Zobrazeno 1 - 10
of 4 275
pro vyhledávání: '"Jones, K P"'
Publikováno v:
Opt. Express 32, 23812-23821 (2024)
We construct a phase-conjugate resonator which passively produces stable pulses that alternate between the probe and the conjugate colors. The requisite phase-conjugate mirror inside the resonator is constructed using non-degenerate four-wave mixing
Externí odkaz:
http://arxiv.org/abs/2406.11071
Publikováno v:
Front. Phys. 11:1242668 (2023)
The structure of the unbound nucleus $^{13}$Be is important to understanding the Borromean, two-neutron halo nucleus $^{14}$Be. The experimental studies conducted over the last four decades are reviewed in the context of the beryllium chain of isotop
Externí odkaz:
http://arxiv.org/abs/2309.10086
Autor:
Kovoor, J., Jones, K. L., Hooker, J., Vostinar, M., Kanungo, R., Pain, S. D., Alcorta, M., Allen, J., Andreoiu, C., Atar, L., Bardayan, D. W., Bhattacharjee, S. S., Blankstein, D., Burbadge, C., Burcher, S., Catford, W. N., Cha, S., Chae, K., Connolly, D., Davids, B., Esker, N. E., Garcia, F. H., Gillespie, S., Ghimire, R., Gula, A., Hackman, G., Hallam, S., Hellmich, M., Henderson, J., Holl, M., Jassal, P., King, S., Knight, T., Kruecken, R., Lepailleur, A., Liang, J., Morrison, L., O'Malley, P. D., Pereira-Lopez, X., Psaltis, A., Radich, A., Refsgaard, J., Shotter, A. C., Williams, M., Workman, O.
Publikováno v:
Phys. Rev. C108, 034601 (2023)
The low-lying structure of $^{13}$Be has remained an enigma for decades. Despite numerous experimental and theoretical studies, large inconsistencies remain. Being both unbound, and one neutron away from $^{14}$Be, the heaviest bound beryllium nucleu
Externí odkaz:
http://arxiv.org/abs/2309.08692
Autor:
Valdés, E. A. Meier, Morris, B. M., Demory, B. -O., Brandeker, A., Kitzmann, D., Benz, W., Deline, A., Florén, H. -G., Sousa, S. G., Bourrier, V., Singh, V., Heng, K., Strugarek, A., Bower, D. J., Jäggi, N., Carone, L., Lendl, M., Jones, K., Oza, A. V., Demangeon, O. D. S., Alibert, Y., Alonso, R., Anglada, G., Asquier, J., Bárczy, T., Navascues, D. Barrado, Barros, S. C. C., Baumjohann, W., Beck, M., Beck, T., Billot, N., Bonfils, X., Borsato, L., Broeg, C., Cabrera, J., Charnoz, S., Cameron, A. Collier, Csizmadia, Sz., Cubillos, P. E., Davies, M. B., Deleuil, M., Delrez, L., Ehrenreich, D., Erikson, A., Fortier, A., Fossati, L., Fridlund, M., Gandolfi, D., Gillon, M., Güdel, M., Günther, M. N., Hoyer, S., Isaak, K. G., Kiss, L. L., Laskar, J., Etangs, A. Lecavelier des, Lovis, C., Magrin, D., Maxted, P. F. L., Mordasini, C., Nascimbeni, V., Olofsson, G., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Santos, N. C., Sarajlic, M., Scandariato, G., Ségransan, D., Sicilia, D., Simon, A. E., Smith, A. M. S., Steller, M., Szabó, Gy. M., Thomas, N., Udry, S., Ulmer, B., Van Grootel, V., Venturini, J., Walton, N. A., Wilson, T. G., Wolter, D.
Publikováno v:
A&A 677, A112 (2023)
55 Cnc e is an ultra-short period super-Earth transiting a Sun-like star. Previous observations in the optical range detected a time-variable flux modulation that is phased with the planetary orbital period, whose amplitude is too large to be explain
Externí odkaz:
http://arxiv.org/abs/2307.06085
Autor:
Browne, J., Chipps, K. A., Schmidt, K., Schatz, H., Ahn, S., Pain, S. D., Montes, F., Ong, W. J., Greife, U., Allen, J., Bardayan, D. W., Blackmon, J. C., Blankstein, D., Cha, S., Chae, K. Y., Febbraro, M., Hall, M. R., Jones, K. L., Kontos, A., Meisel, Z., O'Malley, P. D., Schmitt, K. T., Smith, K., Smith, M. S., Thompson, P., Toomey, R., Vostinar, M., Walter, D.
Publikováno v:
Phys. Rev. Lett. 130 (2023) 212701
The rate of the final step in the astrophysical $\alpha$p-process, the $^{34}$Ar($\alpha$,\textit{p})$^{37}$K reaction, suffers from large uncertainties due to lack of experimental data, despite having a considerable impact on the observable light cu
Externí odkaz:
http://arxiv.org/abs/2305.19422
Autor:
Misch, G. W., Mumpower, M. R., Kondev, F. G., Marley, S. T., Almaraz-Calderon, S., Brodeur, M., Brown, B. A., Carpenter, M. P., Carroll, J. J., Chiara, C. J., Chipps, K. A., Crider, B. P., Gade, A., Grzywacz, R., Jones, K. L., Kay, B. P., Kolos, K., Litvinov, Yu. A., Lopez-Caceres, S., Meyer, B. S., Minamisono, K., Morgan, G. E., Orford, R., Pain, S. D., Purcell, J., Ratkiewicz, A., Schatz, H., Sprouse, T. M., Sun, Y., Surman, R., Tannous, J. A., Walker, P. M.
We report on the Facility for Rare Isotope Beams (FRIB) Theory Alliance topical program "Nuclear Isomers in the Era of FRIB". We outline the many ways isomers influence and contribute to nuclear science and technology, especially in the four FRIB pil
Externí odkaz:
http://arxiv.org/abs/2304.10608
Autor:
Borsato, N. W., Hoeijmakers, H. J., Prinoth, B., Thorsbro, B., Forsberg, R., Kitzmann, D., Jones, K., Heng, K.
Publikováno v:
A&A 673, A158 (2023)
Cross-correlation spectroscopy is an invaluable tool in the study of exoplanets. However, aliasing between spectral lines makes it vulnerable to systematic biases. This work strives to constrain the aliases of the cross-correlation function to provid
Externí odkaz:
http://arxiv.org/abs/2304.04285
Autor:
Harre, J. -V., Smith, A. M. S., Barros, S. C. C., Boué, G., Csizmadia, Sz., Ehrenreich, D., Florén, H. -G., Fortier, A., Maxted, P. F. L., Hooton, M. J., Akinsanmi, B., Serrano, L. M., Rosário, N. M., Demory, B. -O., Jones, K., Laskar, J., Adibekyan, V., Alibert, Y., Alonso, R., Anderson, D. R., Anglada, G., Asquier, J., Bárczy, T., Navascues, D. Barrado y, Baumjohann, W., Beck, M., Beck, T., Benz, W., Billot, N., Biondi, F., Bonfanti, A., Bonfils, X., Brandeker, A., Broeg, C., Cabrera, J., Cessa, V., Charnoz, S., Cameron, A. Collier, Davies, M. B., Deleuil, M., Delrez, L., Demangeon, O. D. S., Erikson, A., Fossati, L., Fridlund, M., Gandolfi, D., Gillon, M., Güdel, M., Hellier, C., Heng, K., Hoyer, S., Isaak, K. G., Kiss, L. L., Etangs, A. Lecavelier des, Lendl, M., Lovis, C., Luntzer, A., Magrin, D., Nascimbeni, V., Olofsson, G., Ottensamer, R., Pagano, I., Pallé, E., Persson, C. M., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Ricker, G. R., Salmon, S., Santos, N. C., Scandariato, G., Seager, S., Ségransan, D., Simon, A. E., Sousa, S. G., Steller, M., Szabó, Gy. M., Thomas, N., Udry, S., Ulmer, B., Van Grootel, V., Walton, N. A., Wilson, T. G., Winn, J. N., Wohler, B.
Publikováno v:
A&A 669, A124 (2023)
Tidal orbital decay is suspected to occur especially for hot Jupiters, with the only observationally confirmed case of this being WASP-12 b. By examining this effect, information on the properties of the host star can be obtained using the so-called
Externí odkaz:
http://arxiv.org/abs/2211.05646
Autor:
Jones, K. D., Morris, B. M., Demory, B. -O., Heng, K., Hooton, M. J., Billot, N., Ehrenreich, D., Hoyer, S., Simon, A. E., Lendl, M., Demangeon, O. D. S., Sousa, S. G., Bonfanti, A., Wilson, T. G., Salmon, S., Csizmadia, Sz., Parviainen, H., Bruno, G., Alibert, Y., Alonso, R., Anglada, G., Bárczy, T., Navascues, D. Barrado y, Barros, S. C. C., Baumjohann, W., Beck, M., Beck, T., Benz, W., Bonfils, X., Brandeker, A., Broeg, C., Cabrera, J., Charnoz, S., Cameron, A. Collier, Davies, M. B., Deleuil, M., Deline, A., Delrez, L., Erikson, A., Fortier, A., Fossati, L., Fridlund, M., Gandolfi, D., Gillon, M., Güdel, M., Isaak, K. G., Kiss, L. L., Laskar, J., Etangs, A. Lecavelier des, Lovis, C., Magrin, D., Maxted, P. F. L., Nascimbeni, V., Olofsson, G., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Ratti, F., Rauer, H., Reimers, C., Ribas, I., Santos, N. C., Scandariato, G., Ségransan, D., Smith, A. M. S., Steller, M., Szabó, Gy. M., Thomas, N., Udry, S., Van Grootel, V., Walter, I., Walton, N. A., Jungo, W. Wang
Publikováno v:
A&A 666, A118 (2022)
Even among the most irradiated gas giants, so-called ultra-hot Jupiters, KELT-9b stands out as the hottest planet thus far discovered with a dayside temperature of over 4500K. At these extreme irradiation levels, we expect an increase in heat redistr
Externí odkaz:
http://arxiv.org/abs/2208.04818
Autor:
Jones, K. L., Bey, A., Burcher, S., Allmond, J. M., Galindo-Uribarri, A., Radford, D. C., Ahn, S., Ayres, A., Bardayan, 1 D. W., Cizewski, J. A., Ruiz, R. F. Garcia, Howard, M. E., Kozub, R. L., Liang, J. F., Manning, B., Matos, M., Nesaraja, C. D., O'Malley, P. D., Padilla-Rodal, E., Pain, S. D., Pittman, S. T., Ratkiewicz, A., Schmitt, K. T., Smith, M. S., Stracener, D. W., Varner, R. L.
The structure of nuclei around the neutron-rich nucleus 132Sn is of particular interest due to the vicinity of the Z = 50 and N = 82 shell closures and the r-process nucleosynthetic path. Four states in 131Sn with a strong single-particle-like compon
Externí odkaz:
http://arxiv.org/abs/2201.08890