Taylor expansions and Padé approximants for cumulants of conserved charge fluctuations at nonvanishing chemical potentials - INSPIRE

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Taylor expansions and Padé approximants for cumulants of conserved charge fluctuations at nonvanishing chemical potentials

HotQCD

Collaboration

•

D. Bollweg
(
- Columbia U.
)

Feb 18, 2022

15 pages

Published in:

Phys.Rev.D 105 (2022) 7, 074511

Published: Apr 1, 2022

e-Print:

2202.09184 [hep-lat]

DOI:

10.1103/PhysRevD.105.074511 (publication)

View in:

ADS Abstract Service

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Abstract: (APS)

Using high statistics datasets generated in (

2 + 1

)-flavor QCD calculations at finite temperature, we present results for low-order cumulants of net-baryon-number fluctuations at nonzero values of the baryon chemical potential. We calculate Taylor expansions for the pressure (zeroth-order cumulant), the net-baryon-number density (first-order cumulant), and the variance of the distribution on net-baryon-number fluctuations (second-order cumulant). We obtain series expansions from an eighth-order expansion of the pressure and compare these to diagonal Padé approximants. This allows us to estimate the range of values for the baryon chemical potential in which these expansions are reliable. We find

μ_{B} / T \leq 2.5

, 2.0, and 1.5 for the zeroth-, first-, and second-order cumulants, respectively. We, furthermore, construct estimators for the radius of convergence of the Taylor series of the pressure. In the vicinity of the pseudocritical temperature

T_{p c} ≃ 156.5 MeV

, we find

μ_{B} / T ≳ 2.9

at vanishing strangeness chemical potential and somewhat larger values for strangeness neutral matter. These estimates are temperature dependent and range from

μ_{B} / T ≳ 2.2

at

T = 135 MeV

to

μ_{B} / T ≳ 3.2

at

T = 165 MeV

. The estimated radius of convergences is the same for any higher-order cumulant.

Note:

15 pages

potential: chemical
charge: fluctuation
baryon number: density
baryon number: fluctuation
charge: conservation law
pressure
Taylor expansion
strangeness
baryon
temperature dependence

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