Zobrazeno 1 - 10
of 86
pro vyhledávání: '"Phoenix B"'
Autor:
Garg, R., Dellmann, S., Lederer-Woods, C., Bruno, C. G., Eberhardt, K., Geppert, C., Heftrich, T., Kajan, I., Käppeler, F., Phoenix, B., Reifarth, R., Schumann, D., Weigand, M., Wheldon, C.
Tantalum-180m is nature's rarest (quasi) stable isotope and its astrophysical origin is an open question. A possible production site of this isotope is the slow neutron capture process in Asymptotic Giant Branch stars, where it can be produced via ne
Externí odkaz:
http://arxiv.org/abs/2304.06799
Autor:
Giomataris, I., Katsioulas, I., Knights, P., Manthos, I., Matthews, J., Neep, T., Nikolopoulos, K., Papaevangelou, T., Phoenix, B., Ward, R.
Publikováno v:
2021 IEEE Nuclear Science Symposium and Medical Imaging Conference (NSS/MIC), 2021, pp. 1-3
We present a fast neutron spectroscopy system based on a nitrogen-filled, large volume gaseous detector, the Spherical Proportional Counter. The system has been successfully operated up to gas pressure of 1.5 bar. Neutron energy is estimated through
Externí odkaz:
http://arxiv.org/abs/2211.03897
Autor:
Giomataris, I., Green, S., Katsioulas, I., Knights, P., Manthos, I., Neep, T., Nikolopoulos, K., Papaevangelou, T., Phoenix, B., Sanders, J., Ward, R.
Publikováno v:
Nuclear Inst. and Methods in Physics Research, A 1049 (2023) 168124
The spherical proportional counter is a large volume gaseous detector which finds application in several fields, including direct Dark Matter searches. When the detector is filled with nitrogen it becomes an effective neutron spectrometer thanks to t
Externí odkaz:
http://arxiv.org/abs/2206.04331
Autor:
Giomataris, I., Green, S., Katsioulas, I., Knights, P., Manthos, I., Matthews, J., Neep, T., Nikolopoulos, K., Papaevangelou, T., Phoenix, B., Sanders, J., Ward, R.
Precise in-situ measurements of the neutron flux in underground laboratories is crucial for direct dark matter searches, as neutron induced backgrounds can mimic the typical dark matter signal. The development of a novel neutron spectroscopy techniqu
Externí odkaz:
http://arxiv.org/abs/2107.02682
Autor:
Allport, P., Bogelspacher, F., Bruce, K., Canavan, R., Dierlamm, A., Gonella, L., Knights, P., Mateu, I., Moll, M., Nikolopoulos, K., Phoenix, B., Price, T., Ram, L., Ravotti, F., Simpson-Allsop, C., Wood, C.
Publikováno v:
JINST 14 (2019) P12004
The scheduled High Luminosity upgrade of the CERN Large Hadron Collider presents new challenges in terms of radiation hardness. As a consequence, campaigns to qualify the radiation hardness of detector sensors and components are undertaken worldwide.
Externí odkaz:
http://arxiv.org/abs/1908.03049
Autor:
Giomataris, I., Green, S., Katsioulas, I., Knights, P., Manthos, I., Neep, T., Nikolopoulos, K., Papaevangelou, T., Phoenix, B., Sanders, J., Ward, R.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, A April 2023 1049
Akademický článek
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Autor:
Garg, R., Dellmann, S., Lederer-Woods, C., Bruno, C. G., Eberhardt, K., Geppert, C., Heftrich, T., Kajan, I., Kappeler, F., Phoenix, B., Reifarth, R., Schumann, D., Weigand, M., Wheldon, C.
Publikováno v:
Garg, R, Dellmann, S, Lederer-Woods, C, Bruno, C G, Eberhardt, K, Geppert, C, Heftrich, T, Kajan, I, Kappeler, F, Phoenix, B, Reifarth, R, Schumann, D, Weigand, M & Wheldon, C 2023, ' 179Ta(n,γ) cross-section measurement and the astrophysical origin of the 180Ta isotope ', Physical Review C, vol. 107, no. 4, 045805, pp. 1-7 . https://doi.org/10.1103/PhysRevC.107.045805
180m} is nature’s rarest (quasi) stable isotope and its astrophysical origin is an open question. A possible production site of this isotope is the slow neutron capture process in Asymptotic Giant Branch stars, where it can be produced via neutron
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3094::3df9b781592ead301d0085ba7d517f62
https://www.pure.ed.ac.uk/ws/files/331396900/Ta179_ng_activation_v03.pdf
https://www.pure.ed.ac.uk/ws/files/331396900/Ta179_ng_activation_v03.pdf
Autor:
Xavier, Jessica, McGreevy, Phoenix B, McDougall, Jenny, Lamb, Jessica, Streukens A, Haywood, Beth, Lock, Kurt, Ackermann, Emma, Loyal, Jackson, Ferguson, Max, Liu, Lisa, Ariba Kamal, Greer, Alissa Merielle, Butler, Amanda, Iammarino, Cassandra Sammy, Palis, Heather, Slaunwhite, Amanda, Buxton, Jane
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::73811086b4ca6aedf06afcbff9b8f0ca
Autor:
Garg, R., Dellmann, S., Lederer-Woods, C., Bruno, C. G., Eberhardt, K., Geppert, C., Heftrich, T., Kajan, I., Käppeler, F., Phoenix, B., Reifarth, R., Schumann, D., Weigand, M., Wheldon, C.
Publikováno v:
Physical Review C, 107 (4), Art.-Nr.: 045805
$^{180m}$Ta is nature's rarest (quasi) stable isotope and its astrophysical origin is an open question. A possible production site of this isotope is the slow neutron capture process in asymptotic giant branch stars, where it can be produced via neut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f0c7540ac3e09c2f2a84413351325b65
https://publikationen.bibliothek.kit.edu/1000158468
https://publikationen.bibliothek.kit.edu/1000158468