2018
DOI: 10.1103/physrevd.98.054014
|View full text |Cite
|
Sign up to set email alerts
|

Fluctuation and dissipation of axial charge from massive quarks

Abstract: In quantum chromodynamics, axial charge is known to be nonconserved due to chiral anomaly and nonvanishing quark mass. In this paper, we explore the role of quark mass in axial charge fluctuation and dissipation. We present two separate calculations of the axial charge correlator, which describe dynamics of axial charge. The first is free quarks at a finite temperature. We find that axial charge can be generated through effective quantum fluctuations in free theory. However, the fluctuation does not follow a r… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

1
19
0

Year Published

2019
2019
2021
2021

Publication Types

Select...
7

Relationship

0
7

Authors

Journals

citations
Cited by 30 publications
(20 citation statements)
references
References 45 publications
1
19
0
Order By: Relevance
“…The ρ tt coupling can also be constrained by LHC and flavor physics. For c γ = 0, tth production constrains O(1) ρ tt [28]. Regardless of the value of c γ , ρ tt can be constrained by B s,d mixing, but it depends on m H ± [29].…”
Section: A General Discussion On Constraintsmentioning
confidence: 99%
“…The ρ tt coupling can also be constrained by LHC and flavor physics. For c γ = 0, tth production constrains O(1) ρ tt [28]. Regardless of the value of c γ , ρ tt can be constrained by B s,d mixing, but it depends on m H ± [29].…”
Section: A General Discussion On Constraintsmentioning
confidence: 99%
“…If the charm quark gets misidentified as b-jet, a sizable ρ cc can mimic bZH signature in pp collision via cg → cA → cZH. However, such possibilities can be excluded with the simultaneous application of c-and b-tagging on the final state event topologies [63].…”
Section: Discussion and Summarymentioning
confidence: 99%
“…For simplicity we utilized the LO µ f i in our analysis and followed Refs. [17][18][19][20] for their explicit expressions. In particular, we focused on two different production modes, the ggF and the V BF in our analysis.…”
Section: Allowed Parameter Spacementioning
confidence: 99%
“…The EBE-AVFD includes fluctuating initial conditions as well as a hadronic cascade stage via UrQMD after the hydrodynamic evolution which accounts for the influence of hadronic re-scatterings and resonance decays. Further improvements of the framework shall address a number of issues, including more accurate determination of axial charge initial conditions [62,63], the fluctuation and dissipation of axial charge during the hydrodynamic evolution [347][348][349][350], as well as the possible generation of the CME current in the pre-equilibrium stage [152].…”
Section: Quantitative Modeling Of Anomalous Chiral Transportmentioning
confidence: 99%