R. J.} and S. Fiorucci and P. Sorensen and L. DeViveiros and A. Bernstein and N. Madden and C. Winant and T. Shutt and J. Kwong and A. Bolozdynya and E. Dahl and U. Oberlack and P. Shagin and R. Gomez and D. McKinsey and A. Manzur and R. Hasty and K. Ni and F. Arneodo and A. Ferella and L. Baudis and J. Angle and J. Orboeck and A. Manalaysay and Lopes, {J. A.M.} and L. Coelho and L. Fernandes and J. Santos",

note = "Funding Information: This work was funded by NSF Grants No. PHY-03-02646 and No. PHY-04-00596, and DOE Grant No. DE-FG02-91ER40688.",

year = "2007",

month = nov,

doi = "10.1016/j.nuclphysbps.2007.08.142",

language = "English (US)",

volume = "173",

pages = "113--116",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier B.V.",

}

Aprile, E, Giboni, KL, Monzani, ME, Plante, G, Yamashita, M, Gaitskell, RJ, Fiorucci, S, Sorensen, P, DeViveiros, L, Bernstein, A, Madden, N, Winant, C, Shutt, T, Kwong, J, Bolozdynya, A, Dahl, E, Oberlack, U, Shagin, P, Gomez, R, McKinsey, D, Manzur, A, Hasty, R, Ni, K, Arneodo, F, Ferella, A, Baudis, L, Angle, J, Orboeck, J, Manalaysay, A, Lopes, JAM, Coelho, L, Fernandes, L & Santos, J 2007, 'XENON', Nuclear Physics B - Proceedings Supplements, vol. 173, pp. 113-116. https://doi.org/10.1016/j.nuclphysbps.2007.08.142

TY - JOUR

T1 - XENON

AU - Aprile, E.

AU - Giboni, K. L.

AU - Monzani, M. E.

AU - Plante, G.

AU - Yamashita, M.

AU - Gaitskell, R. J.

AU - Fiorucci, S.

AU - Sorensen, P.

AU - DeViveiros, L.

AU - Bernstein, A.

AU - Madden, N.

AU - Winant, C.

AU - Shutt, T.

AU - Kwong, J.

AU - Bolozdynya, A.

AU - Dahl, E.

AU - Oberlack, U.

AU - Shagin, P.

AU - Gomez, R.

AU - McKinsey, D.

AU - Manzur, A.

AU - Hasty, R.

AU - Ni, K.

AU - Arneodo, F.

AU - Ferella, A.

AU - Baudis, L.

AU - Angle, J.

AU - Orboeck, J.

AU - Manalaysay, A.

AU - Lopes, J. A.M.

AU - Coelho, L.

AU - Fernandes, L.

AU - Santos, J.

N1 - Funding Information: This work was funded by NSF Grants No. PHY-03-02646 and No. PHY-04-00596, and DOE Grant No. DE-FG02-91ER40688.

PY - 2007/11

Y1 - 2007/11

N2 - The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xenon nuclei. With 1 ton of LXe distributed in ten identical modules, the proposed XENON1T experiment will achieve a sensitivity more than a factor of thousand beyond current limits.The detectors are time projection chambers operated in dual (liquid/gas) phase, to detect simultaneously the ionization, through secondary scintillation in the gas, and primary scintillation in the liquid produced by low energy recoils. We review some of the results from the prototype XENON3 detector and briefly discuss about the status of current XENON10 at Gran Sasso Laboratory in Italy.

AB - The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xenon nuclei. With 1 ton of LXe distributed in ten identical modules, the proposed XENON1T experiment will achieve a sensitivity more than a factor of thousand beyond current limits.The detectors are time projection chambers operated in dual (liquid/gas) phase, to detect simultaneously the ionization, through secondary scintillation in the gas, and primary scintillation in the liquid produced by low energy recoils. We review some of the results from the prototype XENON3 detector and briefly discuss about the status of current XENON10 at Gran Sasso Laboratory in Italy.

UR - http://www.scopus.com/inward/record.url?scp=36248964811&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=36248964811&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2007.08.142

DO - 10.1016/j.nuclphysbps.2007.08.142

M3 - Article

AN - SCOPUS:36248964811

SN - 0920-5632

VL - 173

SP - 113

EP - 116

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

ER -

XENON

Abstract

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