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Logarithmic partial derivatives of fluxes with individual abundances

- Explanation
- These two tables are taken from Tables 1 and 2 of
astro-ph/0412096. The entries represent the logarithmic partial
derivatives of each neutrino flux with respect to each of the principal
element abundances. The first table was computed using the solar model
BP04 and the second table was computed using the solar model BP04+,
both models taken from Bahcall-Pinsonneault, Phys. Rev. Lett., 92,
Number 12, 121301 (2004), astro-ph/0402114.

- In the tables, rows refer to different neutrino fluxes: pp, pep,
hep, 7Be, 8B, 13N, 15O and 17F. Columns refer to different element
abundances divided the hydrogen abundance: C, N, O, Ne, Mg, Si, S, Ar,
Fe. Entries are the logarithmic partial derivatives of the fluxes with
respect to the individual abundances: .

- Obtaining
the tables.

Click here to display tabular form of Table
1 or Table
2
and then use your browser to save the file.

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