◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

R. P. Ratnasingam

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
ORCID 0000-0002-7250-6524

identity via Semantic Scholar / OpenAlex

most citedThree-Dimensional Simulations of Massive Stars: I. Wave Generation and Propagation

103 citations · 139 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2020★ 36 cited

Two-Dimensional Simulations of Internal Gravity Waves in The Radiation Zones of Intermediate-Mass Stars

R. P. Ratnasingam, P. V. F. Edelmann, T. M. Rogers

Intermediate-mass main sequence stars have large radiative envelopes overlying convective cores. This configuration allows internal gravity waves (IGWs) generated at the convective…

astro-ph.SR2019★ 103 cited

Three-Dimensional Simulations of Massive Stars: I. Wave Generation and Propagation

P. V. F. Edelmann, R. P. Ratnasingam, M. G. Pedersen +3

We present the first three-dimensional (3D), hydrodynamic simulations of the core convection zone (CZ) and extended radiative zone spanning from 1% to 90% of the stellar radius of…

astro-ph.SR2019

Astro2020 Science White Paper: gravity-wave asteroseismology of intermediate- and high-mass stars

Andrew Tkachenko, Conny Aerts, Dominic M. Bowman +17

The evolution of a star is driven by the physical processes in its interior making the theory of stellar structure and evolution the most crucial ingredient for not only stellar ev…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.