First results on the search for chameleons with the KWISP detector at CAST

被引：11

作者：

Cuendis, S. Arguedas ^{[7
]}

Baier, J. ^{[5
]}

Barth, K. ^{[7
]}

Baum, S. ^{[17
,18
,19
]}

Bayirli, A. ^{[9
,26
]}

Belov, A. ^{[12
]}

Braeuninger, H. ^{[6
]}

Cantatore, G. ^{[20
,21
]}

Carmona, J. M. ^{[24
]}

Castel, J. F. ^{[24
]}

Cetin, S. A. ^{[9
]}

Dafni, T. ^{[24
]}

Davenport, M. ^{[7
]}

Dermenev, A. ^{[12
]}

Desch, K. ^{[1
]}

Dobrich, B. ^{[7
]}

Fischer, H. ^{[5
]}

Funk, W. g ^{[7
]}

Garcia, J. A. ^{[24
,27
]}

Gardikiotis, A. ^{[13
]}

Garza, J. G. ^{[24
]}

Gninenko, S. ^{[12
]}

Hasinoff, M. D. ^{[22
]}

Hoffmann, D. H. H. ^{[25
]}

Iguaz, F. J. ^{[24
]}

Irastorza, I. G. ^{[24
]}

Jakovcic, K. ^{[23
]}

Kaminski, J. ^{[1
]}

Karuza, M. ^{[14
,15
,16
,20
]}

Krieger, C. ^{[1
,28
]}

Lakic, B. ^{[23
]}

Laurent, J. M. ^{[7
]}

Luzon, G. ^{[24
]}

Maroudas, M. ^{[13
]}

Miceli, L. ^{[2
]}

Neff, S. ^{[4
]}

Ortega, I. ^{[7
,24
]}

Ozbey, A. ^{[9
,29
]}

Pivovaroff, M. J. ^{[10
]}

Rosu, M. ^{[11
]}

Ruz, J. ^{[10
]}

Ruiz Choliz, E. ^{[24
]}

Schmidt, S. ^{[1
]}

Schumann, M. ^{[5
]}

Semertzidis, Y. K. ^{[2
,3
]}

Solanki, S. K. ^{[8
]}

Stewart, L. ^{[7
]}

Tsagris, I. ^{[13
]}

Vafeiadis, T. ^{[7
]}

Vogel, J. K. ^{[10
]}

机构：

[1] Univ Bonn, Phys Inst, D-53115 Bonn, Germany

[2] Inst for Basic Sci Korea, Ctr Axion & Precis Phys Res, Daejeon 34141, South Korea

[3] Korea Adv Inst Sci & Technol, Dept Phys, Daejeon 34141, South Korea

[4] Tech Univ Darmstadt, IKP, Darmstadt, Germany

[5] Albert Ludwigs Univ Freiburg, Phys Inst, D-79104 Freiburg, Germany

[6] Max Planck Inst Extraterr Phys, Garching, Germany

[7] CERN, European Org Nucl Res, CH-1211 Geneva, Switzerland

[8] Max Planck Inst Sonnensyst Forsch, Gottingen, Germany

[9] Istanbul Bilgi Univ, High Energy Phys Res Ctr, Istanbul, Turkey

[10] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA

[11] ELI NP, Magurele 077125, Romania

[12] Russian Acad Sci, INR, Moscow, Russia

[13] Univ Patras, Phys Dept, Patras, Greece

[14] Univ Rijeka, Dept Phys, Rijeka, Croatia

[15] Univ Rijeka, Photon & Quantum Opt Unit, Ctr Excellence Adv Mat & Sensing Devices, Rijeka, Croatia

[16] Ctr Micro & Nano Sci & Technol, Rijeka, Croatia

[17] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, Alba Nova, S-10691 Stockholm, Sweden

[18] KTH Royal Inst Technol, NORDITA, Roslagstullsbacken 23, S-10691 Stockholm, Sweden

[19] Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden

[20] Ist Nazl Fis Nucl, Sez Trieste, Trieste, Italy

[21] Univ Trieste, Trieste, Italy

[22] Univ British Columbia, Dept Phys & Astron, Vancouver, BC, Canada

[23] Rudjer Boskovic Inst, Zagreb, Croatia

[24] Univ Zaragoza, Grp Invest Fis Nucl & Astroparticulas, Zaragoza, Spain

[25] Xi An Jiao Tong Univ, Sch Sci, Xian, Shaanxi, Peoples R China

[26] Bogazici Univ, Phys Dept, Istanbul, Turkey

[27] Chinese Acad Sci, Inst High Energy Phys, Beijing, Peoples R China

[28] Univ Hamburg, Inst Expt Phys, D-22761 Hamburg, Germany

[29] Istanbul Univ Cerrahpasa, Voc Sch Tech Sci, Istanbul, Turkey

[30] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

来源：

PHYSICS OF THE DARK UNIVERSE | 2019年 / 26卷

基金：

欧洲研究理事会; 加拿大自然科学与工程研究理事会;

关键词：

Chameleons; Dark energy; Opto-mechanical sensor; Interferometry;

D O I：

10.1016/j.dark.2019.100367

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report on a first measurement with a sensitive opto-mechanical force sensor designed for the direct detection of coupling of real chameleons to matter. These dark energy candidates could be produced in the Sun and stream unimpeded to Earth. The KWISP detector installed on the CAST axion search experiment at CERN looks for tiny displacements of a thin membrane caused by the mechanical effect of solar chameleons. The displacements are detected by a Michelson interferometer with a homodyne readout scheme. The sensor benefits from the focusing action of the ABRIXAS X-ray telescope installed at CAST, which increases the chameleon flux on the membrane. A mechanical chopper placed between the telescope output and the detector modulates the incoming chameleon stream. We present the results of the solar chameleon measurements taken at CAST in July 2017, setting an upper bound on the force acting on the membrane of 80 pN at 95% confidence level. The detector is sensitive for direct coupling to matter 104 <= beta(m) <= 108, where the coupling to photons is locally bound to beta(gamma) <= 10(11). (c) 2019 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).

引用

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