Research output: Research - peer-review › Journal article

- 10.1093/mnras/stx1890
Final published version

- Andreas C. S. JorgensenAndreas C. S. JorgensenMax Planck Inst Astrophys, Max Planck SocietyMax Planck Inst Halbleiterlabor, Max Planck Society
- Jorgen Christensen-Dalsgaard

We present a comparison between Monte Carlo simulations and a semi-analytical approach that reproduces the theoretical probability distribution functions of the solar neutrino fluxes, stemming from the pp, pep, hep, Be-7, B-8, N-13, O-15 and F-17 source reactions. We obtain good agreement between the two approaches. Thus, the semi-analytical method yields confidence intervals that closely match those found, based on Monte Carlo simulations, and points towards the same general symmetries of the investigated probability distribution functions. Furthermore, the negligible computational cost of this method is a clear advantage over Monte Carlo simulations, making it trivial to take new observational constraints on the input parameters into account.

Original language | English |
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Journal | Royal Astronomical Society. Monthly Notices |

Volume | 471 |

Issue number | 4 |

Pages (from-to) | 4812-4815 |

Number of pages | 4 |

ISSN | 0035-8711 |

DOIs | |

State | Published - Nov 2017 |

- neutrinos, CHEMICAL-COMPOSITION

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