Zobrazeno 1 - 10
of 75
pro vyhledávání: '"Paneru, S."'
Autor:
Paneru, S. N., Brown, K. W., Teh, F. C. E, Zhu, K., Tsang, M. B., DellAquila, D., Chajecki, Z., Lynch, W. G., Sweany, S., Tsang, C. Y., Anthony, A. K., Barney, J., Estee, J., Gasparic, I., Jhang, G., Khanal, O. B., Mandredi, J., Niu, C. Y., Wang, R. S., Zamora, J. C.
Understanding the neutron background is essential for determining the neutron yield from nuclear reactions. In the analysis presented here, the shadow bars are placed in front of neutron detectors to determine the energy dependent neutron background
Externí odkaz:
http://arxiv.org/abs/2212.11093
Autor:
Paneru, S. N., Brune, C. R., Connolly, D., Odell, D., Poudel, M., Phillips, D. R., Karpesky, J., Davids, B., Ruiz, C., Lennarz, A., Greife, U., Alcorta, M., Giri, R., Lovely, M., Bowry, M., Delgado, M., Esker, N. E., Garnsworthy, A., Seeman, C., Machule, P., Fallis, J., Chen, A. A., Laddaran, F., Firmino, A., Weinerman, C.
Measurements of the elastic scattering cross section of 3He and 4He are important in order to improve constraints on theoretical models of 4He(3He,g)7Be, a key reaction in Big Bang nucleosynthesis and solar neutrino production. The astrophysical S-fa
Externí odkaz:
http://arxiv.org/abs/2211.14641
Autor:
Psaltis, A., Chen, A. A., Longland, R., Connolly, D. S., Brune, C. R., Davids, B., Fallis, J., Giri, R., Greife, U, Hutcheon, D. A., Kroll, L., Lennarz, A., Liang, J., Lovely, M., Luo, M., Marshall, C., Paneru, S. N., Parikh, A., Ruiz, C., Shotter, A. C., Williams, M.
A possible mechanism to explain the origin of the light $p$-nuclei in the Galaxy is the nucleosynthesis in the proton-rich neutrino-driven wind ejecta of core-collapse supernovae via the $\nu p$-process. However this production scenario is very sensi
Externí odkaz:
http://arxiv.org/abs/2209.06472
Autor:
Psaltis, A., Chen, A. A., Longland, R., Connolly, D. S., Brune, C. R., Davids, B., Fallis, J., Giri, R., Greife, U, Hutcheon, D. A., Kroll, L., Lennarz, A., Liang, J., Lovely, M., Luo, M., Marshall, C., Paneru, S. N., Parikh, A., Ruiz, C., Shotter, A. C., Williams, M.
We have performed the first direct measurement of two resonances of the $^7$Be($\alpha,\gamma$)$^{11}$C reaction with unknown strengths using an intense radioactive $^7$Be beam and the DRAGON recoil separator. We report on the first measurement of th
Externí odkaz:
http://arxiv.org/abs/2209.06465
Autor:
Ayyad, Y., Mittig, W., Tang, T., Olaizola, B., Potel, G., Rijal, N., Watwood, N., Alvarez-Pol, H., Bazin, D., Caamaño, M., Chen, J., Cortesi, M., Fernández-Domínguez, B., Giraud, S., Gueye, P., Heinitz, S., Jain, R., Kay, B. P., Maugeri, E. A., Monteagudo, B., Ndayisabye, F., Paneru, S. N., Pereira, J., Rubino, E., Santamaria, C., Schumann, D., Surbrook, J., Wagner, L., Zamora, J. C., Zelevinsky, V.
A narrow near-threshold proton-emitting resonance (Ex = 11.4 MeV, J$^{\pi}$ = 1/2$^{+}$ and $\Gamma_{p}$ = 4.4 keV) was directly observed in $^{11}$B via proton resonance scattering. This resonance was previously inferred in the $\beta$-delayed proto
Externí odkaz:
http://arxiv.org/abs/2205.04973
Autor:
Brandenburg, K., Hamad, G., Meisel, Z., Brune, C. R., Carter, D. E., Danley, T., Derkin, J., Jones-Alberty, Y., Kenady, B., Massey, T. N., Paneru, S., Saxena, M., Soltesz, D., Subedi, S. K., Warren, J.
$(\alpha,n)$ reactions play an important role in nuclear astrophysics and applications and are an important background source in neutrino and dark matter detectors. Measurements of total $(\alpha,n)$ cross sections employing direct neutron detection
Externí odkaz:
http://arxiv.org/abs/2111.15472
Autor:
Gastis, P., Perdikakis, G., Dissanayake, J., Tsintari, P., Sultana, I., Brune, C. R., Massey, T. N., Meisel, Z., Voinov, A. V., Brandenburg, K., Danley, T., Giri, R., Jones-Alberty, Y., Paneru, S., Soltesz, D., Subedi, S.
Publikováno v:
Phys. Rev. C 101, 055805 (2020)
40K plays a significant role in the radiogenic heating of earth-like exoplanets, which can affect the development of a habitable environment on their surfaces. The initial amount of 40K in the interior of these planets depends on the composition of t
Externí odkaz:
http://arxiv.org/abs/2001.11600
Akademický článek
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Autor:
Paneru, S. N., Brune, C. R., Giri, R., Livesay, R. J., Greife, U., Blackmon, J. C., Bardayan, D. W., Chipps, K. A., Davids, B., Connolly, D. S., Chae, K. Y., Champagne, A. E., Deibel, C., Jones, K. L., Johnson, M. S., Kozub, R. L., Ma, Z., Nesaraja, C. D., Pain, S. D., Sarazin, F., Shriner Jr., J. F., Stracener, D. W., Smith, M. S., Thomas, J. S., Visser, D. W., Wrede, C.
Publikováno v:
Phys. Rev. C 99, 045807 (2019)
The astrophysical $S$-factor for the radiative proton capture reaction on $^7$Be ($S_{17}$) at low energies is affected by the $s$-wave scattering lengths. We report the measurement of elastic and inelastic scattering cross sections for the $^7$Be+p
Externí odkaz:
http://arxiv.org/abs/1902.00417
Akademický článek
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