Fetching the paper…
Reading the bibliography…
An interpolating function $\tilde F$ between the $a$-anomaly coefficient in even dimensions and the free energy on an odd-dimensional sphere has been proposed recently and is conjectured to monotonically decrease along any renormalization group flow in continuous dimension $d$.
S. Giombi and I. R. Klebanov, (2014), arXiv:1409.1937 [hep-th]
1937
Earlier work this paper cites.
A. B. Zamolodchikov, JETP Lett. 43
1986
Earlier work this paper cites.
J. L. Cardy, Phys. Lett. B215
1988
Earlier work this paper cites.
L. Girardello, M. Petrini, M. Porrati, and A. Zaffaroni, JHEP 12
1998
Earlier work this paper cites.
D. Z. Freedman, S. S. Gubser, K. Pilch, and N. P. Warner, Adv. Theor. Math. Phys. 3
1999
Earlier work this paper cites.
C. Imbimbo, A. Schwimmer, S. Theisen, and S. Yankielowicz, Class.Quant.Grav. 17
2000
Earlier work this paper cites.
A. Schwimmer and S. Theisen, Nucl.Phys. B801
2008
Cited alongside, same era.
R. C. Myers and A. Sinha, Phys. Rev. D82
2010
Cited alongside, same era.
Z. Komargodski and A. Schwimmer, JHEP 1112
2011
Cited alongside, same era.
D. L. Jafferis, I. R. Klebanov, S. S. Pufu, and B. R. Safdi, JHEP 1106
2011
Cited alongside, same era.
I. R. Klebanov, S. S. Pufu, and B. R. Safdi, JHEP 1110
2011
Cited alongside, same era.
H. Casini, M. Huerta, and R. C. Myers, JHEP 1105
2011
Later among the works it cites.
R. C. Myers and A. Sinha, JHEP 1101
2011
Later among the works it cites.
2012
Later among the works it cites.
H. Casini and M. Huerta, Phys.Rev. D85
2012
Later among the works it cites.
2013
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
We define the stress-energy tensor by T μ ν ≡ 2 g δ I δ g μ ν T_{\mu\nu}\equiv\frac{2}{\sqrt{g}}\frac{\delta I}{\delta g^{\mu\nu}} for an action I I . The Euler density is normalized to be ∫ S d d d x g E d = 2 \intop\nolimits_{S^{d}}d^{d}x\sqrt{g}E_{d}=2
Cited in the paper.
There is no sign factor ( − 1 ) d / 2 (-1)^{d/2} in the right hand side because our convention of the a a -anomaly ( 1
Cited in the paper.
S. Ryu and T. Takayanagi, Phys.Rev.Lett. 96
Cited in the paper.
S. Ryu and T. Takayanagi, JHEP 0608
Cited in the paper.
The null energy condition T μ ν ξ μ ξ ν ≥ 0 T_{\mu\nu}\xi^{\mu}\xi^{\nu}\geq 0 is crucial in the proof of the holographic c c -theorem [ 16 , 17 , 18 ] where the d d -dimensional null vector ξ \xi has only two non-zero components ξ z \xi^{z} and ξ t \xi^{t} . Thus defining a formal null vector ξ = ( ξ z , ξ t , 0 , ⋯ , 0 ) \xi=(\xi^{z},\xi^{t},0,\cdots,0) in continuous d d dimensions, the proof can be carried over for d ≥ 1 d\geq 1
Cited in the paper.