Zobrazeno 1 - 10
of 427
pro vyhledávání: '"C Wrede"'
Autor:
L.J. Sun, C. Fry, B. Davids, N. Esker, C. Wrede, M. Alcorta, S. Bhattacharjee, M. Bowry, B.A. Brown, T. Budner, R. Caballero-Folch, L. Evitts, M. Friedman, A.B. Garnsworthy, B.E. Glassman, G. Hackman, J. Henderson, O.S. Kirsebom, J. Lighthall, P. Machule, J. Measures, M. Moukaddam, J. Park, C. Pearson, D. Pérez-Loureiro, C. Ruiz, P. Ruotsalainen, J. Smallcombe, J.K. Smith, D. Southall, J. Surbrook, L.E. Weghorn, M. Williams
Publikováno v:
Physics Letters B, Vol 839, Iss , Pp 137801- (2023)
Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P(p,γ)31S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2)
Externí odkaz:
https://doaj.org/article/1ddf186b181f462fbab9621589f3dff2
Autor:
B.E. Glassman, D. Pérez-Loureiro, C. Wrede, J. Allen, D.W. Bardayan, M.B. Bennett, B.A. Brown, K.A. Chipps, M. Febbraro, M. Friedman, C. Fry, M.R. Hall, O. Hall, S.N. Liddick, P. O'Malley, W.J. Ong, S.D. Pain, C. Prokop, S.B. Schwartz, P. Shidling, H. Sims, P. Thompson, H. Zhang
Publikováno v:
Physics Letters B, Vol 778, Iss C, Pp 397-402 (2018)
Certain astrophysical environments such as thermonuclear outbursts on accreting neutron stars (Type-I X-ray bursts) are hot enough to allow for breakout from the Hot CNO hydrogen burning cycles to the rapid proton capture (rp) process. An important b
Externí odkaz:
https://doaj.org/article/e8bee7d0ec134f36ab782be2c1c7be3a
Autor:
J Kamp, L Neubert, J Schupp, C Wrede, F Laenger, T Salditt, J Reichmann, T Welte, A Haverich, N Schwerk, A Bergmann, S von Hardenberg, M Griese, C Rapp, K Olsson, J Fuge, D Park, M Hoeper, H Kreipe, D Jonigk, L Knudsen, M Kuehnel
Publikováno v:
63. Kongress der Deutschen Gesellschaft für Pneumologie und Beatmungsmedizin e. V..
Akademický článek
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Akademický článek
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Publikováno v:
Notfall + Rettungsmedizin. 24:979-981
Autor:
T. Budner, M. Friedman, C. Wrede, B. A. Brown, J. José, D. Pérez-Loureiro, L. J. Sun, J. Surbrook, Y. Ayyad, D. W. Bardayan, K. Chae, A. A. Chen, K. A. Chipps, M. Cortesi, B. Glassman, M. R. Hall, M. Janasik, J. Liang, P. O’Malley, E. Pollacco, A. Psaltis, J. Stomps, T. Wheeler
Publikováno v:
Physical Review Letters. 128
Autor:
C. Wrede, A. McGrogan
Publikováno v:
Bauingenieur. 95:509-518
Zusammenfassung Carlsberg hat im Zeitraum von März 2016 bis November 2019 die Planung, Vergabe und Ausführung für seine neue Holsten-Brauerei in Hamburg realisiert. Das Projekt erfolgte im Rahmen einer Standortverlagerung von Hamburg-Altona in ein
Autor:
Ruchi Mahajan, A. Adams, J. Allmond, H. Alvarez Pol, E. Argo, Y. Ayyad, D. Bardayan, D. Bazin, T. Budner, A. Chen, K. Chipps, B. Davids, J. Dopfer, M. Friedman, H. Fynbo, R. Grzywacz, J. Jose, J. Liang, S. Pain, D. Perez-Loureiro, E. Pollacco, A. Psaltis, S. Ravishankar, A. Rogers, L. Schaedig, L. J. Sun, J. Surbrook, T. Wheeler, L. Weghorn, C. Wrede
Publikováno v:
EPJ Web Conf.
16th International Symposium on Nuclei in the Cosmos
16th International Symposium on Nuclei in the Cosmos, Sep 2021, Chengdu, China. pp.11034, ⟨10.1051/epjconf/202226011034⟩
16th International Symposium on Nuclei in the Cosmos
16th International Symposium on Nuclei in the Cosmos, Sep 2021, Chengdu, China. pp.11034, ⟨10.1051/epjconf/202226011034⟩
15O(α,γ)19Ne is regarded as one of the most important thermonuclear reactions in type I X-ray bursts. For studying the properties of the key resonance in this reaction using β decay, the existing Proton Detector component of the Gaseous Detector w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::19b95f79f1643696a6a404bc42c8f200
https://hal.science/hal-03615336
https://hal.science/hal-03615336
Autor:
Tyler Wheeler, A. Adams, J. Allmond, H. Alvarez Pol, E. Argo, Y. Ayyad, D. Bardayan, D. Bazin, T. Budner, A. Chen, K. Chipps, B. Davids, J. Dopfer, M. Friedman, H. Fynbo, R. Grzywacz, J. Jose, J. Liang, R. Mahajan, S. Pain, D. Pérez-Loureiro, E. Pollacco, A. Psaltis, S. Ravishankar, A. Rogers, L. Schaedig, L. J. Sun, J. Surbrook, L. Weghorn, C. Wrede
Publikováno v:
EPJ Web Conf.
16th International Symposium on Nuclei in the Cosmos
16th International Symposium on Nuclei in the Cosmos, Sep 2021, Chengdu, China. pp.11046, ⟨10.1051/epjconf/202226011046⟩
16th International Symposium on Nuclei in the Cosmos
16th International Symposium on Nuclei in the Cosmos, Sep 2021, Chengdu, China. pp.11046, ⟨10.1051/epjconf/202226011046⟩
Sensitivity studies have shown that the 15O(α, γ)19Ne reaction is the most important reaction rate uncertainty affecting the shape of light curves from Type I X-ray bursts. This reaction is dominated by the 4.03 MeV resonance in 19Ne. Previous meas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ef23fec93209c135c7e33c5c710bc06
https://hal.science/hal-03615334
https://hal.science/hal-03615334