Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search

James R. Boyce; Andrei Afanasev; George Biallas; Geoffrey Krafft; Mahlon Long; John Mammosser; Dennis Manos; Robert Rimmer; Brianna Thorpe

doi:10.3204/DESY-PROC-2017-02/boyce_jim

Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search

James R. Boyce, Andrei Afanasev, George Biallas, Geoffrey Krafft, Mahlon Long, John Mammosser, Dennis Manos, Robert Rimmer, Brianna Thorpe

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

We report the results of studies showing that temperature dependent photoluminescence is the likely source of unexpected large background rates in afterglow searches for dark sector phenomena, commonly called "chameleons". Using this information, we examine the possibility of a room temperature chameleon afterglow search that automatically eliminates this background. Then, without this background, we discuss a modest search effort exploring the afterglow halflife range 0.1 sec ≤ T_1/2 ≤ 120 sec equivalent to photon coupling constant range 8 × 10¹² ≤ β_γ ≤ 3 × 10¹⁴.

Original language	English
Title of host publication	Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017
Editors	Marios Maroudas
Publisher	Verlag Deutsches Elektronen-Synchrotron
Pages	196-199
Number of pages	4
ISBN (Electronic)	9783945931172
DOIs	https://doi.org/10.3204/DESY-PROC-2017-02/boyce_jim
State	Published - 2017
Event	13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017 - Thessaloniki, Greece Duration: May 15 2017 → May 19 2017

Publication series

Name	Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017

Conference

Conference	13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017
Country/Territory	Greece
City	Thessaloniki
Period	05/15/17 → 05/19/17

Funding

is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under contract DE-AC05-06OR23177.

Funders	Funder number
Office of Nuclear Physics	DE-AC05-06OR23177
U.S. Department of Energy
Office of Science

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10.3204/DESY-PROC-2017-02/boyce_jim

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Boyce, J. R., Afanasev, A., Biallas, G., Krafft, G., Long, M., Mammosser, J., Manos, D., Rimmer, R., & Thorpe, B. (2017). Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search. In M. Maroudas (Ed.), Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017 (pp. 196-199). (Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017). Verlag Deutsches Elektronen-Synchrotron. https://doi.org/10.3204/DESY-PROC-2017-02/boyce_jim

Boyce, James R. ; Afanasev, Andrei ; Biallas, George et al. / Dark-sector photo-magnetic luminescence : The case for a room temperature chameleon search. Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017. editor / Marios Maroudas. Verlag Deutsches Elektronen-Synchrotron, 2017. pp. 196-199 (Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017).

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title = "Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search",

abstract = "We report the results of studies showing that temperature dependent photoluminescence is the likely source of unexpected large background rates in afterglow searches for dark sector phenomena, commonly called {"}chameleons{"}. Using this information, we examine the possibility of a room temperature chameleon afterglow search that automatically eliminates this background. Then, without this background, we discuss a modest search effort exploring the afterglow halflife range 0.1 sec ≤ T1/2 ≤ 120 sec equivalent to photon coupling constant range 8 × 1012 ≤ βγ ≤ 3 × 1014.",

author = "Boyce, {James R.} and Andrei Afanasev and George Biallas and Geoffrey Krafft and Mahlon Long and John Mammosser and Dennis Manos and Robert Rimmer and Brianna Thorpe",

note = "Publisher Copyright: {\textcopyright} Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017. All rights reserved.; 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017 ; Conference date: 15-05-2017 Through 19-05-2017",

year = "2017",

doi = "10.3204/DESY-PROC-2017-02/boyce_jim",

language = "English",

series = "Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017",

publisher = "Verlag Deutsches Elektronen-Synchrotron",

pages = "196--199",

editor = "Marios Maroudas",

booktitle = "Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017",

}

Boyce, JR, Afanasev, A, Biallas, G, Krafft, G, Long, M, Mammosser, J, Manos, D, Rimmer, R & Thorpe, B 2017, Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search. in M Maroudas (ed.), Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017. Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017, Verlag Deutsches Elektronen-Synchrotron, pp. 196-199, 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017, Thessaloniki, Greece, 05/15/17. https://doi.org/10.3204/DESY-PROC-2017-02/boyce_jim

Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search. / Boyce, James R.; Afanasev, Andrei; Biallas, George et al.
Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017. ed. / Marios Maroudas. Verlag Deutsches Elektronen-Synchrotron, 2017. p. 196-199 (Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

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AU - Boyce, James R.

AU - Afanasev, Andrei

AU - Biallas, George

AU - Krafft, Geoffrey

AU - Long, Mahlon

AU - Mammosser, John

AU - Manos, Dennis

AU - Rimmer, Robert

AU - Thorpe, Brianna

PY - 2017

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N2 - We report the results of studies showing that temperature dependent photoluminescence is the likely source of unexpected large background rates in afterglow searches for dark sector phenomena, commonly called "chameleons". Using this information, we examine the possibility of a room temperature chameleon afterglow search that automatically eliminates this background. Then, without this background, we discuss a modest search effort exploring the afterglow halflife range 0.1 sec ≤ T1/2 ≤ 120 sec equivalent to photon coupling constant range 8 × 1012 ≤ βγ ≤ 3 × 1014.

AB - We report the results of studies showing that temperature dependent photoluminescence is the likely source of unexpected large background rates in afterglow searches for dark sector phenomena, commonly called "chameleons". Using this information, we examine the possibility of a room temperature chameleon afterglow search that automatically eliminates this background. Then, without this background, we discuss a modest search effort exploring the afterglow halflife range 0.1 sec ≤ T1/2 ≤ 120 sec equivalent to photon coupling constant range 8 × 1012 ≤ βγ ≤ 3 × 1014.

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T3 - Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017

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BT - Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017

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Boyce JR, Afanasev A, Biallas G, Krafft G, Long M, Mammosser J et al. Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search. In Maroudas M, editor, Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017. Verlag Deutsches Elektronen-Synchrotron. 2017. p. 196-199. (Proceedings of the 13th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2017). doi: 10.3204/DESY-PROC-2017-02/boyce_jim

Dark-sector photo-magnetic luminescence: The case for a room temperature chameleon search

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