Zobrazeno 1 - 10
of 1 696
pro vyhledávání: '"Howard, A B"'
Autor:
Patel, D., Cuong, D. C., Howard, K. B., Garg, U., Khoa, Dao T., Akimune, H., Berg, G. P. A., Fujiwara, M., Harakeh, M. N., Itoh, M., Iwamoto, C., Kawabata, T., Kawase, K., Matta, J. T., Murakami, T., Yosoi, M.
Publikováno v:
Phys. Rec. C 110, 044314 (2024)
Angular distributions of the elastic and inelastic deuteron-nucleus scattering off $^{24}$Mg, $^{28}$Si, $^{58}$Ni, $^{90}$Zr, $^{116}$Sn, and $^{208}$Pb have been measured at a beam energy of 98 MeV/nucleon, with the goal of constraining the deutero
Externí odkaz:
http://arxiv.org/abs/2409.08517
Autor:
Abdullah, M., Bagchi, S., Harakeh, M. N., Akimune, H., Das, D., Doi, T., Donaldson, L. M., Fujikawa, Y., Fujiwara, M., Furuno, T., Garg, U., Gupta, Y. K., Howard, K. B., Hijikata, Y., Inaba, K., Ishida, S., Itoh, M., Kalantar-Nayestanaki, N., Kar, D., Kawabata, T., Kawashima, S., Khokhar, K., Kitamura, K., Kobayashi, N., Matsuda, Y., Nakagawa, A., Nakamura, S., Nosaka, K., Okamoto, S., Ota, S., Pal, S., Pramanik, R., Roy, S., Weyhmiller, S., Yang, Z., Zamora, J. C.
The strength distributions of the Isoscalar Giant Monopole Resonance (ISGMR) and Isoscalar Giant Quadrupole Resonance (ISGQR) in 142,146-150Nd have been determined via inelastic alpha-particle scattering with the Grand Raiden (GR) Spectrometer at the
Externí odkaz:
http://arxiv.org/abs/2407.05685
Autor:
Sensharma, N., Garg, U., Chen, Q. B., Frauendorf, S., Zhu, S., Arroyo, J., Ayangeakaa, A. D., Burdette, D. P., Carpenter, M. P., Copp, P., Cozzi, J. L., Ghugre, S. S., Hartley, D. J., Howard, K. B., Janssens, R. V. F., Kondev, F. G., Lauritsen, T., Li, J., Palit, R., Saracino, A., Seweryniak, D., Weyhmiller, S., Wu, J.
Chirality is a distinct signature that characterizes triaxial shapes in nuclei. We report the first observation of chirality in the nucleus $^{135}$Pr using a high-statistics Gammasphere experiment with the $^{123}$Sb($^{16}$O,4n)$^{135}$Pr reaction.
Externí odkaz:
http://arxiv.org/abs/2403.10749
Autor:
Wang, Yachun, Howard, Cameron B., Xu, Fei, Salvato, Daniele, Bawane, Kaustubh K., Murray, Daniel J., Frazer, David M., Anderson, Scott T., Yao, Tiankai, Yeo, Sunghwan, Kim, June-Hyung, Lee, Byoung-Oon, Kim, Jun Hwan, Fielding, Randall S., Capriotti, Luca
Publikováno v:
In Journal of Nuclear Materials October 2024 599
Autor:
Johnston, Ryan A., Habarugira, Gervais, Harrison, Jessica J., Isberg, Sally R., Moran, Jasmin, Morgan, Mahali S., Davis, Steven S., Melville, Lorna, Howard, Christopher B., Henry, Charles S., Macdonald, Joanne, Bielefeldt-Ohmann, Helle, Hall, Roy A., Hobson-Peters, Jody
Publikováno v:
In Sensors and Actuators: B. Chemical 1 January 2025 422
Autor:
Rona, Gergely, Miwatani-Minter, Bearach, Zhang, Qingyue, Goldberg, Hailey V., Kerzhnerman, Marc A., Howard, Jesse B., Simoneschi, Daniele, Lane, Ethan, Hobbs, John W., Sassani, Elizabeth, Wang, Andrew A., Keegan, Sarah, Laverty, Daniel J., Piett, Cortt G., Pongor, Lorinc S., Xu, Miranda Li, Andrade, Joshua, Thomas, Anish, Sicinski, Piotr, Askenazi, Manor, Ueberheide, Beatrix, Fenyö, David, Nagel, Zachary D., Pagano, Michele
Publikováno v:
In Molecular Cell 4 April 2024 84(7):1224-1242
Autor:
Logan, Amy, Howard, Christopher B., Huda, Pie, Kimpton, Kathleen, Ma, Zerong, Thurecht, Kristofer J., McCarroll, Joshua A., Moles, Ernest, Kavallaris, Maria
Publikováno v:
In Journal of Controlled Release March 2024 367:806-820
Publikováno v:
In Biophysical Journal 20 February 2024 123(4):502-508
Autor:
Frentz, B., Aprahamian, A., Clark, A. M., Dulal, C., Enright, J. D., deBoer, R. J., Görres, J., Henderson, S. L., Howard, K. B., Kelmar, R., Lee, K., Morales, L., Moylan, S., Raman, Z., Tan, W., Weghorn, L. E., Wiescher, M.
Publikováno v:
Phys. Rev. C 103, 045802 (2021)
The CNO cycle is the main energy source in stars more massive than our sun, it defines the energy production and the cycle time that lead to the lifetime of massive stars, and it is an important tool for the determination of the age of globular clust
Externí odkaz:
http://arxiv.org/abs/2012.13029
Autor:
Howard, K. B., Garg, U., Itoh, M., Akimune, H., Fujiwara, M., Furuno, T., Gupta, Y. K., Harakeh, M. N., Inaba, K., Ishibashi, Y., Karasudani, K., Kawabata, T., Kohda, A., Matsuda, Y., Murata, M., Nakamura, S., Okamoto, J., Ota, S., Piekarewicz, J., Sakaue, A., Senyigit, M., Tsumura, M., Yang, Y.
Publikováno v:
Phys. Lett. B 807 (2020) 135608
"Why are the tin isotopes soft?" has remained, for the past decade, an open problem in nuclear structure physics: models which reproduce the isoscalar giant monopole resonance (ISGMR) in the "doubly-closed shell" nuclei, $^{90}$Zr and $^{208}$Pb, ove
Externí odkaz:
http://arxiv.org/abs/2005.10172