Zobrazeno 1 - 10
of 403
pro vyhledávání: '"Vockenhuber, C."'
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B 15 September 2021 503:45-52
Autor:
Fallis, J., Parikh, A., Bertone, P. F., Bishop, S., Buchmann, L., Chen, A. A., Christian, G., Clark, J. A., D'Auria, J. M., Davids, B., Deibel, C. M., Fulton, B. R., Greife, U., Guo, B., Hager, U., Herlitzius, C., Hutcheon, D. A., José, J., Laird, A. M., Li, E. T., Li, Z. H., Lian, G., Liu, W. P., Martin, L., Nelson, K., Ottewell, D., Parker, P. D., Reeve, S., Rojas, A., Ruiz, C., Setoodehnia, K., Sjue, S., Vockenhuber, C., Wang, Y. B., Wrede, C.
The 33S(p,\gamma)34Cl reaction is important for constraining predictions of certain isotopic abundances in oxygen-neon novae. Models currently predict as much as 150 times the solar abundance of 33S in oxygen-neon nova ejecta. This overproduction fac
Externí odkaz:
http://arxiv.org/abs/1309.3543
Autor:
Sallaska, A. L., Wrede, C., Garcia, A., Storm, D. W., Brown, T. A. D., Ruiz, C., Snover, K. A., Ottewell, D. F., Buchmann, L., Vockenhuber, C., Hutcheon, D. A., Caggiano, J. A., Jose, J.
Publikováno v:
Phys.Rev.C83:034611,2011
Gamma-ray telescopes in orbit around the Earth are searching for evidence of the elusive radionuclide 22Na produced in novae. Previously published uncertainties in the dominant destructive reaction, 22Na(p,g)23Mg, indicated new measurements in the pr
Externí odkaz:
http://arxiv.org/abs/1009.3925
Autor:
Sallaska, A. L., Wrede, C., Garcia, A., Storm, D. W., Brown, T. A. D., Ruiz, C., Snover, K. A., Ottewell, D. F., Buchmann, L., Vockenhuber, C., Hutcheon, D. A., Caggiano, J. A.
Publikováno v:
Phys.Rev.Lett.105:152501,2010; Erratum-ibid.105:209901,2010
The radionuclide 22Na is a potential astronomical observable that is expected to be produced in classical novae in quantities that depend on the thermonuclear rate of the 22Na(p,g)23Mg reaction. We have measured the strengths of low-energy 22Na(p,g)2
Externí odkaz:
http://arxiv.org/abs/1008.4170
Autor:
Dillmann, I., Domingo-Pardo, C., Heil, M., Käppeler, F., Wallner, A., Forstner, O., Golser, R., Kutschera, W., Priller, A., Steier, P., Mengoni, A., Gallino, R., Paul, M., Vockenhuber, C.
Publikováno v:
Phys.Rev.C79:065805,2009
The stellar (n,gamma) cross section of 40Ca at kT=25 keV has been measured with a combination of the activation technique and accelerator mass spectrometry (AMS). This combination is required when direct off-line counting of the produced activity is
Externí odkaz:
http://arxiv.org/abs/0907.0107
Autor:
Mythili, S., Davids, B., Alexander, T. K., Ball, G. C., Chicoine, M., Chakrawarthy, R. S., Churchman, R., Forster, J. S., Gujrathi, S., Hackman, G., Howell, D., Kanungo, R., Leslie, J. R., Padilla, E., Pearson, C. J., Ruiz, C., Ruprecht, G., Schumaker, M. A., Tanihata, I., Vockenhuber, C., Walden, P., Yen, S.
Publikováno v:
Phys.Rev.C77:035803,2008
The 15O(alpha,gamma)19Ne reaction plays a role in the ignition of Type I x-ray bursts on accreting neutron stars. The lifetimes of states in 19Ne above the 15O + alpha threshold of 3.53 MeV are important inputs to calculations of the astrophysical re
Externí odkaz:
http://arxiv.org/abs/0711.0777
Autor:
Vockenhuber, C., Arstila, K., Jensen, J., Julin, J., Kettunen, H., Laitinen, M., Rossi, M., Sajavaara, T., Thöni, M., Whitlow, H.J.
Publikováno v:
In Nuclear Inst. and Methods in Physics Research, B 15 January 2017 391:20-26
Publikováno v:
In Geomorphology 1 December 2016 274:180-192
Autor:
Daraoui, A., Riebe, B., Walther, C., Wershofen, H., Schlosser, C., Vockenhuber, C., Synal, H.-A.
Publikováno v:
In Journal of Environmental Radioactivity April 2016 154:101-108
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