A bubble chamber for dark matter detection (the COUPP project status)

W. J. Bolte; J. I. Collar; M. Crisler; J. Hall; J. Krider; K. Crum; D. Holmgren; C. M. Lei; D. Nakazawa; H. Nguyen; B. Odom; K. O'Sullivan; R. Plunkett; E. Ramberg; A. Raskin; J. Rasmussen; R. Schmitt; A. Sonnenschein; M. Szydagis; J. D. Vieira

doi:10.1088/1742-6596/39/1/027

A bubble chamber for dark matter detection (the COUPP project status)

W. J. Bolte, J. I. Collar, M. Crisler, J. Hall, J. Krider, K. Crum, D. Holmgren, C. M. Lei, D. Nakazawa, H. Nguyen, B. Odom, K. O'Sullivan, R. Plunkett, E. Ramberg, A. Raskin, J. Rasmussen, R. Schmitt, A. Sonnenschein, M. Szydagis, J. D. Vieira

Research output: Contribution to journal › Article › peer-review

Abstract

Heavy-liquid bubble chambers can be made stable-enough to be used in searches for Weakly Interacting Massive Particles (WIMPs). Advantages of this approach are optimal choice of target liquid-CF₃I, maximally sensitive to both spin-dependent (SD) and spin-independent (SI) WIMP interactions, low cost, good scalability, room temperature operation, extraordinary intrinsic rejection of minimally-ionizing backgrounds, and a number of features permitting rejection of irreducible neutron backgrounds. A 2 kg prototype chamber is currently operating at the depth of 300 meters water equivalent (m.w.e.) NuMi gallery of Fermilab. Even with the small prototype mass, results competitive in the SI channel and surpassing current limits in the SD channel are expected.

Original language	English (US)
Article number	027
Pages (from-to)	126-128
Number of pages	3
Journal	Journal of Physics: Conference Series
Volume	39
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/39/1/027
State	Published - Apr 1 2006
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy(all)

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10.1088/1742-6596/39/1/027

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Bolte, W. J., Collar, J. I., Crisler, M., Hall, J., Krider, J., Crum, K., Holmgren, D., Lei, C. M., Nakazawa, D., Nguyen, H., Odom, B., O'Sullivan, K., Plunkett, R., Ramberg, E., Raskin, A., Rasmussen, J., Schmitt, R., Sonnenschein, A., Szydagis, M., & Vieira, J. D. (2006). A bubble chamber for dark matter detection (the COUPP project status). Journal of Physics: Conference Series, 39(1), 126-128. Article 027. https://doi.org/10.1088/1742-6596/39/1/027

Bolte, WJ, Collar, JI, Crisler, M, Hall, J, Krider, J, Crum, K, Holmgren, D, Lei, CM, Nakazawa, D, Nguyen, H, Odom, B, O'Sullivan, K, Plunkett, R, Ramberg, E, Raskin, A, Rasmussen, J, Schmitt, R, Sonnenschein, A, Szydagis, M & Vieira, JD 2006, 'A bubble chamber for dark matter detection (the COUPP project status)', Journal of Physics: Conference Series, vol. 39, no. 1, 027, pp. 126-128. https://doi.org/10.1088/1742-6596/39/1/027

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abstract = "Heavy-liquid bubble chambers can be made stable-enough to be used in searches for Weakly Interacting Massive Particles (WIMPs). Advantages of this approach are optimal choice of target liquid-CF3I, maximally sensitive to both spin-dependent (SD) and spin-independent (SI) WIMP interactions, low cost, good scalability, room temperature operation, extraordinary intrinsic rejection of minimally-ionizing backgrounds, and a number of features permitting rejection of irreducible neutron backgrounds. A 2 kg prototype chamber is currently operating at the depth of 300 meters water equivalent (m.w.e.) NuMi gallery of Fermilab. Even with the small prototype mass, results competitive in the SI channel and surpassing current limits in the SD channel are expected.",

author = "Bolte, {W. J.} and Collar, {J. I.} and M. Crisler and J. Hall and J. Krider and K. Crum and D. Holmgren and Lei, {C. M.} and D. Nakazawa and H. Nguyen and B. Odom and K. O'Sullivan and R. Plunkett and E. Ramberg and A. Raskin and J. Rasmussen and R. Schmitt and A. Sonnenschein and M. Szydagis and Vieira, {J. D.}",

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AU - Collar, J. I.

AU - Crisler, M.

AU - Hall, J.

AU - Krider, J.

AU - Crum, K.

AU - Holmgren, D.

AU - Lei, C. M.

AU - Nakazawa, D.

AU - Nguyen, H.

AU - Odom, B.

AU - O'Sullivan, K.

AU - Plunkett, R.

AU - Ramberg, E.

AU - Raskin, A.

AU - Rasmussen, J.

AU - Schmitt, R.

AU - Sonnenschein, A.

AU - Szydagis, M.

AU - Vieira, J. D.

PY - 2006/4/1

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AB - Heavy-liquid bubble chambers can be made stable-enough to be used in searches for Weakly Interacting Massive Particles (WIMPs). Advantages of this approach are optimal choice of target liquid-CF3I, maximally sensitive to both spin-dependent (SD) and spin-independent (SI) WIMP interactions, low cost, good scalability, room temperature operation, extraordinary intrinsic rejection of minimally-ionizing backgrounds, and a number of features permitting rejection of irreducible neutron backgrounds. A 2 kg prototype chamber is currently operating at the depth of 300 meters water equivalent (m.w.e.) NuMi gallery of Fermilab. Even with the small prototype mass, results competitive in the SI channel and surpassing current limits in the SD channel are expected.

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A bubble chamber for dark matter detection (the COUPP project status)

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