Theoretical estimates of the critical exponents of the superfluid transition in 4He by lattice methods

We improve the theoretical estimates of the critical exponents for the three-dimensional XY universality class that apply to the superfluid transition in 4He along the λ line of its phase diagram. We obtain the estimates α=−0.0151(3), ν=0.6717(1), η=0.0381(2), γ=1.3178(2), β=0.3486(1), and δ=4.780(1...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Campostrini, Massimo (VerfasserIn) , Hasenbusch, Martin (VerfasserIn) , Pelissetto, Andrea (VerfasserIn) , Vicari, Ettore (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 6 October 2006
In: Physical review. B, Condensed matter and materials physics
Year: 2006, Jahrgang: 74, Heft: 14, Pages: 1-18
ISSN:1550-235X
DOI:10.1103/PhysRevB.74.144506
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevB.74.144506
Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevB.74.144506
Volltext
Verfasserangaben:Massimo Campostrini, Martin Hasenbusch, Andrea Pelissetto, and Ettore Vicari
Beschreibung
Zusammenfassung:We improve the theoretical estimates of the critical exponents for the three-dimensional XY universality class that apply to the superfluid transition in 4He along the λ line of its phase diagram. We obtain the estimates α=−0.0151(3), ν=0.6717(1), η=0.0381(2), γ=1.3178(2), β=0.3486(1), and δ=4.780(1). Our results are obtained by finite-size scaling analyses of high-statistics Monte Carlo simulations up to lattice size L=128 and resummations of 22nd-order high-temperature expansions of two improved models with suppressed leading scaling corrections. We note that our result for the specific-heat exponent α disagrees with the most recent experimental estimate α=−0.0127(3) at the superfluid transition of 4He in a microgravity environment.
Beschreibung:Im Titel ist die Zahl "4" hochgestellt
Gesehen am 05.07.2022
Beschreibung:Online Resource
ISSN:1550-235X
DOI:10.1103/PhysRevB.74.144506