Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Bowring, A"'
Autor:
Bratrud, G., Lewis, S., Anyang, K., Cesaní, A. Colón, Dyson, T., Magoon, H., Sabhari, D., Spahn, G., Wagner, G., Gualtieri, R., Kurinsky, N. A., Linehan, R., McDermott, R., Sussman, S., Temples, D. J., Uemura, S., Bathurst, C., Cancelo, G., Chen, R., Chou, A., Hernandez, I., Hollister, M., Hsu, L., James, C., Kennard, K., Khatiwada, R., Lukens, P., Novati, V., Raha, N., Ray, S., Ren, R., Rodriguez, A., Schmidt, B., Stifter, K., Yu, J., Baxter, D., Figueroa-Feliciano, E., Bowring, D.
We measure space- and time-correlated charge jumps on a four-qubit device, operating 107 meters below the Earth's surface in a low-radiation, cryogenic facility designed for the characterization of low-threshold particle detectors. The rock overburde
Externí odkaz:
http://arxiv.org/abs/2405.04642
Autor:
Stifter, K., Magoon, H., Anderson, A. J., Temples, D. J., Kurinsky, N. A., Stoughton, C., Hernandez, I., Nuñez, A., Anyang, K., Linehan, R., Young, M. R., Barry, P., Baxter, D., Bowring, D., Cancelo, G., Chou, A., Dibert, K. R., Figueroa-Feliciano, E., Hsu, L., Khatiwada, R., Mork, S. D., Stefanazzi, L., Tabassum, N., Uemura, S., Young, B. A.
We have developed a calibration system based on a micro-electromechanical systems (MEMS) mirror that is capable of delivering an optical beam over a wavelength range of 180 -- 2000 nm (0.62 -- 6.89 eV) in a sub-Kelvin environment. This portable, inte
Externí odkaz:
http://arxiv.org/abs/2405.02258
Autor:
Linehan, R., Hernandez, I., Temples, D. J., Dang, S. Q., Baxter, D., Hsu, L., Figueroa-Feliciano, E., Khatiwada, R., Anyang, K., Bowring, D., Bratrud, G., Cancelo, G., Chou, A., Gualtieri, R., Stifter, K., Sussman, S.
In recent years, the lack of a conclusive detection of WIMP dark matter at the 10 GeV/c$^{2}$ mass scale and above has encouraged development of low-threshold detector technology aimed at probing lighter dark matter candidates. Detectors based on Coo
Externí odkaz:
http://arxiv.org/abs/2404.04423
Autor:
Temples, Dylan J, Wen, Osmond, Ramanathan, Karthik, Aralis, Taylor, Chang, Yen-Yung, Golwala, Sunil, Hsu, Lauren, Bathurst, Corey, Baxter, Daniel, Bowring, Daniel, Chen, Ran, Figueroa-Feliciano, Enectali, Hollister, Matthew, James, Christopher, Kennard, Kyle, Kurinsky, Noah, Lewis, Samantha, Lukens, Patrick, Novati, Valentina, Ren, Runze, Schmidt, Benjamin
Microcalorimeters that leverage microwave kinetic inductance detectors to read out phonon signals in the particle-absorbing target, referred to as kinetic inductance phonon-mediated (KIPM) detectors, offer an attractive detector architecture to probe
Externí odkaz:
http://arxiv.org/abs/2402.04473
Autor:
Boutan, C., LaRoque, B. H., Lentz, E., Oblath, N. S., Taubman, M. S., Tedeschi, J., Yang, J., Jones, A. M., Braine, T., Crisosto, N., Rosenberg, L. J, Rybka, G., Will, D., Zhang, D., Kimes, S., Ottens, R., Bartram, C., Bowring, D., Cervantes, R., Chou, A. S., Knirck, S., Mitchell, D. V., Sonnenschein, A., Wester, W., Khatiwada, R., Carosi, G., Du, N., Durham, S., O'Kelley, S. R., Woollett, N., Duffy, L. D., Bradley, R., Clarke, J., Siddiqi, I., Agrawal, A., Dixit, A. V., Gleason, J. R., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Buckley, J. H., Gaikwad, C., Henriksen, E. A., Hoffman, J., Murch, K. W., Harrington, P. M., Daw, E. J., Perry, M. G., Hilton, G. C.
The ADMX collaboration gathered data for its Run 1A axion dark matter search from January to June 2017, scanning with an axion haloscope over the frequency range 645-680 MHz (2.66-2.81 ueV in axion mass) at DFSZ sensitivity. The resulting axion searc
Externí odkaz:
http://arxiv.org/abs/2312.16668
Autor:
Bartram, C., Braine, T., Cervantes, R., Crisosto, N., Du, N., Goodman, C., Guzzetti, M., Hanretty, C., Lee, S., Leum, G., Rosenberg, L. J., Rybka, G., Sinnis, J., Zhang, D., Awida, M. H., Bowring, D., Chou, A. S., Hollister, M., Knirck, S., Sonnenschein, A., Wester, W., Khatiwada, R., Brodsky, J., Carosi, G., Duffy, L. D., Goryachev, M., McAllister, B., Quiskamp, A., Thomson, C., Tobar, M. E., Boutan, C., Jones, M., LaRoque, B. H., Lentz, E., Man, N. E., Oblath, N. S., Taubman, M. S., Yang, J., Clarke, John, Siddiqi, I., Agrawal, A., Dixit, A. V., Gleason, J. R., Han, Y., Hipp, A. T., Jois, S., Sikivie, P., Sullivan, N. S., Tanner, D. B., Daw, E. J., Perry, M. G., Buckley, J. H., Gaikwad, C., Hoffman, J., Murch, K. W., Russell, J.
The Axion Dark Matter eXperiment (ADMX) has previously excluded Dine-Fischler-Srednicki-Zhitnisky (DFSZ) axions between 680-790 MHz under the assumption that the dark matter is described by the isothermal halo model. However, the precise nature of th
Externí odkaz:
http://arxiv.org/abs/2311.07748
Autor:
Knirck, Stefan, Hoshino, Gabe, Awida, Mohamed H., Cancelo, Gustavo I., Di Federico, Martin, Knepper, Benjamin, Lapuente, Alex, Littmann, Mira, Miller, David W., Mitchell, Donald V., Rodriguez, Derrick, Ruschman, Mark K., Sawtell, Matthew A., Stefanazzi, Leandro, Sonnenschein, Andrew, Teafoe, Gary W., Bowring, Daniel, Carosi, G., Chou, Aaron, Chang, Clarence L., Dona, Kristin, Khatiwada, Rakshya, Kurinsky, Noah A., Liu, Jesse, Pena, Cristián, Salemi, Chiara P., Wang, Christina W., Yu, Jialin
Publikováno v:
Phys. Rev. Lett. 132, 131004 (2024)
We present first results from a dark photon dark matter search in the mass range from 44 to 52 $\mu{\rm eV}$ ($10.7 - 12.5\,{\rm GHz}$) using a room-temperature dish antenna setup called GigaBREAD. Dark photon dark matter converts to ordinary photons
Externí odkaz:
http://arxiv.org/abs/2310.13891
Autor:
The MICE Collaboration, Bogomilov, M., Tsenov, R., Vankova-Kirilova, G., Song, Y. P., Tang, J. Y., Li, Z. H., Bertoni, R., Bonesini, M., Chignoli, F., Mazza, R., de Bari, A., Orestano, D., Tortora, L., Kuno, Y., Sakamoto, H., Sato, A., Ishimoto, S., Chung, M., Sung, C. K., Filthaut, F., Fedorov, M., Jokovic, D., Maletic, D., Savic, M., Jovancevic, N., Nikolov, J., Vretenar, M., Ramberger, S., Asfandiyarov, R., Blondel, A., Drielsma, F., Karadzhov, Y., Boyd, S., Greis, J. R., Lord, T., Pidcott, C., Taylor, I., Charnley, G., Collomb, N., Dumbell, K., Gallagher, A., Grant, A., Griffiths, S., Hartnett, T., Martlew, B., Moss, A., Muir, A., Mullacrane, I., Oates, A., Owens, P., Stokes, G., Warburton, P., White, C., Adams, D., Bayliss, V., Boehm, J., Bradshaw, T. W., Brown, C., Courthold, M., Govans, J., Hayler, T., Hills, M., Lagrange, J. B., Macwaters, C., Nichols, A., Preece, R., Ricciardi, S., Rogers, C., Stanley, T., Tarrant, J., Tucker, M., Watson, S., Wilson, A., Bayes, R., Nugent, J. C., Soler, F. J. P., Chatzitheodoridis, G. T., Dick, A. J., Ronald, K., Whyte, C. G., Young, A. R., Gamet, R., Cooke, P., Blackmore, V. J., Colling, D., Dobbs, A., Dornan, P., Franchini, P., Hunt, C., Jurj, P. B., Kurup, A., Long, K., Martyniak, J., Middleton, S., Pasternak, J., Uchida, M. A., Cobb, J. H., Booth, C. N., Hodgson, P., Langlands, J., Overton, E., Pec, V., Smith, P. J., Wilbur, S., Ellis, M., Gardener, R. B. S., Kyberd, P., Nebrensky, J. J., DeMello, A., Gourlay, S., Lambert, A., Li, D., Luo, T., Prestemon, S., Virostek, S., Palmer, M., Witte, H., Adey, D., Bross, A. D., Bowring, D., Liu, A., Neuffer, D., Popovic, M., Rubinov, P., Freemire, B., Hanlet, P., Kaplan, D. M., Mohayai, T. A., Rajaram, D., Snopok, P., Torun, Y., Cremaldi, L. M., Sanders, D. A., Coney, L. R., Hanson, G. G., Heidt, C.
Accelerated muon beams have been considered for next-generation studies of high-energy lepton-antilepton collisions and neutrino oscillations. However, high-brightness muon beams have not yet been produced. The main challenge for muon acceleration an
Externí odkaz:
http://arxiv.org/abs/2310.05669
Autor:
Bogomilov, M., Tsenov, R., Vankova-Kirilova, G., Song, Y. P., Tang, J. Y., Li, Z. H., Bertoni, R., Bonesini, M., Chignoli, F., Mazza, R., Palladino, V., de Bari, A., Orestano, D., Tortora, L., Kuno, Y., Sakamoto, H., Sato, A., Ishimoto, S., Chung, M., Sung, C. K., Filthaut, F., Fedorov, M., Jokovic, D., Maletic, D., Savic, M., Jovancevic, N., Nikolov, J., Vretenar, M., Ramberger, S., Asfandiyarov, R., Blondel, A., Drielsma, F., Karadzhov, Y., Charnley, G., Collomb, N., Dumbell, K., Gallagher, A., Grant, A., Griffiths, S., Hartnett, T., Martlew, B., Moss, A., Muir, A., Mullacrane, I., Oates, A., Owens, P., Stokes, G., Warburton, P., White, C., Adams, D., Bayliss, V., Boehm, J., Bradshaw, T. W., Brown, C., Courthold, M., Govans, J., Hills, M., Lagrange, J. -B., Macwaters, C., Nichols, A., Preece, R., Ricciardi, S., Rogers, C., Stanley, T., Tarrant, J., Tucker, M., Watson, S., Wilson, A., Bayes, R., Nugent, J. C., Soler, F. J. P., Gamet, R., Cooke, P., Blackmore, V. J., Colling, D., Dobbs, A., Dornan, P., Franchini, P., Hunt, C., Jurj, P. B., Kurup, A., Long, K., Martyniak, J., Middleton, S., Pasternak, J., Uchida, M. A., Cobb, J. H., Booth, C. N., Hodgson, P., Langlands, J., Overton, E., Pec, V., Smith, P. J., Wilbur, S., Chatzitheodoridis, G. T., Dick, A. J., Ronald, K., Whyte, C. G., Young, A. R., Boyd, S., Greis, J. R., Lord, T., Pidcott, C., Taylor, I., Ellis, M., Gardener, R. B. S., Kyberd, P., Nebrensky, J. J., Palmer, M., Witte, H., Adey, D., Bross, A. D., Bowring, D., Hanlet, P., Liu, A., Neuffer, D., Popovic, M., Rubinov, P., DeMello, A., Gourlay, S., Lambert, A., Li, D., Luo, T., Prestemon, S., Virostek, S., Freemire, B., Kaplan, D. M., Mohayai, T. A., Rajaram, D., Snopok, P., Torun, Y., Cremaldi, L. M., Sanders, D. A., Summers, D. J., Coney, L. R., Hanson, G. G., Heidt, C.
Multiple Coulomb Scattering (MCS) is a well known phenomenon occurring when charged particles traverse materials. Measurements of muons traversing low $Z$ materials made in the MuScat experiment showed that theoretical models and simulation codes, su
Externí odkaz:
http://arxiv.org/abs/2209.10251
Autor:
Adams, C. B., Aggarwal, N., Agrawal, A., Balafendiev, R., Bartram, C., Baryakhtar, M., Bekker, H., Belov, P., Berggren, K. K., Berlin, A., Boutan, C., Bowring, D., Budker, D., Caldwell, A., Carenza, P., Carosi, G., Cervantes, R., Chakrabarty, S. S., Chaudhuri, S., Chen, T. Y., Cheong, S., Chou, A., Co, R. T., Conrad, J., Croon, D., D'Agnolo, R. T., Demarteau, M., DePorzio, N., Descalle, M., Desch, K., Di Luzio, L., Diaz-Morcillo, A., Dona, K., Drachnev, I. S., Droster, A., Du, N., Dunne, K., Döbrich, B., Ellis, S. A. R., Essig, R., Fan, J., Foster, J. W., Fry, J. T., Rosso, A. Gallo, Barceló, J. M. García, Irastorza, I. G., Gardner, S., Geraci, A. A., Ghosh, S., Giaccone, B., Giannotti, M., Gimeno, B., Grin, D., Grote, H., Guzzetti, M., Awida, M. H., Henning, R., Hoof, S., Hoshino, G., Irsic, V., Irwin, K. D., Jackson, H., Kimball, D. F. Jackson, Jaeckel, J., Jakovcic, K., Jewell, M. J., Kagan, M., Kahn, Y., Khatiwada, R., Knirck, S., Kovachy, T., Krueger, P., Kuenstner, S. E., Kurinsky, N. A., Leane, R. K., Leder, A. F., Lee, C., Lehnert, K. W., Lentz, E. W., Lewis, S. M., Liu, J., Lynn, M., Majorovits, B., Marsh, D. J. E., Maruyama, R. H., McAllister, B. T., Millar, A. J., Miller, D. W., Mitchell, J., Morampudi, S., Mueller, G., Nagaitsev, S., Nardi, E., Noroozian, O., O'Hare, C. A. J., Oblath, N. S., Ouellet, J. L., Pappas, K. M. W., Peiris, H. V., Perez, K., Phipps, A., Pivovaroff, M. J., Quílez, P., Rapidis, N. M., Robles, V. H., Rogers, K. K., Rudolph, J., Ruz, J., Rybka, G., Safdari, M., Safdi, B. R., Safronova, M. S., Salemi, C. P., Schuster, P., Schwartzman, A., Shu, J., Simanovskaia, M., Singh, J., Singh, S., Sinha, K., Sinnis, J. T., Siodlaczek, M., Smith, M. S., Snow, W. M., Sokolov, A. V., Sonnenschein, A., Speller, D. H., Stadnik, Y. V., Sun, C., Sushkov, A. O., Tait, T. M. P., Takhistov, V., Tanner, D. B., Tavecchio, F., Temples, D. J., Thomas, J. H., Tobar, M. E., Toro, N., Tsai, Y. -D., van Assendelft, E. C., van Bibber, K., Vandegar, M., Visinelli, L., Vitagliano, E., Vogel, J. K., Wang, Z., Wickenbrock, A., Winslow, L., Withington, S., Wooten, M., Yang, J., Young, B. A., Yu, F., Zhou, K., Zhou, T.
Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This Snowmass white p
Externí odkaz:
http://arxiv.org/abs/2203.14923