Determination of K-shell absorption jump factor for some elements using EDXRF Technique
Özet
Upper limits are presented on the diffuse flux of ultra-high energy $\nu_e$,
based on analysis of data taken by the RICE experiment during August, 2000. The
RICE receiver array at South Pole monitors cold ice for radio-wavelength
Cherenkov radiation resulting from neutrino-induced in-ice showers. For
energies above 1 EeV, RICE is an effective detector of over 15 km$^3$ sr.
Potential signal events are separated from backgrounds using vertex location,
event reconstruction, and signal shape. These are the first terrestrial limits
exploiting the physics of radio Cherenkov emissions from charged-current
$\nu_e+N\to e+N'$ interactions.
Anahtar kelimeler
Atıf için künye
BUDAK, G., Karabulut, A., & ERTUĞRUL, M. (2003). Determination of K-shell absorption jump factor for some elements using EDXRF Technique. Radiation Measurements, 37(2), 103–107. https://doi.org/10.1016/s1350-4487%2802%2900181-6
BibTeX
@article{budak2003-62470,
author = {BUDAK, Gökhan and Karabulut, Abdulhalik and ERTUĞRUL, Mehmet},
title = {Determination of K-shell absorption jump factor for some elements using EDXRF Technique},
journal = {Radiation Measurements},
year = {2003},
volume = {37},
number = {2},
pages = {103--107},
issn = {1350-4487},
doi = {10.1016/s1350-4487(02)00181-6},
url = {https://akademik.atauni.edu.tr/yayinlar/62470-determination-of-k-shell-absorption-jump-factor-for-some-elements-using-edxrf}
}