◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

I. Araya

37 papers hereh-index 13386 citations53 works total

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

author position
  • first author11
  • middle author22
  • last author3

Across the 36 of 37 papers where every author was matched, so the position is known.

fields
  • hep-th16
  • astro-ph.SR13
  • astro-ph.CO6
  • astro-ph.GA1
  • gr-qc1
same name
  • I. Araya — 6 papers, h 3
  • I. Araya — 5 papers, h 0
  • I. Araya — 2 papers
  • I. Araya — 1 paper
  • I. Araya — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20102023
most citedA cyclic bipolar wind in the interacting binary V393 Scorpii

38 citations · 465 across the 37 of their papers we have counts for

collaborators
Showing 2017Show all

4 papers · 1 filter

hep-th2017★ 17 cited

Renormalization of Entanglement Entropy from topological terms

Giorgos Anastasiou, Ignacio J. Araya, Rodrigo Olea

We propose a renormalization scheme for Entanglement Entropy of 3D CFTs with a 4D asymptotically AdS gravity dual in the context of the gauge/gravity correspondence. The procedure…

gr-qc2017★ 4 cited

Extended Rindler Spacetime and a New Multiverse Structure

Ignacio J. Araya, Itzhak Bars

This is the first of a series of papers in which we use analyticity properties of quantum fields propagating on a spacetime to uncover a new multiverse geometry when the classical…

astro-ph.SR2017★ 37 cited

Stellar parameters and Hα line profile variability of Be stars in the BeSOS survey

C. Arcos, S. Kanaan, J. Chávez +3

The Be phenomenon is present in about 20% of the B-type stars. Be stars show variability on a broad range of timescales, which in most cases is related to the presence of a circ…

astro-ph.SR2017★ 8 cited

Ω-Slow Solutions and Be Star Disks

I. Araya, C. E. Jones, M. Curé +4

As the disk formation mechanism(s) in Be stars is(are) as yet unknown, we investigate the role of rapidly rotating radiation-driven winds in this process. We implemented the effect…

◍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.