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Electromagnetic modeling and science reach of DMRadio-m$^3$

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	DMRadio Collaboration, AlShirawi, A., Ankel, V., Bartram, C., Begin, J., Bell, C., Benabou, J. N., Brouwer, L., Chaudhuri, S., Cho, H. -M., Corbin, J., Craddock, W., Cuadra, S., Droster, A., Echevers, J., Foster, J. W., Fry, J. T., Graham, P. W., Henning, R., Irwin, K. D., Kadribasic, F., Kahn, Y., Keller, A., Kolevatov, R., Kuenstner, S., Kunder, A., Kurita, N., Leder, A. F., Li, D., Otto, N., Ouellet, J. L., Pappas, K. M. W., Phipps, A., Rapidis, N. M., Safdi, B. R., Salemi, C. P., Simanovskaia, M., Singh, J., Stark, P., van Assendelft, E. C., van Bibber, K., Wells, K., Wiedemann, J., Winslow, L., Wisniewski, W. J., Wright, D., Yi, A. K., Young, B. A.
Formato:	Preprint
Publicado:	2023
Materias:	High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology Instrumentation and Detectors
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

_version_	1866915473221746688
author	DMRadio Collaboration AlShirawi, A. Ankel, V. Bartram, C. Begin, J. Bell, C. Benabou, J. N. Brouwer, L. Chaudhuri, S. Cho, H. -M. Corbin, J. Craddock, W. Cuadra, S. Droster, A. Echevers, J. Foster, J. W. Fry, J. T. Graham, P. W. Henning, R. Irwin, K. D. Kadribasic, F. Kahn, Y. Keller, A. Kolevatov, R. Kuenstner, S. Kunder, A. Kurita, N. Leder, A. F. Li, D. Otto, N. Ouellet, J. L. Pappas, K. M. W. Phipps, A. Rapidis, N. M. Safdi, B. R. Salemi, C. P. Simanovskaia, M. Singh, J. Stark, P. van Assendelft, E. C. van Bibber, K. Wells, K. Wiedemann, J. Winslow, L. Wisniewski, W. J. Wright, D. Yi, A. K. Young, B. A.
author_facet	DMRadio Collaboration AlShirawi, A. Ankel, V. Bartram, C. Begin, J. Bell, C. Benabou, J. N. Brouwer, L. Chaudhuri, S. Cho, H. -M. Corbin, J. Craddock, W. Cuadra, S. Droster, A. Echevers, J. Foster, J. W. Fry, J. T. Graham, P. W. Henning, R. Irwin, K. D. Kadribasic, F. Kahn, Y. Keller, A. Kolevatov, R. Kuenstner, S. Kunder, A. Kurita, N. Leder, A. F. Li, D. Otto, N. Ouellet, J. L. Pappas, K. M. W. Phipps, A. Rapidis, N. M. Safdi, B. R. Salemi, C. P. Simanovskaia, M. Singh, J. Stark, P. van Assendelft, E. C. van Bibber, K. Wells, K. Wiedemann, J. Winslow, L. Wisniewski, W. J. Wright, D. Yi, A. K. Young, B. A.
contents	DMRadio-m$^3$ is an experiment that is designed to be sensitive to KSVZ and DFSZ QCD axion models in the 10--200\,MHz (41 neV$/c^2$ -- 0.83 $μ$eV/$c^2$) range. The experiment uses a solenoidal dc magnetic field to convert an axion dark-matter signal to an ac electromagnetic response in a coaxial copper pickup. The current induced by this axion signal is measured by dc SQUIDs. In this work, we present the electromagnetic modeling of the response of the experiment to an axion signal over the full frequency range of DMRadio-m$^3$, which extends from the low-frequency, lumped-element limit to a regime where the axion Compton wavelength is only a factor of two larger than the detector size. With these results, we determine the live time and sensitivity of the experiment. The primary science goal of sensitivity to DFSZ axions across 30--200 MHz can be achieved with a $3σ$ live scan time of 2.9 years.
format	Preprint
id	arxiv_https___arxiv_org_abs_2302_14084
institution	arXiv
publishDate	2023
record_format	arxiv
spellingShingle	Electromagnetic modeling and science reach of DMRadio-m$^3$ DMRadio Collaboration AlShirawi, A. Ankel, V. Bartram, C. Begin, J. Bell, C. Benabou, J. N. Brouwer, L. Chaudhuri, S. Cho, H. -M. Corbin, J. Craddock, W. Cuadra, S. Droster, A. Echevers, J. Foster, J. W. Fry, J. T. Graham, P. W. Henning, R. Irwin, K. D. Kadribasic, F. Kahn, Y. Keller, A. Kolevatov, R. Kuenstner, S. Kunder, A. Kurita, N. Leder, A. F. Li, D. Otto, N. Ouellet, J. L. Pappas, K. M. W. Phipps, A. Rapidis, N. M. Safdi, B. R. Salemi, C. P. Simanovskaia, M. Singh, J. Stark, P. van Assendelft, E. C. van Bibber, K. Wells, K. Wiedemann, J. Winslow, L. Wisniewski, W. J. Wright, D. Yi, A. K. Young, B. A. High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology Instrumentation and Detectors DMRadio-m$^3$ is an experiment that is designed to be sensitive to KSVZ and DFSZ QCD axion models in the 10--200\,MHz (41 neV$/c^2$ -- 0.83 $μ$eV/$c^2$) range. The experiment uses a solenoidal dc magnetic field to convert an axion dark-matter signal to an ac electromagnetic response in a coaxial copper pickup. The current induced by this axion signal is measured by dc SQUIDs. In this work, we present the electromagnetic modeling of the response of the experiment to an axion signal over the full frequency range of DMRadio-m$^3$, which extends from the low-frequency, lumped-element limit to a regime where the axion Compton wavelength is only a factor of two larger than the detector size. With these results, we determine the live time and sensitivity of the experiment. The primary science goal of sensitivity to DFSZ axions across 30--200 MHz can be achieved with a $3σ$ live scan time of 2.9 years.
title	Electromagnetic modeling and science reach of DMRadio-m$^3$
topic	High Energy Physics - Experiment Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology Instrumentation and Detectors
url	https://arxiv.org/abs/2302.14084