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researcher

C. Wetterich

65 papers hereh-index 19980 citations35 works total

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

author position
  • sole author24
  • middle author1
  • last author39

Across the 64 of 65 papers where every author was matched, so the position is known.

fields
  • hep-ph19
  • hep-th16
  • quant-ph6
  • gr-qc5
  • cond-mat.quant-gas4
  • cond-mat.str-el4
same name
  • C. Wetterich — 173 papers, h 59
  • C. Wetterich — 10 papers, h 9
  • C. Wetterich — 5 papers, h 3
  • C. Wetterich — 4 papers, h 2
  • C. Wetterich — 2 papers
  • C. Wetterich — 2 papers, h 3

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
19932024
most citedCosmology and the Fate of Dilatation Symmetry

2.7k citations · 5.3k across the 65 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

cond-mat.stat-mech2008★ 48 cited

Efimov effect from functional renormalization

S. Moroz, S. Floerchinger, R. Schmidt +1

We apply a field-theoretic functional renormalization group technique to the few-body (vacuum) physics of non-relativistic atoms near a Feshbach resonance. Three systems are consid…

quant-ph2008★ 13 cited

Probabilistic observables, conditional correlations, and quantum physics

C. Wetterich

We discuss the classical statistics of isolated subsystems. Only a small part of the information contained in the classical probability distribution for the subsystem and its envir…

hep-th2008★ 23 cited

Dilatation symmetry in higher dimensions and the vanishing of the cosmological constant

C. Wetterich

A wide class of dilatation symmetric effective actions in higher dimensions leads to a vanishing four-dimensional cosmological constant. This requires no tuning of parameters and r…

astro-ph2008★ 90 cited

Neutrino clustering in growing neutrino quintessence

D. F. Mota, V. Pettorino, G. Robbers +1

A growing neutrino mass can stop the dynamical evolution of a dark energy scalar field, thus explaining the 'why now' problem. We show that such models lead to a substantial neutri…

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