2015
DOI: 10.48550/arxiv.1508.04038
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

Fluid/gravity correspondence: A nonconformal realization in compactified D4 branes

Chao Wu,
Yidian Chen,
Mei Huang

Abstract: We develop the framework of boundary derivative expansion (BDE) formalism of fluid/gravity correspondence in compactified D4-brane system, which is a nonconformal background used in top-down holographic QCD models. Such models contain the D4-D6 model and the Sakai-Sugimoto (SS) model, with the background of the compactified black D4 branes under the near horizon limit. By using the dimensional reduction technique, we derive a 5D Einstein gravity minimally coupled with 3 scalar fields from the 10D D4-brane back… Show more

Help me understand this report
View published versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
2

Citation Types

2
59
0

Year Published

2016
2016
2019
2019

Publication Types

Select...
5

Relationship

3
2

Authors

Journals

citations
Cited by 6 publications
(61 citation statements)
references
References 56 publications
2
59
0
Order By: Relevance
“…Re-expressed (2.16) in Eddington-Finkelstein coordinates dv = dt + dr r 3/2 f (r) with the coordinates are boosted as dv → −u µ dx µ , dx i → P i µ dx µ , one will 4 Q4 is defined through the normalization condition for F4: 2κ 2 µ4Nc = S 4 F4, where 2κ 2 = (2π) 7 l 8 s and µ4 = ((2π) 4 l 5 s ) −1 is the D4-brane charge. 5 This has been explained in [57]. One can calculate the Ricci scalar and the square of the Rieman tensor which separately gives R = − 5(14r 3 +r 3 H ) 6r 11/3 and RMNP QR M NP Q = 25(62r 6 +2r 3 r 3 H +125r 6 H ) 108r 22/3 , from which we can easily see that at r → 0, both of these two approach to zero.…”
Section: Brief Review Of the First Ordermentioning
confidence: 92%
See 4 more Smart Citations
“…Re-expressed (2.16) in Eddington-Finkelstein coordinates dv = dt + dr r 3/2 f (r) with the coordinates are boosted as dv → −u µ dx µ , dx i → P i µ dx µ , one will 4 Q4 is defined through the normalization condition for F4: 2κ 2 µ4Nc = S 4 F4, where 2κ 2 = (2π) 7 l 8 s and µ4 = ((2π) 4 l 5 s ) −1 is the D4-brane charge. 5 This has been explained in [57]. One can calculate the Ricci scalar and the square of the Rieman tensor which separately gives R = − 5(14r 3 +r 3 H ) 6r 11/3 and RMNP QR M NP Q = 25(62r 6 +2r 3 r 3 H +125r 6 H ) 108r 22/3 , from which we can easily see that at r → 0, both of these two approach to zero.…”
Section: Brief Review Of the First Ordermentioning
confidence: 92%
“…If the reader wants to learn more about it, we recommend her/him to Ref. [57], where we develop a nonconformal version of the fluid/gravity correspondence by using the compactified, near-extremal black D4-brane.…”
Section: Brief Review Of the First Ordermentioning
confidence: 99%
See 3 more Smart Citations