no code implementations • 18 Oct 2019 • T. Braine, R. Cervantes, N. Crisosto, N. Du, S. Kimes, L. J Rosenberg, G. Rybka, J. Yang, D. Bowring, A. S. Chou, R. Khatiwada, A. Sonnenschein, W. Wester, G. Carosi, N. Woollett, L. D. Duffy, R. Bradley, C. Boutan, M. Jones, B. H. LaRoque, N. S. Oblath, M. S. Taubman, J. Clarke, A. Dove, A. Eddins, S. R. O'Kelley, S. Nawaz, I. Siddiqi, N. Stevenson, A. Agrawal, A. V. Dixit, J. R. Gleason, S. Jois, P. Sikivie, N. S. Sullivan, D. B. Tanner, E. Lentz, E. J. Daw, J. H. Buckley, P. M. Harrington, E. A. Henriksen, K. W. Murch
This paper reports on a cavity haloscope search for dark matter axions in the galactic halo in the mass range $2. 81$-$3. 31$ ${\mu}eV$.
High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics Instrumentation and Detectors
no code implementations • 3 Jan 2019 • C. Boutan, M. Jones, B. H. LaRoque, N. S. Oblath, R. Cervantes, N. Du, N. Force, S. Kimes, R. Ottens, L. J. Rosenberg, G. Rybka, J. Yang, G. Carosi, N. Woollett, D. Bowring, A. S. Chou, R. Khatiwada, A. Sonnenschein, W. Wester, R. Bradley, E. J. Daw, A. Agrawal, A. V. Dixit, J. Clarke, S. R. O'Kelley, N. Crisosto, J. R. Gleason, S. Jois, P. Sikivie, I. Stern, N. S. Sullivan, D. B. Tanner, P. M. Harrington, E. Lentz
The $\mu$eV axion is a well-motivated extension to the standard model.
High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics Instrumentation and Detectors
no code implementations • 16 Apr 2018 • N. Du, N. Force, R. Khatiwada, E. Lentz, R. Ottens, L. J Rosenberg, G. Rybka, G. Carosi, N. Woolett, D. Bowring, A. S. Chou, A. Sonnenschein, W. Wester, C. Boutan, N. S. Oblath, R. Bradley, E. J. Daw, A. V. Dixit, J. Clarke, S. R. O'Kelley, N. Crisosto, J. R. Gleason, S. Jois, P. Sikivie, I. Stern, N. S. Sullivan, D. B. Tanner, G. C. Hilton
This Letter reports results from a haloscope search for dark matter axions with masses between 2. 66 and 2. 81 $\mu$eV.
High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics Instrumentation and Detectors
no code implementations • 30 Oct 2009 • The ADMX Collaboration, S. J. Asztalos, G. Carosi, C. Hagmann, D. Kinion, K. van Bibber, M. Hotz, L. Rosenberg, G. Rybka, J. Hoskins, J. Hwang, P. Sikivie, D. B. Tanner, R. Bradley, J. Clarke
Axions in the micro eV mass range are a plausible cold dark matter candidate and may be detected by their conversion into microwave photons in a resonant cavity immersed in a static magnetic field.
Cosmology and Nongalactic Astrophysics
