Difficulties in probing nuclear physics: A study of 
            44Ti and 
            56Ni

Aimee Hungerford; Christopher L. Fryer; Francis Timmes; Patrick Young; Michael Bennet; Steven Diehl; Falk Herwig; Raphael Hirschi; Marco Pignatari; Georgios Magkotsios; Gabriel Rockefeller

Difficulties in probing nuclear physics: A study of ⁴⁴Ti and ⁵⁶Ni

Aimee Hungerford, Christopher L. Fryer, Francis Timmes, Patrick Young, Michael Bennet, Steven Diehl, Falk Herwig, Raphael Hirschi, Marco Pignatari, Georgios Magkotsios, Gabriel Rockefeller

Earth and Space Exploration, School of (SESE)

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

Abstract

The nucleosynthetic yield from a supernova explosion depends upon a variety of effects: progenitor evolution, explosion process, details of the nuclear network, and nuclear rates. Especially in studies of integrated stellar yields, simplifications reduce these uncertainties. But nature is much more complex, and to actually study nuclear rates, we will have to understand the full, complex set of processes involved in nucleosynthesis. Here we discuss a few of these complexities and detail how the NuGrid collaboration will address them.

Original language	English (US)
Title of host publication	Proceedings of Science
State	Published - 2008
Event	10th Symposium on Nuclei in the Cosmos, NIC 2008 - Mackinac Island, MI, United States Duration: Jul 27 2008 → Aug 1 2008

Other

Other	10th Symposium on Nuclei in the Cosmos, NIC 2008
Country/Territory	United States
City	Mackinac Island, MI
Period	7/27/08 → 8/1/08

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Cite this

@inproceedings{03ee11dc7dfc4d7e909e3e4ad50a94d1,

title = "Difficulties in probing nuclear physics: A study of 44Ti and 56Ni",

abstract = "The nucleosynthetic yield from a supernova explosion depends upon a variety of effects: progenitor evolution, explosion process, details of the nuclear network, and nuclear rates. Especially in studies of integrated stellar yields, simplifications reduce these uncertainties. But nature is much more complex, and to actually study nuclear rates, we will have to understand the full, complex set of processes involved in nucleosynthesis. Here we discuss a few of these complexities and detail how the NuGrid collaboration will address them.",

author = "Aimee Hungerford and Fryer, {Christopher L.} and Francis Timmes and Patrick Young and Michael Bennet and Steven Diehl and Falk Herwig and Raphael Hirschi and Marco Pignatari and Georgios Magkotsios and Gabriel Rockefeller",

year = "2008",

language = "English (US)",

booktitle = "Proceedings of Science",

note = "10th Symposium on Nuclei in the Cosmos, NIC 2008 ; Conference date: 27-07-2008 Through 01-08-2008",

}

TY - GEN

T1 - Difficulties in probing nuclear physics

T2 - 10th Symposium on Nuclei in the Cosmos, NIC 2008

AU - Hungerford, Aimee

AU - Fryer, Christopher L.

AU - Timmes, Francis

AU - Young, Patrick

AU - Bennet, Michael

AU - Diehl, Steven

AU - Herwig, Falk

AU - Hirschi, Raphael

AU - Pignatari, Marco

AU - Magkotsios, Georgios

AU - Rockefeller, Gabriel

PY - 2008

Y1 - 2008

N2 - The nucleosynthetic yield from a supernova explosion depends upon a variety of effects: progenitor evolution, explosion process, details of the nuclear network, and nuclear rates. Especially in studies of integrated stellar yields, simplifications reduce these uncertainties. But nature is much more complex, and to actually study nuclear rates, we will have to understand the full, complex set of processes involved in nucleosynthesis. Here we discuss a few of these complexities and detail how the NuGrid collaboration will address them.

AB - The nucleosynthetic yield from a supernova explosion depends upon a variety of effects: progenitor evolution, explosion process, details of the nuclear network, and nuclear rates. Especially in studies of integrated stellar yields, simplifications reduce these uncertainties. But nature is much more complex, and to actually study nuclear rates, we will have to understand the full, complex set of processes involved in nucleosynthesis. Here we discuss a few of these complexities and detail how the NuGrid collaboration will address them.

UR - http://www.scopus.com/inward/record.url?scp=84887311212&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84887311212&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84887311212

BT - Proceedings of Science

Y2 - 27 July 2008 through 1 August 2008

ER -

Difficulties in probing nuclear physics: A study of ⁴⁴Ti and ⁵⁶Ni

Abstract

Other

ASJC Scopus subject areas

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