◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

B. Sykes

3 papers hereh-index 00 citations3 works total

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

author position
  • first author2
  • last author1

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

fields
  • astro-ph.HE2
  • astro-ph.GA1

identity via Semantic Scholar / OpenAlex

most citedAn estimate of the stochastic gravitational wave background from the MassiveBlackII simulation

15 citations · 20 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2026

Core-collapse supernovae and supernova neutrinos

B. Mueller, B. Sykes

Core-collapse supernovae are the terminal explosions of massive stars. After successive phases of nuclear fusion proceeding up to silicon burning, these stars form an iron core tha…

astro-ph.HE2022★ 5 cited

A Black-Hole Excision Scheme for General Relativistic Core-Collapse Supernova Simulations

B. Sykes, B. Mueller, I. Cordero-Carrión +2

Fallback supernovae and the collapsar scenario for long-gamma ray burst and hypernovae have received considerable interest as pathways to black-hole formation and extreme transient…

astro-ph.GA2022★ 15 cited

An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation

Bailey Sykes, Hannah Middleton, Andrew Melatos +3

A population of super-massive black hole binaries is expected to generate a stochastic gravitational wave background (SGWB) in the pulsar timing array (PTA) frequency range of $10^…

◍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.