First Results on the Search for Chameleons with the KWISP Detector at CAST

Autor: C. Krieger, Sami K. Solanki, K. Barth, B. Döbrich, S. Neff, Michael J. Pivovaroff, J. Castel, A. Belov, I. Tsagris, E. Ruiz Chóliz, Marc Schumann, A. Ozbey, A. V. Dermenev, A. Bayirli, L. Stewart, S. C. Yildiz, J. Ruz, J. G. Garza, L. Miceli, Serkant Ali Cetin, S. Arguedas Cuendis, T. Dafni, Giovanni Cantatore, J. M. Laurent, F.J. Iguaz, T. Vafeiadis, J. M. Carmona, Klaus Kurt Desch, I. G. Irastorza, M. Maroudas, M. D. Hasinoff, S. N. Gninenko, Biljana Lakić, I. Ortega, H. Bräuninger, M. Vretenar, Konstantin Zioutas, Søren Schmidt, Marin Karuza, Sebastian Baum, Julia Vogel, G. Luzón, A. Gardikiotis, Yannis K. Semertzidis, J. Baier, M. Davenport, Krešimir Jakovčić, M. Rosu, H. Fischer, Wolfgang Funk, J. A. García, Dieter Hoffmann, J. Kaminski
Přispěvatelé: Arguedas Cuendis, S., Baier, J., Barth, K., Baum, S., Bayirli, A., Belov, A., Brauninger, H., Cantatore, G., Carmona, J. M., Castel, J. F., Cetin, S. A., Dafni, T., Davenport, M., Dermenev, A., Desch, K., Dobrich, B., Fischer, H., Funk, W., Garcia, J. A., Gardikiotis, A., Garza, J. G., Gninenko, S., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jakovcic, K., Kaminski, J., Karuza, M., Krieger, C., Lakic, B., Laurent, J. M., Luzon, G., Maroudas, M., Miceli, L., Neff, S., Ortega, I., Ozbey, A., Pivovaroff, M. J., Rosu, M., Ruz, J., Choliz, E. R., Schmidt, S., Schumann, M., Semertzidis, Y. K., Solanki, S. K., Stewart, L., Tsagris, I., Vafeiadis, T., Vogel, J. K., Vretenar, M., Yildiz, S. C., Zioutas, K., İÜC
Jazyk: angličtina
Rok vydání: 2019
Předmět:
Astrophysics and Astronomy
Physics - Instrumentation and Detectors
Photon
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
astro-ph.SR
Physics::Instrumentation and Detectors
Chameleons
FOS: Physical sciences
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
7. Clean energy
High Energy Physics - Experiment
law.invention
Telescope
High Energy Physics - Experiment (hep-ex)
Optics
law
Opto-mechanical sensor
0103 physical sciences
Chameleon
Dark energy
Detectors and Experimental Techniques
010306 general physics
chameleons
dark energy
opto-mechanical sensor
interferometry
Axion
physics.ins-det
Solar and Stellar Astrophysics (astro-ph.SR)
Physics
Coupling
010308 nuclear & particles physics
business.industry
hep-ex
Detector
Michelson interferometer
Astronomy and Astrophysics
Instrumentation and Detectors (physics.ins-det)
Interferometry
Astrophysics - Solar and Stellar Astrophysics
Space and Planetary Science
astro-ph.CO
Direct coupling
business
Particle Physics - Experiment
Astrophysics - Cosmology and Nongalactic Astrophysics
Zdroj: Zaguán. Repositorio Digital de la Universidad de Zaragoza
instname
Physics of the Dark Universe
Zaguán: Repositorio Digital de la Universidad de Zaragoza
Universidad de Zaragoza
Popis: 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 $10^4 \leq\beta_m \leq 10^8$, where the coupling to photons is locally bound to $\beta_\gamma \leq 10^{11}$.
Comment: 21 pages, 12 figures
Databáze: OpenAIRE