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C. Burgess

6 papers hereh-index 7445 citations11 works total

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

author position
  • sole author3
  • first author3

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • hep-th4
  • physics.comp-ph1
  • physics.optics1
same name
  • C. Burgess — 114 papers, h 62
  • C. Burgess — 31 papers, h 24
  • C. Burgess — 14 papers, h 15
  • C. Burgess — 14 papers, h 9
  • C. Burgess — 11 papers, h 8
  • C. Burgess — 8 papers, 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
20052025
most citedMultiple Inflation, Cosmic String Networks and the String Landscape

95 citations · 100 across the 6 of their papers we have counts for

collaborators
Showing hep-thShow all

4 papers · 1 filter

hep-th2025

Dark Energy and the Symbiosis Between Micro-physics and Cosmology (Naturally)

C. P. Burgess

These lectures aim to highlight the remarkable symbiosis that currently exists between the physics of the very small and the physics of the very large, using the unsolved puzzle of…

hep-th2025

Reminiscences about Steven Weinberg (This Time it's Personal)

C. P. Burgess

Steven Weinberg productive scientific life teaches us many things, one of the most important of which is the power of his example. This essay contains personal reminiscences and a…

hep-th2005★ 2 cited

Supersymmetric Large Extra Dimensions and the Cosmological Constant Problem

C. P. Burgess

This article briefly summarizes and reviews the motivations for - and the present status of - the proposal that the small size of the observed Dark Energy density can be understood…

hep-th2005★ 95 cited

Multiple Inflation, Cosmic String Networks and the String Landscape

C. P. Burgess, Richard Easther, Anupam Mazumdar +2

Motivated by the string landscape we examine scenarios for which inflation is a two-step process, with a comparatively short inflationary epoch near the string scale and a longer p…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.