activity
19932023
most citedExact evolution equation for the effective potential

2.2k citations · 10.6k across the 172 of their papers we have counts for

collaborators

173 papers

cond-mat.quant-gas2023★ 1 cited

Towards quantitative precision in ultracold atoms with functional renormalisation

Bruno M. Faigle-Cedzich, Jan M. Pawlowski, Christof Wetterich

We compute the equation of state, the gap as well as the density fluctuations of a two-component superfluid Fermi gas over the whole range of BEC-BCS crossover at vanishing tempera…

hep-th2022★ 4 cited

Scaling solutions for asymptotically free quantum gravity

Saswato Sen, Christof Wetterich, Masatoshi Yamada

We compute scaling solutions of functional flow equations for quantum gravity in a general truncation with up to four derivatives of the metric. They connect the asymptotically fre…

astro-ph.CO2022★ 64 cited

Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions

Adrià Gómez-Valent, Ziyang Zheng, Luca Amendola +2

Some cosmological models with non-negligible dark energy fractions in particular windows of the pre-recombination epoch are capable of alleviating the Hubble tension quite efficien…

hep-ph2022★ 5 cited

Gluon condensates and effective gluon mass

Jan Horak, Friederike Ihssen, Joannis Papavassiliou +3

Lattice simulations along with studies in continuum QCD indicate that non-perturbative quantum fluctuations lead to an infrared regularisation of the gluon propagator in covariant…

hep-th2021★ 28 cited

Asymptotic freedom and safety in quantum gravity

Saswato Sen, Christof Wetterich, Masatoshi Yamada

We compute non-perturbative flow equations for the couplings of quantum gravity in fourth order of a derivative expansion. The gauge invariant functional flow equation for arbitrar…

astro-ph.CO2021★ 4 cited

Early dark energy in the pre- and post-recombination epochs

Adrià Gómez-Valent, Ziyang Zheng, Luca Amendola +2

Many quintessence models possess scaling or attractor solutions where the fraction of dark energy follows the dominant component in previous epochs of the expansion, or phase trans…