University of Hertfordshire

By the same authors

The key role of SNe Ia for galactic chemical evolution of p-nuclei: 2D - 3D comparison

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Standard

The key role of SNe Ia for galactic chemical evolution of p-nuclei : 2D - 3D comparison. / Travaglio, Claudia; Röpke, F. K.; Seitenzahl, I. R.; Gallino, R.; Rauscher, T.; Hillebrandt, W.

Proceedings of Science. Vol. 07-11-July-2015 Proceedings of Science (PoS), 2014. 032.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Harvard

Travaglio, C, Röpke, FK, Seitenzahl, IR, Gallino, R, Rauscher, T & Hillebrandt, W 2014, The key role of SNe Ia for galactic chemical evolution of p-nuclei: 2D - 3D comparison. in Proceedings of Science. vol. 07-11-July-2015, 032, Proceedings of Science (PoS), 13th Nuclei in the Cosmos, NIC 2014, Debrecen, Hungary, 7/07/14. <http://pos.sissa.it/archive/conferences/204/032/NIC%20XIII_032.pdf>

APA

Travaglio, C., Röpke, F. K., Seitenzahl, I. R., Gallino, R., Rauscher, T., & Hillebrandt, W. (2014). The key role of SNe Ia for galactic chemical evolution of p-nuclei: 2D - 3D comparison. In Proceedings of Science (Vol. 07-11-July-2015). [032] Proceedings of Science (PoS). http://pos.sissa.it/archive/conferences/204/032/NIC%20XIII_032.pdf

Vancouver

Travaglio C, Röpke FK, Seitenzahl IR, Gallino R, Rauscher T, Hillebrandt W. The key role of SNe Ia for galactic chemical evolution of p-nuclei: 2D - 3D comparison. In Proceedings of Science. Vol. 07-11-July-2015. Proceedings of Science (PoS). 2014. 032

Author

Travaglio, Claudia ; Röpke, F. K. ; Seitenzahl, I. R. ; Gallino, R. ; Rauscher, T. ; Hillebrandt, W. / The key role of SNe Ia for galactic chemical evolution of p-nuclei : 2D - 3D comparison. Proceedings of Science. Vol. 07-11-July-2015 Proceedings of Science (PoS), 2014.

Bibtex

@inproceedings{dfc6aeaf3d5048bc9213c157a6dcbc7e,
title = "The key role of SNe Ia for galactic chemical evolution of p-nuclei: 2D - 3D comparison",
abstract = "The bulk of the p-isotopes is created in the 'gamma processes', mainly by sequences of photodisintegrations and beta decays in explosive conditions in core collapse or in Type Ia supernovae (SNe Ia). We explore single-degenerate SNe Ia in the framework of 2D (DDT-a, Travaglio et al. 2011) and 3D (N100, Seitenzahl et al. 2013) delayed-detonation explosion models. A detailed analysis of the comparison between 2 and 3 dimensions will be presented in this work. Using a Galactic chemical evolution code, we give estimates of the contribution of SNe Ia to the solar p-process composition (see Travaglio et al. 2014 for a detailed analysis).",
author = "Claudia Travaglio and R{\"o}pke, {F. K.} and Seitenzahl, {I. R.} and R. Gallino and T. Rauscher and W. Hillebrandt",
note = "ISSN: 18248039; 13th Nuclei in the Cosmos, NIC 2014 ; Conference date: 07-07-2014 Through 11-07-2014",
year = "2014",
month = dec,
day = "31",
language = "English",
volume = "07-11-July-2015",
booktitle = "Proceedings of Science",
publisher = "Proceedings of Science (PoS)",

}

RIS

TY - GEN

T1 - The key role of SNe Ia for galactic chemical evolution of p-nuclei

T2 - 13th Nuclei in the Cosmos, NIC 2014

AU - Travaglio, Claudia

AU - Röpke, F. K.

AU - Seitenzahl, I. R.

AU - Gallino, R.

AU - Rauscher, T.

AU - Hillebrandt, W.

N1 - ISSN: 18248039

PY - 2014/12/31

Y1 - 2014/12/31

N2 - The bulk of the p-isotopes is created in the 'gamma processes', mainly by sequences of photodisintegrations and beta decays in explosive conditions in core collapse or in Type Ia supernovae (SNe Ia). We explore single-degenerate SNe Ia in the framework of 2D (DDT-a, Travaglio et al. 2011) and 3D (N100, Seitenzahl et al. 2013) delayed-detonation explosion models. A detailed analysis of the comparison between 2 and 3 dimensions will be presented in this work. Using a Galactic chemical evolution code, we give estimates of the contribution of SNe Ia to the solar p-process composition (see Travaglio et al. 2014 for a detailed analysis).

AB - The bulk of the p-isotopes is created in the 'gamma processes', mainly by sequences of photodisintegrations and beta decays in explosive conditions in core collapse or in Type Ia supernovae (SNe Ia). We explore single-degenerate SNe Ia in the framework of 2D (DDT-a, Travaglio et al. 2011) and 3D (N100, Seitenzahl et al. 2013) delayed-detonation explosion models. A detailed analysis of the comparison between 2 and 3 dimensions will be presented in this work. Using a Galactic chemical evolution code, we give estimates of the contribution of SNe Ia to the solar p-process composition (see Travaglio et al. 2014 for a detailed analysis).

UR - http://www.scopus.com/inward/record.url?scp=84957671329&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84957671329

VL - 07-11-July-2015

BT - Proceedings of Science

PB - Proceedings of Science (PoS)

Y2 - 7 July 2014 through 11 July 2014

ER -