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 |
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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 |
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