◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

J. Chambers

3 papers hereh-index 7183 citations12 works total

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

author position
  • sole author3

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

fields
  • astro-ph.EP3
same name
  • J. Chambers — 17 papers, h 34
  • J. Chambers — 3 papers, h 61
  • J. Chambers — 2 papers, h 24
  • J. Chambers — 1 paper, h 9
  • J. Chambers — 1 paper, h 19
  • J. Chambers — 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
20172021
most citedSteamworlds: atmospheric structure and critical mass of planets accreting icy pebbles

19 citations · 19 across the 1 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

4 papers · 1 filter

astro-ph.EP2024

Large Fluctuations within 1 AU in Protoplanetary Disks

John Chambers

Protoplanetary disks are often assumed to change slowly and smoothly during planet formation. Here, we investigate the time evolution of isolated disks subject to viscosity and a d…

astro-ph.EP2021

Rapid Formation of Jupiter and Wide-Orbit Exoplanets in Disks with Pressure Bumps

John Chambers

The formation of gas-giant planets within the lifetime of a protoplanetary disk is challenging especially far from a star. A promising model for the rapid formation of giant-planet…

astro-ph.EP2018

Planet Formation: An Optimized Population-Synthesis Approach

John Chambers

The physics of planet formation is investigated using a population synthesis approach. We develop a simple model for planetary growth including pebble and gas accretion, and orbita…

astro-ph.EP2017★ 19 cited

Steamworlds: atmospheric structure and critical mass of planets accreting icy pebbles

John Chambers

In the core accretion model, gas-giant planets first form a solid core, which then accretes gas from a protoplanetary disk when the core exceeds a critical mass. Here, we model the…

◍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.