Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars

T. Rauscher; N. Nishimura; R. Hirschi

doi:10.1063/1.4953300

Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars

T. Rauscher, N. Nishimura, R. Hirschi

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

1 Citation (Scopus)

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Abstract

Nucleosynthesis of heavy elements requires the use of different experimental and theoretical methods to determine astrophysical reaction rates than light element nucleosynthesis. Additionally, there are also larger uncertainties involved in the astrophysical models, both because the sites are not well known and because of differing numerical treatments in different models. As an example for the latter, the production of p-nuclei is compared in two different stellar models, demonstrating that a model widely used for postproduction calculations may have a zone grid too coarse to follow the synthesis of p-nuclei in detail.

Original language	English
Title of host publication	CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology
Editors	Barbara Szczerbinska, Rouzbeh Allahverdi, Kaladi Babu, Baha Balantekin, Bhaskar Dutta, Teruki Kamon, Jason Kumar, Farinaldo Queiroz, Louis Strigari, Rebecca Surman
Place of Publication	South Dakota, USA
Publisher	American Institute of Physics (AIP)
Volume	1743
ISBN (Print)	9780735414006
DOIs	https://doi.org/10.1063/1.4953300
Publication status	Published - 21 Jun 2016
Event	5th Workshop on Dark Matter, Neutrino Physics and Astrophysics, CETUP* 2015 and 9th International Conference on Interconnections between Particle Physics and Cosmology, PPC 2015 - Lead/Deadwood, United States Duration: 15 Jun 2015 → 17 Jul 2015

Conference

Conference	5th Workshop on Dark Matter, Neutrino Physics and Astrophysics, CETUP* 2015 and 9th International Conference on Interconnections between Particle Physics and Cosmology, PPC 2015
Country/Territory	United States
City	Lead/Deadwood
Period	15/06/15 → 17/07/15

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10.1063/1.4953300

1510.04994v2Accepted author manuscript, 800 KBLicence: Unspecified

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Rauscher, T., Nishimura, N., & Hirschi, R. (2016). Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars. In B. Szczerbinska, R. Allahverdi, K. Babu, B. Balantekin, B. Dutta, T. Kamon, J. Kumar, F. Queiroz, L. Strigari, & R. Surman (Eds.), CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology (Vol. 1743). Article 040008 American Institute of Physics (AIP). https://doi.org/10.1063/1.4953300

Rauscher, T. ; Nishimura, N. ; Hirschi, R. / Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars. CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology. editor / Barbara Szczerbinska ; Rouzbeh Allahverdi ; Kaladi Babu ; Baha Balantekin ; Bhaskar Dutta ; Teruki Kamon ; Jason Kumar ; Farinaldo Queiroz ; Louis Strigari ; Rebecca Surman. Vol. 1743 South Dakota, USA : American Institute of Physics (AIP), 2016.

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title = "Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars",

abstract = "Nucleosynthesis of heavy elements requires the use of different experimental and theoretical methods to determine astrophysical reaction rates than light element nucleosynthesis. Additionally, there are also larger uncertainties involved in the astrophysical models, both because the sites are not well known and because of differing numerical treatments in different models. As an example for the latter, the production of p-nuclei is compared in two different stellar models, demonstrating that a model widely used for postproduction calculations may have a zone grid too coarse to follow the synthesis of p-nuclei in detail.",

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doi = "10.1063/1.4953300",

language = "English",

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editor = "Szczerbinska, {Barbara } and Allahverdi, {Rouzbeh } and Babu, {Kaladi } and Balantekin, {Baha } and Dutta, {Bhaskar } and Teruki Kamon and Kumar, {Jason } and Queiroz, {Farinaldo } and Strigari, {Louis } and Surman, {Rebecca }",

booktitle = "CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology",

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Rauscher, T, Nishimura, N & Hirschi, R 2016, Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars. in B Szczerbinska, R Allahverdi, K Babu, B Balantekin, B Dutta, T Kamon, J Kumar, F Queiroz, L Strigari & R Surman (eds), CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology. vol. 1743, 040008, American Institute of Physics (AIP), South Dakota, USA, 5th Workshop on Dark Matter, Neutrino Physics and Astrophysics, CETUP* 2015 and 9th International Conference on Interconnections between Particle Physics and Cosmology, PPC 2015, Lead/Deadwood, United States, 15/06/15. https://doi.org/10.1063/1.4953300

Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars. / Rauscher, T.; Nishimura, N.; Hirschi, R.
CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology. ed. / Barbara Szczerbinska; Rouzbeh Allahverdi; Kaladi Babu; Baha Balantekin; Bhaskar Dutta; Teruki Kamon; Jason Kumar; Farinaldo Queiroz; Louis Strigari; Rebecca Surman. Vol. 1743 South Dakota, USA: American Institute of Physics (AIP), 2016. 040008.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

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T1 - Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars

AU - Rauscher, T.

AU - Nishimura, N.

AU - Hirschi, R.

N1 - T. Rauscher, N. Nishimura, and R. Hirschi, ‘Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars’, in proceedings CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology. Deadwood, South Dakota, USA. 15-17 July 2015. Barbara Szczerbinska, Rouzbeh Allahverdi, Kaladi Babu, Baha Balantekin, Bhaskar Dutta, Teruki Kamon, Jason Kumar, Farinaldo Queiroz, Louis Strigari, and Rebecca Surman eds., AIP Conference Proceedings 1743, 040008 (2016); doi: http://dx.doi.org/10.1063/1.4953300ISBN 9780735414006. Published by AIP Publishing.

PY - 2016/6/21

Y1 - 2016/6/21

N2 - Nucleosynthesis of heavy elements requires the use of different experimental and theoretical methods to determine astrophysical reaction rates than light element nucleosynthesis. Additionally, there are also larger uncertainties involved in the astrophysical models, both because the sites are not well known and because of differing numerical treatments in different models. As an example for the latter, the production of p-nuclei is compared in two different stellar models, demonstrating that a model widely used for postproduction calculations may have a zone grid too coarse to follow the synthesis of p-nuclei in detail.

AB - Nucleosynthesis of heavy elements requires the use of different experimental and theoretical methods to determine astrophysical reaction rates than light element nucleosynthesis. Additionally, there are also larger uncertainties involved in the astrophysical models, both because the sites are not well known and because of differing numerical treatments in different models. As an example for the latter, the production of p-nuclei is compared in two different stellar models, demonstrating that a model widely used for postproduction calculations may have a zone grid too coarse to follow the synthesis of p-nuclei in detail.

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DO - 10.1063/1.4953300

M3 - Conference contribution

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SN - 9780735414006

VL - 1743

BT - CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology

A2 - Szczerbinska, Barbara

A2 - Allahverdi, Rouzbeh

A2 - Babu, Kaladi

A2 - Balantekin, Baha

A2 - Dutta, Bhaskar

A2 - Kamon, Teruki

A2 - Kumar, Jason

A2 - Queiroz, Farinaldo

A2 - Strigari, Louis

A2 - Surman, Rebecca

PB - American Institute of Physics (AIP)

CY - South Dakota, USA

T2 - 5th Workshop on Dark Matter, Neutrino Physics and Astrophysics, CETUP* 2015 and 9th International Conference on Interconnections between Particle Physics and Cosmology, PPC 2015

Y2 - 15 June 2015 through 17 July 2015

ER -

Rauscher T, Nishimura N, Hirschi R. Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars. In Szczerbinska B, Allahverdi R, Babu K, Balantekin B, Dutta B, Kamon T, Kumar J, Queiroz F, Strigari L, Surman R, editors, CETUP* 2015 – Workshop on Dark Matter, Neutrino Physics and Astrophysics PPC 2015 – IXth International Conference on Interconnections between Particle Physics and Cosmology. Vol. 1743. South Dakota, USA: American Institute of Physics (AIP). 2016. 040008 doi: 10.1063/1.4953300

Theory considerations for nucleosynthesis beyond Fe with special emphasis on p-nuclei in massive stars

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