starlib.physics.unc.edu

//Nucleosynthesis Simulator//

Nuclear physics processes generate the energy that makes stars shine. These very same processes in stars are responsible for the synthesis of the elements. When stars eject part of their matter by various means, they enrich the interstellar medium with the nuclear ashes and thereby provide the building blocks for the birth of new stars, of planets, and of life itself. The theory of this building of elements is called nucleosynthesis. Special thanks to McG.

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//Nucleosynthesis Simulator// | starlib.physics.unc.edu Reviews

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Nuclear physics processes generate the energy that makes stars shine. These very same processes in stars are responsible for the synthesis of the elements. When stars eject part of their matter by various means, they enrich the interstellar medium with the nuclear ashes and thereby provide the building blocks for the birth of new stars, of planets, and of life itself. The theory of this building of elements is called nucleosynthesis. Special thanks to McG.

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//Nucleosynthesis Simulator// | starlib.physics.unc.edu Reviews

https://starlib.physics.unc.edu

Nuclear physics processes generate the energy that makes stars shine. These very same processes in stars are responsible for the synthesis of the elements. When stars eject part of their matter by various means, they enrich the interstellar medium with the nuclear ashes and thereby provide the building blocks for the birth of new stars, of planets, and of life itself. The theory of this building of elements is called nucleosynthesis. Special thanks to McG.

INTERNAL PAGES

starlib.physics.unc.edu

1

//Nucleosynthesis Simulator//

http://starlib.physics.unc.edu/RateCalc.php

The calculation of thermonuclear reaction rates is a complicated and involved process. General information on reaction rates can be found in a recent textbook. The rates are calculated according to a method described here. Running this code on our server requires registering and logging into our site, though input files are freely available. That paper also explains the input file format. Starting the MC Simulation. Display Default Input Files. To run the Monte Carlo simulation on our STARLIB server, cop...

2

//Nucleosynthesis Simulator//

http://starlib.physics.unc.edu/index.html

Nuclear physics processes generate the energy that makes stars shine. These very same processes in stars are responsible for the synthesis of the elements. When stars eject part of their matter by various means, they enrich the interstellar medium with the nuclear ashes and thereby provide the building blocks for the birth of new stars, of planets, and of life itself. The theory of this building of elements is called nucleosynthesis. Special thanks to McG.

3

//Nucleosynthesis Simulator//

http://starlib.physics.unc.edu/Details.php

Is a next-generation library of thermonuclear reaction and decay rates. Additional information is available in our publication in the Astrophysical Journal Supplement Series. Incorporates the results of the Monte Carlo based thermonuclear reaction rate evaluation of Iliadis et al., Nucl. Phys. A841, 31 (2010). Unlike other libraries, STARLIB. Also provides factor uncertainties and probability density functions of reaction rates at each temperature grid point. Ie, the tabulated reverse rates already conta...

4

//Nucleosynthesis Simulator//

http://starlib.physics.unc.edu/RateLib.php

The nuclear physics library for astrophysical research that can be accessed here is called STARLIB, which is described in detail in this publication. STARLIB has a number of unique features: (i) it is a tabular library listing reaction rates (cm. Constants on a grid of temperatures between 1 MK and 10 GK; (ii) it incorporates a recent evaluation. Using the menus below, you may display the rate for a specified reaction and cut/paste the results into an editor. Click on. Special reactions (for example, tho...

5

//Nucleosynthesis Simulator//

http://starlib.physics.unc.edu/Links.php

Below are a list of links to additional nuclear astrophysics thermonuclear reaction rate libraries and other sources of interest. BRUSLIB Network Generator NetGen. Oak Ridge Nuclear Astrophysics Data. BRUSLIB's TALYS Reaction Rates. BNL National Nuclear Data Center. These pages are maintained by Anne Sallaska and Christian Iliadis, in collaboration with Art Champagne (UNC),. Sumner Starrfield (ASU), and Frank Timmes (ASU). For comments, send a message to the webmaster.

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cococubed.asu.edu

K-20 and public outreach from cococubed

http://cococubed.asu.edu/outreach_pages/outreach.shtml

Education and Public Outreach. 2016 NSF SI2 PI Workshop. 2016 MESA Summer School. Education and Public Outreach. Ed Brown's lecture notes. K-12: Earth, Moon and Mars. Sally Ride Science Festival. Contact: F.X.Timmes. At UC Santa Barbara:. 9791; 12 YouTube videos. On customizing pgstar based on material presented at the 2014 MESA summer school. 9798; The MESA-Web. 9788; Ed Brown's excellent lecture notes. 9788; The Open Astrophysics Bookshelf. 9817; Smashing White Dwarfs. Friends of the KITP, 2015.

cococubed.asu.edu

some astronomy talks from cococubed

http://cococubed.asu.edu/talk_pages/talks.shtml

Silicon ejecta from SNIa. Peak Luminosity of SNIa. 2016 NSF SI2 PI Workshop. 2016 MESA Summer School. Education and Public Outreach. Contact: F.X.Timmes. Star; Unustable Isotopes / Explosive Burning. April 2016, Notre Dame. Star; Smashing White Dwarfs. January 2016, UNC Chapel Hill. Star; MESA - Customizing. Star; Hunting the Progenitors. Of Supernovae Type Ia. March 2014, Stony Brook. Star; On Silicon Group Elements. Institute for Advanced Study. Star; Connecting Nuclear Astrophysics.

cococubed.asu.edu

cococubed home page

http://cococubed.asu.edu/index.html

School of Earth and Space Exploration. 2016 NSF SI2 PI Workshop. 2016 ASU EdX AST111x. 2016 MESA Summer School. Education and Public Outreach. Contact: F.X.Timmes. Bull; Astronomy research. Bull; Software instruments. Bull; Bicycle adventures. Bull; AAS Journals. Bull; 2016 NSF SI2 PI Workshop. Bull; Teaching materials. Bull; 2016 ASU EdX AST111x. Bull; 2016 MESA Summer School. Bull; Education and Public Outreach. 2016 MESA Summer School.

cococubed.asu.edu

astronomy software instruments from cococubed

http://cococubed.asu.edu/code_pages/codes.shtml

Stellar equation of states. Neutrino energy loss rates. Fitting to conic sections. Derivatives on uneven grids. Quadratics, Cubics, Quartics. Plane - Cube Intersection. 2016 NSF SI2 PI Workshop. 2016 MESA Summer School. Education and Public Outreach. Contact: F.X.Timmes. Some software instruments, some more intricate than others:. 9738; Stellar equation of states. 9738; Equation of state with ionization. 9738; EOS for core collapse supernovae. 9738; Electron chemical potentials. 9738; Voigt Function.

ndc3.net

Nuclear Data Cloud Computing Systems

http://www.ndc3.net/systems/systems.html

Nuclear Data Cloud Computing Systems. Please send your suggestions for entries on this list to cloud@ndc3.net. 149; Computational Infrastructure for Nuclear Astrophysics. Upload, visualize, save, share, modify, compare, numerically integrate, parameterize;. Upload, generate from numerical integration, parameterize, visualize, save, share, modify, compare, store in libraries;. Create, modify, share, use in element synthesis calculations;. 149; nuclearmasses.org. 149; bigbangonline.org. 149; NON-SMOKER WEB.

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starlib.physics.unc.edu

//Nucleosynthesis Simulator//

Nuclear physics processes generate the energy that makes stars shine. These very same processes in stars are responsible for the synthesis of the elements. When stars eject part of their matter by various means, they enrich the interstellar medium with the nuclear ashes and thereby provide the building blocks for the birth of new stars, of planets, and of life itself. The theory of this building of elements is called nucleosynthesis. Special thanks to McG.

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