Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: The effects of rotation on wave-induced transport in stars: the case of
  an intermediate-mass star   Internal gravity waves propagate in stellar radiative zones and transport
angular momentum throughout the evolution of stars, shaping the internal
rotation pro le of these regions. We use the analytical study of Andre\'e et
al. (2018) to assess the impact of rotation and differential rotation on the
thermal dissipation of internal gravity waves near the equatorial plane,
without making any assumption on the relative strength of rotation relative to
that of the background stable stratification. This dissipation is one of the
mechanisms allowing a wave-induced deposition/extraction of angular momentum.
Here, we apply the analysis to a 3 solar mass star of which we have computed
the one-dimensional evolution, from the pre-main sequence to the end of the
main sequence. We show that rotation and differential rotation do not
significantly modify the efficiency of the damping of internal gravity waves by
thermal diffusion, except very close to their excitation region.

3
The categories of this paper are: physics
7
The categories of this paper are: hep-th
22
The categories of this paper are: chao-dyn
0
The categories of this paper are: hep-ph
29
The categories of this paper are: funct-an
16
The categories of this paper are: stat
15
The categories of this paper are: nucl-ex
4
The categories of this paper are: cond-mat
31
The categories of this paper are: ao-sci
13
The categories of this paper are: quant-ph
17
The categories of this paper are: q-fin
19
The categories of this paper are: eess
2
The categories of this paper are: math
35
The categories of this paper are: mtrl-th
12
The categories of this paper are: nucl-th
34
The categories of this paper are: chem-ph