Zobrazeno 1 - 10
of 32
pro vyhledávání: '"B H LaRoque"'
Autor:
A Ashtari Esfahani, Z Bogorad, S Böser, N Buzinsky, C Claessens, L de Viveiros, M Fertl, J A Formaggio, L Gladstone, M Grando, M Guigue, J Hartse, K M Heeger, X Huyan, J Johnston, A M Jones, K Kazkaz, B H LaRoque, M Li, A Lindman, C Matthé, R Mohiuddin, B Monreal, J A Nikkel, E Novitski, N S Oblath, J I Peña, W Pettus, R Reimann, R G H Robertson, G Rybka, L Saldaña, M Schram, P L Slocum, J Stachurska, Y-H Sun, P T Surukuchi, A B Telles, F Thomas, M Thomas, T Thümmler, L Tvrznikova, W Van De Pontseele, B A VanDevender, T E Weiss, T Wendler, E Zayas, A Ziegler
Publikováno v:
New Journal of Physics, Vol 24, Iss 5, p 053013 (2022)
Cyclotron radiation emission spectroscopy (CRES) is a modern approach for determining charged particle energies via high-precision frequency measurements of the emitted cyclotron radiation. For CRES experiments with gas within the fiducial volume, si
Externí odkaz:
https://doaj.org/article/5377238c6ee7434eb8106b850d1897bc
Autor:
A Ashtari Esfahani, S Böser, N Buzinsky, R Cervantes, C Claessens, L de Viveiros, M Fertl, J A Formaggio, L Gladstone, M Guigue, K M Heeger, J Johnston, A M Jones, K Kazkaz, B H LaRoque, A Lindman, E Machado, B Monreal, E C Morrison, J A Nikkel, E Novitski, N S Oblath, W Pettus, R G H Robertson, G Rybka, L Saldaña, V Sibille, M Schram, P L Slocum, Y-H Sun, T Thümmler, B A VanDevender, T E Weiss, T Wendler, E Zayas
Publikováno v:
New Journal of Physics, Vol 22, Iss 3, p 033004 (2020)
The cyclotron radiation emission spectroscopy (CRES) technique pioneered by Project 8 measures electromagnetic radiation from individual electrons gyrating in a background magnetic field to construct a highly precise energy spectrum for beta decay st
Externí odkaz:
https://doaj.org/article/54e59a8e97ff4748a02232cfd578aca3
Autor:
A Ashtari Esfahani, S Böser, N Buzinsky, R Cervantes, C Claessens, L de Viveiros, M Fertl, J A Formaggio, L Gladstone, M Guigue, K M Heeger, J Johnston, A M Jones, K Kazkaz, B H LaRoque, A Lindman, E Machado, B Monreal, E C Morrison, J A Nikkel, E Novitski, N S Oblath, W Pettus, R G H Robertson, G Rybka, L Saldaña, V Sibille, M Schram, P L Slocum, Y-H Sun, J R Tedeschi, T Thümmler, B A VanDevender, M Wachtendonk, M Walter, T E Weiss, T Wendler, E Zayas
Publikováno v:
New Journal of Physics, Vol 21, Iss 11, p 113051 (2019)
The Locust simulation package is a new C++ software tool developed to simulate the measurement of time-varying electromagnetic fields using RF detection techniques. Modularity and flexibility allow for arbitrary input signals, while concurrently supp
Externí odkaz:
https://doaj.org/article/4afa1aa1f7784ccb9b2086bfa32e77f2
Autor:
R. Cervantes, G. Carosi, S. Kimes, C. Hanretty, B. H. LaRoque, G. Leum, P. Mohapatra, N. S. Oblath, R. Ottens, Y. Park, G. Rybka, J. Sinnis, J. Yang
Publikováno v:
Physical Review D. 106
Autor:
R. Cervantes, G. Carosi, C. Hanretty, S. Kimes, B. H. LaRoque, G. Leum, P. Mohapatra, N. S. Oblath, R. Ottens, Y. Park, G. Rybka, J. Sinnis, J. Yang
Publikováno v:
Physical Review Letters. 129
Autor:
R. Khatiwada, D. Bowring, A. S. Chou, A. Sonnenschein, W. Wester, D. V. Mitchell, T. Braine, C. Bartram, R. Cervantes, N. Crisosto, N. Du, L. J. Rosenberg, G. Rybka, J. Yang, D. Will, S. Kimes, G. Carosi, N. Woollett, S. Durham, L. D. Duffy, R. Bradley, C. Boutan, M. Jones, B. H. LaRoque, N. S. Oblath, M. S. Taubman, J. Tedeschi, John Clarke, A. Dove, A. Hashim, I. Siddiqi, N. Stevenson, A. Eddins, S. R. O’Kelley, S. Nawaz, A. Agrawal, A. V. Dixit, J. R. Gleason, S. Jois, P. Sikivie, N. S. Sullivan, D. B. Tanner, J. A. Solomon, E. Lentz, E. J. Daw, M. G. Perry, J. H. Buckley, P. M. Harrington, E. A. Henriksen, K. W. Murch, G. C. Hilton
Publikováno v:
The Review of scientific instruments. 92(12)
Axion Dark Matter eXperiment (ADMX) ultra low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in the $2.66$ to $3.1$ $\mu$eV mass range with Dine-Fischler-Srednicki-Z
Autor:
C. Bartram, T. Braine, R. Cervantes, N. Crisosto, N. Du, G. Leum, P. Mohapatra, T. Nitta, L. J. Rosenberg, G. Rybka, J. Yang, John Clarke, I. Siddiqi, A. Agrawal, A. V. Dixit, M. H. Awida, A. S. Chou, M. Hollister, S. Knirck, A. Sonnenschein, W. Wester, J. R. Gleason, A. T. Hipp, S. Jois, P. Sikivie, N. S. Sullivan, D. B. Tanner, E. Lentz, R. Khatiwada, G. Carosi, C. Cisneros, N. Robertson, N. Woollett, L. D. Duffy, C. Boutan, M. Jones, B. H. LaRoque, N. S. Oblath, M. S. Taubman, E. J. Daw, M. G. Perry, J. H. Buckley, C. Gaikwad, J. Hoffman, K. Murch, M. Goryachev, B. T. McAllister, A. Quiskamp, C. Thomson, M. E. Tobar, V. Bolkhovsky, G. Calusine, W. Oliver, K. Serniak
We describe the first implementation of a Josephson Traveling Wave Parametric Amplifier (JTWPA) in an axion dark matter search. The operation of the JTWPA for a period of about two weeks achieved sensitivity to axion-like particle dark matter with ax
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf1603b525907b3210a0bf0581ea0925
http://arxiv.org/abs/2110.10262
http://arxiv.org/abs/2110.10262
Autor:
Sebastian Böser, Gray Rybka, M. Guigue, Walter C. Pettus, R. Cervantes, Malachi Schram, M. Grando, T. Wendler, Mathew Thomas, Kareem Kazkaz, B. H. LaRoque, James Nikkel, M. Ottiger, B.A. VanDevender, Benjamin Monreal, J. Johnston, M. Betancourt, L. Saldaña, R. G. H. Robertson, X. Huyan, Joseph A. Formaggio, Z. Bogorad, A. Ashtari Esfahani, R. Mohiuddin, V. Sibille, L. de Viveiros, E. Zayas, A. Lindman, Martin Fertl, N. Buzinsky, L. Tvrznikova, L. Gladstone, J. Hartse, A. Ziegler, Thomas Thümmler, P. T. Surukuchi, N. S. Oblath, A. B. Telles, C. Claessens, K. M. Heeger, T. E. Weiss, Y. H. Sun, P. L. Slocum, E. Novitski, Jonathan R. Tedeschi, A. M. Jones
Publikováno v:
Physical Review C
Physical Review C, American Physical Society, 2021, 103 (6), pp.065501. ⟨10.1103/PhysRevC.103.065501⟩
Physical Review C, American Physical Society, 2021, 103 (6), pp.065501. ⟨10.1103/PhysRevC.103.065501⟩
Bayesian modeling techniques enable sensitivity analyses that incorporate detailed expectations regarding future experiments. A model-based approach also allows one to evaluate inferences and predicted outcomes, by calibrating (or measuring) the cons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8376a26cd41a9c1628d52cff9ec9806a
http://arxiv.org/abs/2012.14341
http://arxiv.org/abs/2012.14341
Autor:
L. D. Duffy, S. Kimes, Joseph Gleason, A. Eddins, L. J. Rosenberg, Matthew Jones, W. C. Wester, Gray Rybka, J. A. Solomon, Pierre Sikivie, Nathan Woollett, Kater Murch, Jihui Yang, Akash Dixit, B. H. LaRoque, N. S. Oblath, Erik Henriksen, T. Braine, N. Stevenson, E. J. Daw, M. S. Taubman, Andrew Sonnenschein, D. Bowring, Erik W. Lentz, Irfan Siddiqi, N. Du, J. H. Buckley, Gianpaolo Carosi, John Clarke, D. B. Tanner, Aaron S. Chou, Ankur Agrawal, Shahid Nawaz, Allison Dove, N. Crisosto, S. R. O'Kelley, R. Khatiwada, S. Jois, Neil Sullivan, P. M. Harrington, C. Boutan, Richard F. Bradley, R. Cervantes
Publikováno v:
Physical Review Letters
This paper reports on a cavity haloscope search for dark matter axions in the galactic halo in the mass range $2.81$-$3.31$ ${\mu}eV$. This search excludes the full range of axion-photon coupling values predicted in benchmark models of the invisible
Autor:
Pierre Sikivie, R. Cervantes, M. G. Perry, Ankur Agrawal, J. H. Buckley, M. S. Taubman, R. Khatiwada, Allison Dove, Kater Murch, N. Stevenson, Neil Sullivan, E. J. Daw, D. Bowring, S. R. O'Kelley, P. M. Harrington, Maxim Goryachev, Joseph Gleason, Matthew Jones, Ben T. McAllister, N. Crisosto, C. Boutan, W. C. Wester, L. D. Duffy, B. H. LaRoque, Nathan Woollett, N. Du, N. S. Oblath, Aaron S. Chou, A. Eddins, G. Leum, Erik Henriksen, Gray Rybka, L. J. Rosenberg, Chelsea Bartram, John Clarke, S. Jois, Irfan Siddiqi, Akash Dixit, Andrew Sonnenschein, D. B. Tanner, Shahid Nawaz, Jihui Yang, J. A. Solomon, T. Braine, Michael E. Tobar, Erik W. Lentz, Gianpaolo Carosi
Searching for axion dark matter, the ADMX collaboration acquired data from January to October 2018, over the mass range 2.81--3.31 $\mu$eV, corresponding to the frequency range 680--790 MHz. Using an axion haloscope consisting of a microwave cavity i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::517bf7513806fa5788b83dd36f27fd3e