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researcher

P. Agrawal

47 papers hereh-index 273.8k citations74 works total

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

author position
  • first author41
  • middle author5
  • last author1

Across the 47 of 47 papers where every author was matched, so the position is known.

fields
  • hep-ph38
  • astro-ph.CO4
  • hep-th4
  • astro-ph.HE1
same name
  • P. Agrawal — 51 papers, h 20
  • P. Agrawal — 33 papers, h 20
  • P. Agrawal — 14 papers, h 9
  • P. Agrawal — 11 papers, h 33
  • P. Agrawal — 5 papers, h 22
  • P. Agrawal — 4 papers, h 2

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
20082022
most citedOn the Cosmological Implications of the String Swampland

556 citations · 3.1k across the 46 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

4 papers · 1 filter

astro-ph.CO2019★ 52 cited

A CMB Millikan Experiment with Cosmic Axiverse Strings

Prateek Agrawal, Anson Hook, Junwu Huang

We study axion strings of hyperlight axions coupled to photons. Hyperlight axions -- axions lighter than Hubble at recombination -- are a generic prediction of the string axiverse.…

astro-ph.CO2019★ 79 cited

H0​ Tension, Swampland Conjectures and the Epoch of Fading Dark Matter

Prateek Agrawal, Georges Obied, Cumrun Vafa

Motivated by the swampland dS conjecture, we consider a rolling scalar field as the source of dark energy. Furthermore, the swampland distance conjecture suggests that the rolling…

astro-ph.CO2019★ 150 cited

Rock 'n' Roll Solutions to the Hubble Tension

Prateek Agrawal, Francis-Yan Cyr-Racine, David Pinner +1

Local measurements of the Hubble parameter are increasingly in tension with the value inferred from a ΛCDM fit to the cosmic microwave background (CMB) data. In this paper, we co…

astro-ph.CO2017★ 47 cited

Dark Catalysis

Prateek Agrawal, Francis-Yan Cyr-Racine, Lisa Randall +1

Recently it was shown that dark matter with mass of order the weak scale can be charged under a new long-range force, decoupled from the Standard Model, with only weak constraints…

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