activity
19932020
most citedRole of the scalar field in gravitational lensing

155 citations · 726 across the 23 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2020★ 6 cited

Convective Differential Rotation in Stars and Planets II: Observational and Numerical Tests

Adam S. Jermyn, Shashikumar M. Chitre, Pierre Lesaffre +1

Differential rotation is central to a great many mysteries in stars and planets. In Part I we predicted the order of magnitude and scaling of the differential rotation in both hydr…

astro-ph.SR2020★ 9 cited

Convective Differential Rotation in Stars and Planets I: Theory

Adam S. Jermyn, Shashikumar M. Chitre, Pierre Lesaffre +1

We derive the scaling of differential rotation in both slowly- and rapidly-rotating convection zones using order of magnitude methods. Our calculations apply across stars and fluid…

astro-ph.SR2018★ 17 cited

Enhanced Rotational Mixing in the Radiative Zones of Massive Stars

Adam S. Jermyn, Christopher A. Tout, Shashikumar M. Chitre

Convection in the cores of massive stars becomes anisotropic when they rotate. This anisotropy leads to a misalignment of the thermal gradient and the thermal flux, which in turn r…

astro-ph.SR2018★ 10 cited

Turbulence Closure for Mixing Length Theories

Adam S. Jermyn, Pierre Lesaffre, Christopher A. Tout +1

We present an approach to turbulence closure based on mixing length theory with three-dimensional fluctuations against a two-dimensional background. This model is intended to be ra…

astro-ph.SR2014★ 11 cited

Properties of - and -modes in hydromagnetic turbulence

Nishant K. Singh, Axel Brandenburg, S. M. Chitre +1

With the ultimate aim of using the fundamental or -mode to study helioseismic aspects of turbulence-generated magnetic flux concentrations, we use randomly forced hydromagnetic…

astro-ph.SR2013★ 7 cited

A two-dimensional mixing length theory of convective transport

P. Lesaffre, S. M. Chitre, A. T. Potter +1

The helioseismic observations of the internal rotation profile of the Sun raise questions about the two-dimensional (2D) nature of the transport of angular momentum in stars. Here…