Zobrazeno 1 - 10
of 169
pro vyhledávání: '"Nichol, B"'
Autor:
Main, D., Drmota, P., Nadlinger, D. P., Ainley, E. M., Agrawal, A., Nichol, B. C., Srinivas, R., Araneda, G., Lucas, D. M.
Distributed quantum computing (DQC) combines the computing power of multiple networked quantum processing modules, enabling the execution of large quantum circuits without compromising on performance and connectivity. Photonic networks are well-suite
Externí odkaz:
http://arxiv.org/abs/2407.00835
Autor:
Drmota, P., Main, D., Ainley, E. M., Agrawal, A., Araneda, G., Nadlinger, D. P., Nichol, B. C., Srinivas, R., Cabello, A., Lucas, D. M.
We report the first experimental demonstration of the odd-cycle game. We entangle two ions separated by ~2 m and the players use them to win the odd-cycle game significantly more often than the best classical strategy allows. The experiment implement
Externí odkaz:
http://arxiv.org/abs/2406.08412
Autor:
Drmota, P., Nadlinger, D. P., Main, D., Nichol, B. C., Ainley, E. M., Leichtle, D., Mantri, A., Kashefi, E., Srinivas, R., Araneda, G., Ballance, C. J., Lucas, D. M.
We report the first hybrid matter-photon implementation of verifiable blind quantum computing. We use a trapped-ion quantum server and a client-side photonic detection system networked via a fibre-optic quantum link. The availability of memory qubits
Externí odkaz:
http://arxiv.org/abs/2305.02936
Autor:
Drmota, P., Main, D., Nadlinger, D. P., Nichol, B. C., Weber, M. A., Ainley, E. M., Agrawal, A., Srinivas, R., Araneda, G., Ballance, C. J., Lucas, D. M.
We integrate a long-lived memory qubit into a mixed-species trapped-ion quantum network node. Ion-photon entanglement first generated with a network qubit in Sr-88 is transferred to Ca-43 with 0.977(7) fidelity, and mapped to a robust memory qubit. W
Externí odkaz:
http://arxiv.org/abs/2210.11447
Autor:
Yu, Zhefu, Martini, Paul, Penton, A., Davis, T. M., Kochanek, C. S., Lewis, G. F., Lidman, C., Malik, U., Sharp, R., Tucker, B. E., Aguena, M., Annis, J., Bertin, E., Bocquet, S., Brooks, D., Rosell, A. Carnero, Carollo, D., Kind, M. Carrasco, Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., García-Bellido, J., Gatti, M., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Mena-Fernández, J., Menanteau, F., Miquel, R., Nichol, B., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Raveri, M., Romer, A. K., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Vincenzi, M., Walker, A. R., Weaverdyck, N.
The correlation between the broad line region radius and continuum luminosity ($R-L$ relation) of active galactic nuclei (AGN) is critical for single-epoch mass estimates of supermassive black holes (SMBHs). At $z \sim 1-2$, where AGN activity peaks,
Externí odkaz:
http://arxiv.org/abs/2208.05491
Autor:
Dixon, M., Lidman, C., Mould, J., Kelsey, L., Brout, D., Möller, A., Wiseman, P., Sullivan, M., Galbany, L., Davis, T. M., Vincenzi, M., Scolnic, D., Lewis, G. F., Smith, M., Kessler, R., Duffy, A., Taylor, E., Flynn, C., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveir, F., Annis, J., Asorey, J., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Rosell, A. Carnero, Carollo, D., Kind, M. Carrasco, Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Doel, P., Everett, S., Ferrero, I., Flaugher, B., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gerdes, D. W., Glazebrook, K., Gruen, D., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Kuehn, K., Kuropatkin, N., Malik, U., March, M., Menanteau, F., Miquel, R., Morgan, R., Nichol, B., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Tarle, G., To, C., Tucker, B. E., Tucker, D. L., Varga, T. N.
We use stacked spectra of the host galaxies of photometrically identified type Ia supernovae (SNe Ia) from the Dark Energy Survey (DES) to search for correlations between Hubble diagram residuals and the spectral properties of the host galaxies. Util
Externí odkaz:
http://arxiv.org/abs/2206.12085
Autor:
Nichol, B. C., Srinivas, R., Nadlinger, D. P., Drmota, P., Main, D., Araneda, G., Ballance, C. J., Lucas, D. M.
Optical atomic clocks are our most precise tools to measure time and frequency. They enable precision frequency comparisons between atoms in separate locations to probe the space-time variation of fundamental constants, the properties of dark matter,
Externí odkaz:
http://arxiv.org/abs/2111.10336
Autor:
Nichol, B., Kemp, E., Wilson, R., Rodrigues, A.M., Hesselgreaves, H., Robson, C., Haighton, C.
Publikováno v:
In Public Health May 2024 230:29-37