@Book{1795113855,
author="Scheibe, Ludwig",
title="Thermal evolution models for Uranus and Neptune",
year="2021",
address="Rostock",
abstract="Uranus and Neptune (U{\&}N) have highly different intrinsic heat fluxes. Here, the principles behind a new computer code for calculating numerical structure and evolution models of planets are presented, and with this program the thermal evolution of U{\&}N is investigated using up-to-date equation of state data. Particularly, it is shown that the assumption of a thermal boundary layer in the planet's envelope, trapping part of its heat in the deep interior, impacts the planet's cooling drastically and thus allows for an explanation of U{\&}N's heat fluxes within the same framework.<eng>",
school="Universit{\"a}t Rostock",
note="vorgelegt von Ludwig Scheibe",
note="GutachterInnen: Ronald Redmer (Universit{\"a}t Rostock, Institut f{\"u}r Physik) ; Doris Breuer (Deutsches Zentrum f{\"u}r Luft- und Raumfahrt, Institut f{\"u}r Planetenforschung)",
note="Dissertation Universit{\"a}t Rostock 2022",
doi="10.18453/rosdok_id00003533",
url="http://purl.uni-rostock.de/rosdok/id00003533",
url="https://nbn-resolving.org/urn:nbn:de:gbv:28-rosdok_id00003533-9",
url="https://d-nb.info/1293536997/34",
url="https://doi.org/10.18453/rosdok_id00003533",
language="English"
}