Thursday, May 12, 2022

Emergent Sasaki-Einstein geometry and AdS/CFT






Nice to see folks are still trying to get from quantum ideas to the General theory of Relativity.  my Cloud Cosmology takes a completely different track.  We imagine the act of creation through the conscious creation of the Space Time Pendulum which also creates TIME and naturally floods the cosmos with such pendulums or most likely neutrinos.  Consciousness is part of the content of this imagined cosmos as is TIME.

these then self assemble to produce the spectrum of particles and a cosmology expanding at light speed.  From any such act of creation we have a body of particles left behind traveling sub light.  Reasonably a universe looks like a galaxy or perhaps a star even or possibly a planet.  This is the cosmos i have been observing for decades.

The metric for all these particles are higher ordered Pythagoreans described in my published paper in Physics Essays (AIP). This naturally leaves us with a local Pythagorean geometry and Space Time of the General Theory which is not nearly so important but still complete.

The big breakthrough is in how we handle TIME.  It is literally one page of creation after another.  This will be extremely useful for empirical physics.


Emergent Sasaki-Einstein geometry and AdS/CFT


Nature Communications volume 13, Article number: 365 (2022)

https://www.nature.com/articles/s41467-021-27951-9?mc_cid=cdf33400ef&mc_eid=0fbfc02f32



Abstract


A central problem in any quantum theory of gravity is to explain the emergence of the classical spacetime geometry in some limit of a more fundamental, microscopic description of nature. The gauge/gravity-correspondence provides a framework in which this problem can, in principle, be addressed. This is a holographic correspondence which relates a supergravity theory in five-dimensional Anti-deSitter space to a strongly coupled superconformal gauge theory on its 4-dimensional flat Minkowski boundary. In particular, the classical geometry should therefore emerge from some quantum state of the dual gauge theory. Here we confirm this by showing how the classical metric emerges from a canonical state in the dual gauge theory. In particular, we obtain approximations to the Sasaki-Einstein metric underlying the supergravity geometry, in terms of an explicit integral formula involving the canonical quantum state in question. In the special case of toric quiver gauge theories we show that our results can be computationally simplified through a process of tropicalization.

Introduction


It is expected that a quantum theory of gravity should be able to explain the emergence of the classical spacetime geometry in some limit of a more fundamental, microscopic description of Nature. The AdS/CFT-correspondence (or “gauge/gravity correspondence”) introduced in ref. 1, provides a framework in which this problem can, in principle, be addressed. The AdS/CFT correspondence relates a supergravity theory in the five-dimensional Anti-deSitter space AdS5 to a strongly coupled, rank N, superconformal gauge theory on the 4-dimensional flat boundary {{\mathbb{R}}}^{3,1} of AdS5. This is a holographic correspondence since {{\mathbb{R}}}^{3,1} is the (conformal) boundary of AdS5; hence it relates a gravitational theory in spacetime, to a conformal field theory (without gravity) on the boundary2,3,4. In particular, the classical geometry, i.e., the supergravity vacuum, should therefore emerge from a particular quantum state of the dual gauge theory. The main aim of our work is to make this precise by exhibiting a canonical (i.e., background independent) such quantum state ΨN and by showing that the supergravity vacuum in question emerges from the probability amplitude of ΨN in the t’Hooft limit where the rank N of the gauge group tends to infinity.

In the general setting of minimal supersymmetry, the supergravity vacuum is encoded by a Sasaki–Einstein metric gM on a five-dimensional compact manifold M5,6. On the gauge theory side the {{{{{\mathcal{N}}}}}}=1 superconformal symmetry is encoded by a complex cone Y of six real dimensions. This means that Y is a complex affine algebraic variety with a unique singular point y0 (the tip of the cone), endowed with a repulsive holomorphic {{\mathbb{R}}}_{ \,{ > }\,0}-action, representing the conformal dilatation symmetry of the gauge theory. In the AdS/CFT correspondence the compact manifold M on the supergravity side arises as to the base of the complex cone Y of the gauge theory:

M:=\left(Y-\{{y}_{0}\}\right)/{{\mathbb{R}}}_{ \,{ > }\,0}.

(1)

The complex cone (Y,{{\mathbb{R}}}_{ \,{ > }\,0}) comes with a canonical holomorphic three-form Ω which is homogeneous of degree 3. Such a space Y is often called a Calabi–Yau cone in the literature and is usually endowed with a conical Calabi–Yau metric gY, i.e., a Ricci flat conical Kähler metric, as well as a radial coordinate r, arising as the distance to the vertex point y0 with respect to the Calabi–Yau metric gY. However, in the background independent formalism that we shall stress, the complex cone Y is not, a priori, endowed with any metric. This is crucial since our aim is to show how a metric emerges from the metric-independent BPS-sector of the gauge theory. Recall that BPS-states can be represented by holomorphic polynomial functions on the vacuum moduli space of the rank N gauge theory, whose mesonic branch is given by the symmetric product YN/SN, where SN denotes the symmetric group on N elements. The vacuum moduli space can thus be described in purely complex algebro-geometric terms7,8,9.

In this work, we show that by imposing all the manifest symmetries of the rank N gauge theory one naturally arrives at a canonical quantum BPS-state ΨN. More precisely, ΨN can be realized as a wave function on the vacuum moduli space YN/SN and its amplitude ∣ΨN∣2 induces a measure on YN:
| {{{\Psi }}}_{N}({y}_{1},...,{y}_{N}){| }^{2}{\left({{\Omega }}\wedge \bar{{{\Omega }}}\right)}^{\otimes N}

(2)

which is SN–invariant and {{\mathbb{R}}}_{ \,{ > }\,0}-invariant along each factor of YN (here \bar{{{\Omega }}} denotes the conjugate of Ω multiplied by −i so that {{\Omega }}\wedge \bar{{{\Omega }}} is a volume form on Y). Somewhat surprisingly the state ΨN does not appear to have been considered before in the literature. Its explicit expression is given in Section II C, where the relation to the BPS-sector of the gauge theory is also explained. By quotienting out the conformal {{\mathbb{R}}}_{ \,{ > }\,0}-symmetry, we arrive at a measure on MN/SN, which after normalization yields a canonical probability measure. Equivalently, we obtain a canonical ensemble of N “point-particles” on M. We show that a Sasaki–Einstein metric gM on M emerges from the canonical ensemble in the large N-limit. In a little more detail, our construction goes as follows. First, the volume form dVM of gM emerges, after which the metric gM can be recovered from dVM in a standard manner (by simply differentiating dVM twice). In fact, in the course of this procedure an N-dependent radial function rN on Y naturally appears in an intermediate step and it induces a “quantum correction” {g}_{M}^{(N)} to the Sasaki–Einstein metric gM on M. In this way, a limiting radial coordinate r on Y emerges from the gauge theory as N → ∞. From the perspective of the AdS/CFT correspondence, the radial coordinate r on Y corresponds to the radial coordinate on AdS5 and thus our work reveals how the geometry of AdS5, transversal to the conformal boundary {{\mathbb{R}}}^{3,1}, naturally emerges from the gauge theory. A “spin-off effect” of this procedure is that it also produces (by a kind of back-reaction) a conical Calabi–Yau metric on Y, namely the cone over gM, whose distance to the vertex point y0 is precisely r. It should be stressed that there are very few cases known where the Sasaki–Einstein metric gM on M can be explicitly computed (but see ref. 10 for a notable family of exceptions). Thus an important feature of our construction is that it furnishes canonical approximations {g}_{M}^{(N)} of Sasaki–Einstein metrics, encoded in terms of algebro-geometric data through an explicit integral formula. These can be numerically computed using Monte-Carlo methods, as detailed in section “Specialization to the toric case” for the toric case. Some relations to previous results and ideas for future work are discussed in section “Discussion”.

Results

Background: AdS/CFT and BPS-states

Recall that the low-energy dynamics of a general supersymmetric gauge theory is controlled by the moduli space of classical vacua {{{{{\mathcal{M}}}}}}. The space {{{{{\mathcal{M}}}}}} may be defined as the critical points, modulo complex gauge equivalence, of the superpotential W appearing in the (UV) Lagrangian of the gauge theory11,12. Moreover, the BPS-operators of the gauge theory, i.e., the local operators preserving half of the supercharges, may be represented by holomorphic, polynomial functions on {{{{{\mathcal{M}}}}}}. They thus form a ring known as the chiral ring of the gauge theory, which is graded by the R-charge. In the superconformal case, the BPS-operators can be viewed as states by the usual operator-state correspondence in CFT. The BPS-states are chiral primary states and saturate the BPS-bound,
{{\Delta }}=\frac{3}{2}R,

(3)

where Δ denotes the conformal dimension. As a consequence, the BPS-sector tends to be robust under non-perturbative corrections and can thus be used to probe the strong-coupling regime of the gauge theory.

In the setting of the AdS/CFT correspondence, the mesonic branch of the moduli space of vacua of the rank N gauge theory is the symmetric product8
{{{{{{\mathcal{M}}}}}}}_{N}={{{\mbox{Sym}}}}^{N}Y={Y}^{N}/{S}_{N},

(4)

where Y is a complex cone. From the string theory perspective, this space parametrizes the transverse positions of ND3-branes inside Y. For example, in the maximally supersymmetric SU(N)-case, the superpotential W(Z1, Z2, Z3) is defined on 3 complex N × N matrices Zi (transforming in the adjoint representation) and W=Tr\left({Z}_{1}[{Z}_{2},{Z}_{3}]\right). Thus the mesonic vacuum moduli space {{{{{{\mathcal{M}}}}}}}_{N} may be parametrized by the set {({{\mathbb{C}}}^{3})}^{N}/{S}_{N} of joint eigenvalues of (Z1, Z2, Z3), showing that, indeed, Y={{\mathbb{C}}}^{3} in this case.

The mesonic BPS-sector in the maximally supersymmetric case is isomorphic to the ring of holomorphic, polynomial functions on {({{\mathbb{C}}}^{3})}^{N}/{S}_{N}. Gauge theories with minimal supersymmetries may be constructed using quivers, encoding the matter content of the Lagrangian, as well as the superpotential13. In general, this is a highly non-trivial task, but our approach only requires that the corresponding moduli space of classical vacua, encoded by the complex cone Y, is given.
Mathematical prerequisites: complex-geometric setup

In this section we provide complex-geometric background, emphasizing a background-independent (i.e., metric-independent) perspective; see ref. 14 and the monograph15 for the more standard metric-dependent point of view. Let Y be a three-dimensional complex algebraic affine variety with an isolated singularity y0. Concretely, Y may be realized as the zero-locus of a collection of holomorphic polynomials on some complex space {{\mathbb{C}}}^{M}. Denote by J the induced complex structure on the regular locus Y − {y0}. Assume that Y is endowed with a

A repulsive holomorphic {{\mathbb{R}}}_{ \,{ > }\,0}-action that fixes y0


a holomorphic top-form Ω, defined on the non-singular locus Y − {y0}, which is homogeneous of degree 3 with respect to the {{\mathbb{R}}}_{ \,{ > }\,0}-action on Y. 

Such a space Y will here simply be called a complex cone, though it is often called a Calabi–Yau cone in the physics literature and an affine Gorenstein cone in the mathematics literature. The form Ω is uniquely determined up to a multiplicative constant and can often be written down explicitly.

The vector field on Y generating the {{\mathbb{R}}}_{ \,{ > }\,0}-action will be called the dilatation vector field and denoted by δ. Rotating δ with the complex structure J on Y yields another vector field that we shall denote by ξ: 
\xi =J\delta .

(5)

The space {{{{{\mathcal{O}}}}}}(Y) of holomorphic functions on Y decomposes with respect to the {{\mathbb{R}}}_{ \,{ > }\,0}-action:
{{{{{\mathcal{O}}}}}}(Y)=\mathop{\bigoplus}\limits_{k=0,1,...}{{{{{{\mathcal{O}}}}}}}_{{\lambda }_{k}}(Y),\ \ \ \ 0={\lambda }_{0}\le {\lambda }_{1}\le \cdots,

(6)

where {{{{{{\mathcal{O}}}}}}}_{{\lambda }_{k}}(Y) is the vector space of holomorphic (polynomial) functions, which are homogeneous of degree λk with respect to {{\mathbb{R}}}_{ \,{ > }\,0}. From the perspective of the underlying superconformal gauge theory, the infinitesimal {{\mathbb{R}}}_{ \,{ > }\,0}-action δ represents the conformal dilatation and \frac{2}{3}\xi represents the R-symmetry (the factor 2/3 ensures that Ω has the same R-charge, 2, as the chiral superspace volume form d2θ, where θ denotes fermionic coordinates of positive chirality). Thus, Eq. (5) is the complex-geometric realization of the BPS-relation (3) and the summands {{{{{{\mathcal{O}}}}}}}_{{\lambda }_{k}}(Y) in the decomposition (6) are thus BPS-states of dimension and R-charge equal to λk.

The base of a complex cone Y is the compact five-dimensional manifold M defined by
M:=\left(Y-\{{y}_{0}\}\right)/{{\mathbb{R}}}_{ \,{ > }\,0}.

(7)

Thus, M is the base of the fibration (Y − {y0}) → M obtained by quotienting out the {{\mathbb{R}}}_{ \,{ > }\,0}-action on Y. Since the vector field ξ on Y commutes with the generator of the {{\mathbb{R}}}_{ \,{ > }\,0}-action it induces a vector field on M that we denote by the same symbol ξ—known as the Reeb vector field on M in the mathematics literature. A metric gM on M is said to define a Sasaki–Einstein metric on (M, ξ) if gM has constant Ricci curvature, normalized so that it coincides with the Ricci curvature of the standard round metric on the unit-sphere, and is compatible, in a certain sense, with the complex structure on Y. 

The compatibility in question can be formulated in various ways, but the crucial point for our purposes is that a Sasaki–Einstein metric gM can be explicitly recovered from its volume form {{{\mathrm{d}}}}{V}_{{g}_{M}} as follows. First observe that {{{\mathrm{d}}}}{V}_{{g}_{M}} induces a radial function, i.e., positive function r on Y which is one-homogeneous with respect to the {{\mathbb{R}}}_{ \,{ > }\,0}-action:
r:={\left(\frac{{\iota }_{\delta }{{\Omega }}\wedge \bar{{{\Omega }}}}{{{{\mathrm{d}}}}{V}_{{g}_{M}}}\right)}^{1/6},

(8)

where we have identified the volume form {{{\mathrm{d}}}}{V}_{{g}_{M}} on M with its pull-back to Y. The metric gM on M with volume form {{{\mathrm{d}}}}{V}_{{g}_{M}} is a Sasaki–Einstein metric iff the corresponding radial function r on Y solves the following PDE, after perhaps rescaling r, 
{\left(d{d}^{c}({r}^{2})\right)}^{3}={{\Omega }}\wedge \overline{{{\Omega }}},\ {d}^{c}:={J}^{* }d

(9)

on the regular locus Y − {y0} of Y. Here, d denotes the exterior derivative and dc denotes its “rotation” by the complex structure J, so that ddc(r2) defines a two-form on Y and thus the three-fold exterior product {\left(d{d}^{c}({r}^{2})\right)}^{3} defines a six-form on Y. 

The PDE (9) is the celebrated Calabi–Yau equation on the complex cone Y; it is equivalent to the condition that the conical Kähler metric
{g}_{Y}:=d{d}^{c}({r}^{2})(\cdot ,J\cdot ),

(10)

on Y is a Calabi–Yau metric, i.e., the Ricci curvature of gY vanishes. Finally, gM may be explicitly recovered by identifying M with the level set {r = 1} in Y and letting gM be the restriction of gY to the level set {r = 1}. 

It is important to emphasize that, in general, the base (M, ξ) of a complex cone (Y,{{\mathbb{R}}}_{ \,{ > }\,0}) may not admit a Sasaki–Einstein metric9,14,16. Equivalently, this means that a complex cone may not admit a conical Calabi–Yau metric and hence no radial solution r to the Calabi–Yau equation (9). Indeed, by16 there exists a Sasaki–Einstein metric on (M, ξ) iff the complex cone (Y,{{\mathbb{R}}}_{ \,{ > }\,0}) is K-stable. This is a purely algebro-geometric condition.

As shown in ref. 17 the K-stability of Y can be viewed as a generalized form of the maximization condition for the a-central charge of the SCFT. This means that, in general, there are obstructions to the existence of a SCFT with a given {{\mathbb{R}}}_{ \,{ > }\,0}-graded mesonic chiral ring {{{{{\mathcal{O}}}}}}({Y}^{N}/{S}_{N}). In the present approach, a different, but conjecturally equivalent, stability type condition naturally appears, which is a variant of the notion of Gibbs stability introduced in the context of Fano manifolds in ref. 18.
Main results: emergent geometry

According to the AdS/CFT-correspondence the classical supergravity vacuum geometry in AdS5 should emerge from some limit of a quantum state in the dual CFT gauge theory on the boundary. Concretely, in the present setting the non-trivial part of the supergravity vacuum in question is encoded by a Sasaki–Einstein metric gM on the internal compact space M, corresponding to the base of the complex cone Y of the dual gauge theory6. Hence, we want to show that the Sasaki–Einstein metric gM on M emerges in a certain “large N-limit” of a specific (and background free) quantum BPS-state ΨN in the dual-rank N gauge theory.

First, recall that Y is endowed with a holomorphic top-form Ω and hence one can endow the mesonic classical vacuum moduli space YN/SN with the volume form {({{\Omega }}\wedge \overline{{{\Omega }}})}^{\otimes N}. Let {\psi }_{1},\ldots ,{\psi }_{{N}_{k}} be a maximal number of linearly independent mesonic BPS-states for the rank 1 gauge theory with the same R-charge λk. In other words, {\psi }_{1},\ldots ,{\psi }_{{N}_{k}} form a basis in the space {{{{{{\mathcal{O}}}}}}}_{{\lambda }_{k}}(Y) of holomorphic functions on Y with the same charge λk. Denote by Ψdet the corresponding Slater determinant, i.e., the totally antisymmetric holomorphic function on {Y}^{{N}_{k}} given by
{{{\Psi }}}_{{{\mbox{det}}}}({y}_{1},\ldots ,{y}_{{N}_{k}}):=\mathop{\sum}\limits_{\sigma \in {S}_{{N}_{k}}}{(-1)}^{| \sigma | }{\psi }_{\sigma (1)}({y}_{1})\cdots {\psi }_{\sigma ({N}_{k})}({y}_{{N}_{k}}).

(11)

The function Ψdet is independent of the choice of bases in {{{{{{\mathcal{O}}}}}}}_{{\lambda }_{k}}(Y) up to an overall multiplicative constant. It thus defines a baryonic BPS-state in the rank Nk gauge theory8,19.

We aim to construct a symmetric measure on the mesonic classical vacuum moduli space {Y}^{{N}_{k}}/{S}_{{N}_{k}}, which is invariant under the conformal {{\mathbb{R}}}_{ \,{ > }\,0}-action on each factor. One might be tempted to try with the density ∣Ψdet∣2, but this is unfortunately not {({{\mathbb{R}}}_{ \,{ > }\,0})}^{{N}_{k}}-invariant. The resolution is to simply take a suitable fractional power of the Slater determinant, namely
{{{\Psi }}}_{{N}_{k}}:={{{\Psi }}}_{\,{{\mbox{det}}}\,}^{-3/{\lambda }_{k}}.

(12)

Then, an {({{\mathbb{R}}}_{ \,{ > }\,0})}^{{N}_{k}}-invariant measure on YN/SN is given by the combination
| {{{\Psi }}}_{{N}_{k}}({y}_{1},\cdots \ ,{y}_{{N}_{k}}){| }^{2}\,\,{({{\Omega }}\wedge \overline{{{\Omega }}})}^{\otimes {N}_{k}}.

(13)

This measure is both invariant under the {S}_{{N}_{k}} permutation symmetry and the conformal {{\mathbb{R}}}_{ \,{ > }\,0}-symmetry, as well as the R-symmetry. However, since Y is non-compact, the integral of this measure over {Y}^{{N}_{k}}/{S}_{{N}_{k}} diverges. To circumvent this problem, we simply quotient by the {({{\mathbb{R}}}_{ \,{ > }\,0})}^{{N}_{k}}-action to get an induced measure on the compact space {M}^{{N}_{k}}/{S}_{{N}_{k}}. To be specific, contracting the top-form {{\Omega }}\wedge \overline{{{\Omega }}} on Y with the dilatation vector field δ yields a 5-form {\iota }_{\delta }({{\Omega }}\wedge \overline{{{\Omega }}}) on Y. Thus, the {({{\mathbb{R}}}_{ \,{ > }\,0})}^{{N}_{k}}-invariant form
| {{{\Psi }}}_{{N}_{k}}({y}_{1},\cdots \ ,{y}_{{N}_{k}}){| }^{2}{({\iota }_{\delta }{{\Omega }}\wedge \overline{{{\Omega }}})}^{\otimes {N}_{k}}

(14)

maybe identified with a measure on the compact quotient space {M}^{{N}_{k}}/{S}_{{N}_{k}}. Finally, the canonical probability measure {{{\mathrm{d}}}}{{\mathbb{P}}}_{{N}_{k}} on {M}^{{N}_{k}}/{S}_{{N}_{k}} is defined by
{{{\mathrm{d}}}}{{\mathbb{P}}}_{{N}_{k}}:=\frac{1}{{{{{{{\mathcal{Z}}}}}}}_{{N}_{k}}}| {{{\Psi }}}_{{N}_{k}}{| }^{2}{\left({\iota }_{\delta }({{\Omega }}\wedge \overline{{{\Omega }}})\right)}^{\otimes {N}_{k}},

(15)

where
{{{{{{\mathcal{Z}}}}}}}_{{N}_{k}}:=\int\nolimits_{{M}^{{N}_{k}}/{S}_{{N}_{k}}}| {{{\Psi }}}_{{N}_{k}}{| }^{2}{\left({\iota }_{\delta }({{\Omega }}\wedge \overline{{{\Omega }}})\right)}^{\otimes {N}_{k}}.

(16)

Note that in (15) we have made the implicit assumption that {{{{{{\mathcal{Z}}}}}}}_{{N}_{k}} is finite. Since | {{{\Psi }}}_{{N}_{k}}{| }^{2} blows-up along a hypersurface in {Y}^{{N}_{k}}/{S}_{{N}_{k}}, namely the zero-locus of the Slater determinant Ψdet, this is actually a very non-trivial condition. We interpret it as a consistency condition (which turns out to be related to the mathematical notions of K-stability and Gibbs stability).

Since ΨN is holomorphic away from its singularity locus in YN/SN (the vanishing locus of {{{\Psi }}}_{\det }) the state ΨN can be viewed as a bound state of BPS-states in the rank N gauge theory.

We emphasize that by “canonical” we mean that the definition of {{{\mathrm{d}}}}{{\mathbb{P}}}_{{N}_{k}} is background independent, in the sense that it does not depend on any underlying metric on Y or M. It only depends on the complex structure J on the classical vacuum moduli space and the {{\mathbb{R}}}_{ \,{ > }\,0}-action and thus only on the superconformal symmetry of the rank N-gauge theory. This is a crucial point for describing the emergence of the classical Sasaki–Einstein metric gM on M, which is our main focus.

We have also restricted the values of the rank N to be a sequence of integers
{N}_{k}:=\dim {{{{{{\mathcal{O}}}}}}}_{{\lambda }_{k}}(Y),

(17)

i.e., the multiplicity of the R-charge λk. This can be seen as a quantization condition. As is well-known, in the quasi-regular case (discussed in the next section) Nk is a polynomial in k of the form,
{N}_{k}=\frac{{\lambda }_{k}^{2}}{2}V+{{{{{\mathcal{O}}}}}}({k}^{1}),\ \ {\lambda }_{k} \sim k,\ \ k\to \infty

(18)

where the positive number V is an algebraic invariant of the complex cone (Y,{{\mathbb{R}}}_{ \,{ > }\,0}), known as its volume9,14,16.

Assume, for simplicity, that the complex cone (Y,{{\mathbb{R}}}_{ \,{ > }\,0}) associated to the gauge theory is quasi-regular. A complex cone (Y,{{\mathbb{R}}}_{ \,{ > }\,0}) is quasi-regular if (up to a rescaling) the {{\mathbb{R}}}_{ \,{ > }\,0}-action on Y can be complexified to a holomorphic {{\mathbb{C}}}^{\times }-action. Denote by {{{\mathrm{d}}}}{{\mathbb{P}}}_{N}^{(1)} the probability measure on M defined as the 1 − point correlation measure of the canonical ensemble ({{{\mathrm{d}}}}{{\mathbb{P}}}_{N},{M}^{N}/{S}_{N}) introduced in the previous section. In other words, {{{\mathrm{d}}}}{{\mathbb{P}}}_{N}^{(1)} is obtained by “integrating out” all but one of the factors of MN: 
{{{\mathrm{d}}}}{{\mathbb{P}}}_{N}^{(1)}(y)\,=\, \frac{1}{{{{{{{\mathcal{Z}}}}}}}_{N}}\int\nolimits_{{M}^{N-1}/{S}_{N-1}}| {{{\Psi }}}_{{N}_{k}}(y,{y}_{2},...,{y}_{N}){| }^{2}\\ \times {\left({\iota }_{\delta }({{\Omega }}\wedge \overline{{{\Omega }}})\right)}^{\otimes N-1}.

(19)

Our main conjecture can now be stated as follows:

Conjecture A: Assume that the canonical ensemble ({{{\mathrm{d}}}}{{\mathbb{P}}}_{N},{M}^{N}/{S}_{N}) is well-defined, i.e., that {{{{{{\mathcal{Z}}}}}}}_{N} \, < \, \infty . Then(i)

The one-point correlation measure d{{\mathbb{P}}}_{N}^{(1)} converges, as N → ∞, to the volume form dVM of a Sasaki–Einstein metric gM on (M, ξ), normalized to have unit-volume,
\mathop{\lim }\limits_{N\to \infty }{{{\mathrm{d}}}}{{\mathbb{P}}}_{N}^{(1)}={{{\mathrm{d}}}}{V}_{M};

(20)
(ii)

The sequence of radial functions
{r}_{N}:={\left(\frac{{{{\mathrm{d}}}}{{\mathbb{P}}}_{N}^{(1)}}{{\iota }_{\delta }({{\Omega }}\wedge \overline{{{\Omega }}})}\right)}^{-1/6}

(21)

on the complex cone (Y, R>0) converges, as N → ∞, toward the radial function r of the Calabi–Yau metric gY on Y corresponding to the Sasaki–Einstein metric gM on (M, ξ).
(iii)

Conversely, if there exists a unique Sasaki–Einstein metric gM on M, then {{{{{{\mathcal{Z}}}}}}}_{N} \; < \; \infty .

We emphasize that for finite N, the radial function rN yields an explicit approximation {g}_{M}^{(N)} to the Sasaki–Einstein metric gM on M by identifying M with the level set {rN = 1} and setting
{g}_{M}^{(N)}=d{d}^{c}{({r}_{N}^{2})}_{| M}(\cdot ,J\cdot )

(22)

(c.f. Eq. (10)). Hence, part (ii) of the conjecture is equivalent to
\mathop{\lim }\limits_{N\to \infty }{g}_{M}^{(N)}={g}_{M},

(23)

which is the sought-after emergence of the Sasaki–Einstein metric on M in the large N limit.

To be mathematically precise, the convergence statements in the conjecture are supposed to hold in the standard weak topologies. In fact, we make the stronger conjecture that the random measure {N}^{-1}\mathop{\sum }\nolimits_{i = 1}^{N}{\delta }_{{x}_{i}} on the canonical ensemble converges in law toward the deterministic measure dVM. Below we will prove a β-deformed version of this conjecture.

We first introduce a real-analytic family of probability measures {{{\mathrm{d}}}}{{\mathbb{P}}}_{N,\beta } on MN/SN, defined for a real parameter β, such that {{{\mathrm{d}}}}{{\mathbb{P}}}_{N,\beta } coincides with d{{\mathbb{P}}}_{N} for β = −1, if {{{{{{\mathcal{Z}}}}}}}_{N} \, < \, \infty . To this end, fix a background radial function r0 on Y. We can then identify the base M:=\left(Y-\{{y}_{0}\}\right)/{{\mathbb{R}}}_{ \,{ > }\,0} of the cone Y with the level set \left\{{r}_{0}=1\right\} in Y and define d{{\mathbb{P}}}_{N,\beta } as follows:
{{{\mathrm{d}}}}{{\mathbb{P}}}_{N,\beta }:=\frac{1}{{{{{{{\mathcal{Z}}}}}}}_{N,\beta }}{\left|{{{\Psi }}}_{\det }{({y}_{1},{y}_{2},...,{y}_{N})}^{2}\right|}^{\frac{3\beta }{{\lambda }_{k}}}{{{\mathrm{d}}}}{V}_{0}^{\otimes N},

(24)

where dV0 denotes the volume form on M obtained by restricting the five-form {\iota }_{\delta }{{\Omega }}\wedge \bar{{{\Omega }}} to the level set \left\{{r}_{0}=1\right\} and {{{{{{\mathcal{Z}}}}}}}_{N,\beta } is the corresponding normalization constant (recall that N is the multiplicity of the charge λk). The parameter β can be viewed as a regularization parameter, since {{{{{{\mathcal{Z}}}}}}}_{N,\beta } is automatically finite when β > 0 (or slightly negative). However, it should be stressed that it is only in the canonical case β = −1 that the probability measure (24) is independent of the choice of radial function r0. Let rN,β be the radial function on Y defined by
{r}_{N,\beta }:={\left(\frac{{{{\mathrm{d}}}}{{\mathbb{P}}}_{N,\beta }^{(1)}}{{{{\mathrm{d}}}}{V}_{0}}\right)}^{1/6\beta }{r}_{0}

(25)

(coinciding with rN when β = − 1) and denote by {g}_{M,\beta }^{(N)} the corresponding metric on M, obtained by replacing the radial function rN in Eq. (22) with rN,β. We then have:

Theorem B: For each β > 0, there exists(i)

a volume form μβ on M such that
\mathop{\lim }\limits_{N\to \infty }{{{\mathrm{d}}}}{{\mathbb{P}}}_{N,\beta }^{(1)}={\mu }_{\beta },

(ii)

a radial function rβ on Y such that
\mathop{\lim }\limits_{N\to \infty }{r}_{N,\beta }={r}_{\beta },

(iii)

and a Sasaki metric gM,β on M such that
\mathop{\lim }\limits_{N\to \infty }{g}_{M,\beta }^{(N)}={g}_{N,\beta }.


Moreover, if (M, ξ) admits a Sasaki–Einstein metric, then rβ and gM,β extend real-analytically to [−1, ∞] and setting β = − 1 yields a Sasaki–Einstein metric gM on M. 

The proof is given in §IV. In the course of the proof, we will show that the square of the limiting radial function rβ is the unique conical Kähler potential on Y solving the following PDE on Y − {y0}: 
{(d{d}^{c}{r}_{\beta }^{2})}^{3}={\left(\frac{{r}_{\beta }^{2}}{{r}_{0}^{2}}\right)}^{3(\beta +1)}{{\Omega }}\wedge \bar{{{\Omega }}}.

(26)

In particular, for β = −1 this is indeed the Calabi–Yau equation (9) for the radial function r corresponding to a Sasaki–Einstein metric gM on M. 
Finiteness properties of the normalizing constant

Loosely speaking, Theorem B thus shows that Conjecture A holds after the analytic continuation. More precisely, it shows that Conjecture A holds under the assumption that the order of taking the limits Nk → ∞ and β → −1 may be interchanged. By a physics level of rigor Conjecture A may thus be considered as established. However, we do expect that the introduction of the parameter β is not needed and, in particular, that {{{{{{\mathcal{Z}}}}}}}_{N} \, < \, \infty if and only if (M, ξ) admits a unique Sasaki–Einstein metric. In the case when the Sasaki–Einstein metric is not unique, i.e., when the Lie algebra {\mathfrak{g}}(Y,\xi ) of the automorphism group of (Y, ξ) is non-trivial20, we conjecture that {{{{{{\mathcal{Z}}}}}}}_{N,\beta } \, < \, \infty for any β > −1 when N is sufficiently large. The “only if direction” can be deduced from recent mathematical results in complex geometry for complex cones Y of any dimension, as will be shown elsewhere. Proving the remaining direction appears, however, to be very challenging, except in the case when Y has complex dimension two, where a direct proof of Conjecture A can be given.

For example, when Y={{\mathbb{C}}}^{2} realizing M as the Hopf fibration over the two-sphere S2 and factorizing {{{\Psi }}}_{\det }({x}_{1},{x}_{2},...,{x}_{N}) reveals that {{{{{{\mathcal{Z}}}}}}}_{N,\beta } can be expressed as the configurational partition function for N particles on S2 interacting by the 2D-gravitational force with a mean-field scaling:
{{{{{{\mathcal{Z}}}}}}}_{N,\beta }={C}_{N}\int\nolimits_{{({S}^{2})}^{N}}\mathop{\prod}\limits_{1\le i\ne j\le N}\parallel \! {x}_{i}-{x}_{j}{\parallel }_{{{\mathbb{R}}}^{3}}^{\frac{2\beta }{N-1}}{{{\mathrm{d}}}}{A}^{\otimes N},

(27)

expressed in terms of the restriction to S2 of the Euclidean norm on {{\mathbb{R}}}^{3} (c.f. Eq. (36)). Applying the arithmetic-geometric means inequality reveals that the integral is finite precisely when β > −(1 − 1/N). A similar argument applies to any Y of complex dimension two, using that Y is a Kleinian singularity, i.e., Y={{\mathbb{C}}}^{2}/G for a finite subgroup G of SU(2) and thus that M is a Seifert fibration over S2, branched over three points (in this case {{{{{{\mathcal{Z}}}}}}}_{N,\beta } \; < \; \infty for β = −1-when N is sufficiently large-since {\mathfrak{g}}(Y,\xi ) is trivial; details will appear elsewhere). For higher-dimensional Y the Slater determinant {{{\Psi }}}_{\det }({x}_{1},{x}_{2},...,{x}_{N}) can not, however, be factorized. But a condition ensuring that our canonical partition function {{{{{{\mathcal{Z}}}}}}}_{N} is finite for any N is that Y is an exceptional singularity21,22. For example, there are exactly (up to conjugation) five cases of exceptional (non-isolated) singularities of the form Y={{\mathbb{C}}}^{3}/G, for G a finite subgroup of SL({\mathbb{C}},3); notably Klein’s simple group of order 168, PSL(2, 7),21, Cor 3.15. See ref. 23 for the construction of the matter content and gauge groups of the corresponding gauge theories; the quiver graphs for the five “exceptional” groups G appear in figure 5 in refs. 23.

Moreover, a list of three-dimensional exceptional quasi-homogeneous (isolated) hypersurface singularities in {{\mathbb{C}}}^{4} is given in ref. 22, Cor 1.1. Consider for example the case when Y is a Briskorn–Pham singularity:
\left\{{Z}_{0}^{{a}_{0}}+{Z}_{1}^{{a}_{1}}+{Z}_{2}^{{a}_{2}}+{Z}_{3}^{{a}_{3}}=0\right\}\subset {{\mathbb{C}}}^{4},

(28)

endowed with the diagonal {{\mathbb{C}}}^{* }-action with weights proportional to {a}_{i}^{-1}. If the powers ai are coprime and taken in increasing order, then Y is an exceptional Gorenstein affine variety iff 1 \, < \, \mathop{\sum }\nolimits_{i = 0}^{3}{a}_{i}^{-1} \; < \; 1+{a}_{3}^{-1}. This condition is, for example, satisfied for the powers (2, 3, 7, 11) and is, in fact, equivalent to the condition that {{{{{{\mathcal{Z}}}}}}}_{N} \, < \, \infty for any N. It also implies that the base of Y admits a Sasaki–Einstein metric. However, in Conjecture A we only demand that {{{{{{\mathcal{Z}}}}}}}_{N} \, < \, \infty for N sufficiently large.

Discussion


Let us conclude by briefly mentioning some relations to previous work. First of all, our work is very much in the spirit of the program for emergent geometry in AdS/CFT initiated by Berenstein24,25. The main new feature in our work is the appearance of a negative and fractional power of the Slater determinant in the definition of the state ΨN (see Eq. (12)) and its β-deformation. This is crucial in order to obtain background independence and to see the emergence of the spacetime metric, as explained in Section II C.

As explained at the end of section “Methods”, our approach builds on the probabilistic approach to Kähler–Einstein metrics on Fano manifolds introduced in refs. 18,26,27, which, in turn, is motivated by the Yau–Tian–Donaldson (YTD) conjecture for Fano manifolds. A different connection between the YTD conjecture and AdS/CFT was first exhibited in ref. 17 (compare the discussion on stability in section “Mathematical prerequisites: complex geometric setup”).

Finally, we note that our canonical ensemble on M may be viewed as an ensemble of N dual giant gravitons28, as will be elaborated on in a separate publication.

Methods

Proof of Theorem B

We will show how to deduce the theorem from the results in refs. 27,29 concerning a probabilistic approach to Kähler–Einstein metrics on Fano manifolds. We thus start with some well-known geometric preparations to realize M0 as a fibration over a Fano manifold (orbifold); see ref. 30, Section 2.3. First assume that ξ is a regular Reeb vector field. This means that the orbits of the complexification of ξ coincide with the orbits of a {{\mathbb{C}}}^{* }-action on Y without fixed points on Y*: = Y − {y0}. The corresponding compact complex manifold X:={Y}^{* }/{{\mathbb{C}}}^{* } is a Fano manifold, i.e., the dual {K}_{X}^{* } of its canonical line bundle KX is ample. The natural projection from Y to X realizes Y* as the total space of the qth tensor power {K}_{X}^{\otimes q}\to X for some rational positive number q, when the zero-section has been removed (and Y gets identified with the variety obtained by blowing down the zero-section). For example, in the cases when Y is {{\mathbb{C}}}^{3} and the conifold one gets X={{\mathbb{P}}}^{2} and X={{\mathbb{P}}}^{1}\times {{\mathbb{P}}}^{1} with q = 1/3 and q = 1/2, respectively. In other words, denoting by L the ample line bundle {({K}_{X}^{* })}^{\otimes q}, we may identify Y with the total space of the fibration L* → X, with the zero-section deleted. The fixed radial function r0 on Y corresponds to a Hermitian metric ∥⋅∥ on L* and the induced quotient fibration M0 → X realizes M0 is a principal U(1)-bundle over X, namely the unit-circle bundle of (L*, ∥⋅∥): 
{M}_{0} \kern1pc \hookrightarrow \kern1pc {L}^{* }(={Y}^{* })\\ \kern0.8pc \searrow \kern2pc \downarrow \\ \kern4pcX

(29)

where
{M}_{0}=\left\{{r}_{0}=1\right\}=\left\{\parallel \cdot \parallel =1\right\}.

(30)

As a consequence, there is a one-to-one correspondence between the space {{{{{\mathcal{P}}}}}}{({M}_{0})}^{\xi } of ξ-invariant probability measures μ on M0 and the space {{{{{\mathcal{P}}}}}}(X) of probability measure ν on X: 
\mu =\nu \otimes {{{\mathrm{d}}}}\theta ,

(31)

expressing μ as the fiber product of ν with the ξ-invariant probability measures dθ defined on the fibers of the fibration M0 → X. In other words, ν is proportional to the contraction of μ with ξ, descended to X. Introducing local holomorphic coordinates z on X and locally trivializing L* with the holomorphic section (dz)⊗q of {K}_{X}^{\otimes q} we may locally express
{{\Omega }}={{{\mathrm{d}}}}z\wedge {{{\mathrm{d}}}}({w}^{1/q}),\ \ \ {r}_{0}^{2}={\left(| w{| }^{2}{e}^{{\phi }_{0}(z)}\right)}^{1/3q},

(32)

where w is a local holomorphic coordinate along the fibers of L* and {e}^{{\phi }_{0}(z)} denotes the squared norm of (dz)⊗q, i.e., {e}^{{\phi }_{0}(z)}=\parallel {({{{\mathrm{d}}}}z)}^{\otimes q}{\parallel }^{2}. The local formula for Ω follows from the observation that dz ∧ d(w1/q) glues to define an equivariant global holomorphic three-form on Y*. The appearance of the power 1/3q in the formula for {r}_{0}^{2} then follows from the relation \xi =3q{\xi }_{{L}^{* }}, where {\xi }_{{L}^{* }}is the standard U(1)-action along the fibers of L* (satisfying {\xi }_{{L}^{* }}w=iw), resulting from the normalization condition ξΩ = 3iΩ. Since the weight space {H}_{{\lambda }_{k}}(Y) may be identified with the space H0 (X, L⊗k) of holomorphic sections of the kth tensor power of the holomorphic line bundle L → X it also follows that λk = 3qk. Concretely, the identification in question is obtained by noting that an element Ψ in {H}_{{\lambda }_{k}}(Y) may be locally expressed as Ψ(z, w) = fk(z)wk for a local holomorphic function fk(z), globally transforming as a holomorphic section of L⊗k → X. In particular,
{{{\Psi }}}_{\det }={f}_{\det }({z}_{1},...,{z}_{N}){w}_{1}^{k}\cdots {w}_{N}^{k}

(33)

where the local holomorphic function {f}_{\det }({z}_{1},...,{z}_{N}) on XN transforms as a holomorphic section of {({L}^{\otimes k})}^{ \boxplus N}\to {X}^{N}, namely as the Slater determinant of H0(X, L⊗k). Moreover, by Eq. (32) we have
\begin{array}{lll}{\left|{{{\Psi }}}_{\det }\right|}_{| {M}_{0}^{N}}^{2}&=&| {f}_{\det }({z}_{1},...,{z}_{N}){| }^{2}{e}^{-k{\phi }_{0}({z}_{1})}\cdots {e}^{-k{\phi }_{0}({z}_{N})}\\ &=:& \kern-9.2pc \parallel {f}_{\det }{\parallel }^{2},\end{array}

(34)

using, in the last equality, the induced Hermitian metric ∥⋅∥ on {({L}^{\otimes k})}^{ \boxplus {N}_{k}}\to {X}^{N}. With these preparations in place, we can thus express
{{{\mathrm{d}}}}{{\mathbb{P}}}_{N,\beta }^{(1)}={\nu }_{N,\beta }\otimes {{{\mathrm{d}}}}{\theta }^{\otimes N},

(35)

where νN,β is the probability measure on XN defined by
{\nu }_{N,\beta }=\frac{\parallel {f}_{\det }{\parallel }^{\frac{2}{k}\,\frac{\beta }{q}}{{{{\mathrm{d}}}}{V}_{X}}^{\otimes N}}{{\int}_{{X}^{N}}\parallel {f}_{\det }{\parallel }^{\frac{2}{k}\,\frac{\beta }{q}}{{{{\mathrm{d}}}}{V}_{X}}^{\otimes N}},

(36)

where the volume form dVX on X corresponds to the volume form dV0 on M0 under the correspondence (31). The probability measure νN,β on XN is precisely the probability measure defined by the “temperature deformed” determinantal point process on X introduced in ref. 27, associated with the Hermitian holomorphic line bundle (L, ∥⋅∥) over the compact complex manifold X endowed with a volume form dVX at the inverse temperature β/q. By ref. 27, Theorem 5.7 (and ref. 27, Lemma 5.1) its one-point correlations measures {\nu }_{N,\beta }^{(1)} converge as N → ∞, in the weak topology of measures on X, toward a volume form νβ on X of the form {\nu }_{\beta }={e}^{\frac{\beta }{q}{\varphi }_{\beta }}d{V}_{X} for the unique smooth function φβ on X satisfying the following PDE on X: 
\frac{1}{V}{({\omega }_{L}+d{d}^{c}{\varphi }_{\beta })}^{2}={e}^{\frac{\beta }{q}{\varphi }_{\beta }}{{{\mathrm{d}}}}{V}_{X},

(37)

where ωL is the Kähler form defined by the curvature of the metric ∥⋅∥ on L, locally expressed as ωL = ddcϕ0(z). Using that {\omega }_{L}=d{d}^{c}{{{{\mathrm{log}}}}}\,{({r}_{0})}^{2}/3q a direct calculation now reveals that the radial function rβ on Y defined by
{r}_{\beta }:={\left(\frac{{\mu }_{\beta }}{{{{\mathrm{d}}}}{V}_{0}}\right)}^{1/6\beta }{r}_{0},

(38)

satisfies the PDE (26). This proves the convergence in item 1 of Theorem B with μβ the volume form in {{{{{\mathcal{P}}}}}}{(M)}^{\xi } corresponding to νβ in {{{{{\mathcal{P}}}}}}(X). Similarly, applying27, Corollary 5.8 then proves the convergence of rN,β and gN,β toward rβ and gβ, respectively. Moreover, if (M, ξ) admits a Sasaki–Einstein metric, then it corresponds to a Kähler–Einstein metric ωX on X. Thus, as shown in Step 2 of the proof of ref. 29, Theorem 7.9, the PDE (37) on X admits a unique solution φβ for any β > −1 and φβ defines a real-analytic family converging to the Kähler potential φ−1 of a Kähler–Einstein metric on X, as β → −1. When rephrased in terms of rβ and gM,β this concludes the proof of Theorem B in the regular case. Finally, in the case when ξ is quasi-regular one can proceed essentially as in the regular case, using that in this case, the quotient X is a Fano orbifold, so that the role of KX is now played by the orbifold canonical line bundle of X. 

This concludes the proof of Theorem B.
Specialization to the toric case

In this section, we specialize our proposal to the case of a toric quiver gauge theory. As is well-known in this case the corresponding complex cone Y is a toric affine Gorenstein variety. As shown in refs. 31,32 (Y, ξ) admits a conical Calabi–Yau metric gY iff ξ is the unique minimizer of the volume functional V(ξ) on the space of normalized Reeb vectors, introduced in ref. 33. Equivalently, from the gauge theory point of view, this means that the U(1)R-symmetry induced by ξ maximizes the a-central charge. We explain how gY emerges from our proposal using a tropicalization procedure, which renders the proposal provably convergent and computationally feasible. It also applies to irregular Reeb vector fields.

Let Y be a 3-dimensional normal affine toric variety. This means that Y is a normal affine variety endowed with the holomorphic action of the 3-dimensional complex torus 3 with an open dense orbit, where {T}_{{\mathbb{C}}}:={({{\mathbb{C}}}^{* })}^{3} denotes the complexification of the compact torus T: = U(1)3. Accordingly, we can identify {T}_{{\mathbb{C}}} with an open subset of Y and view Y as an {T}_{{\mathbb{C}}}-equivariant compactification of {T}_{{\mathbb{C}}}. Denote by y0 the unique point in Y which is fixed under {T}_{{\mathbb{C}}} and by z = (z1, z2, z3) the holomorphic coordinates on {T}_{{\mathbb{C}}}. Since it requires no extra effort we will allow y0 to be a non-isolated singularity, following32.

The ring {{{{{\mathcal{R}}}}}}(Y), consisting of all holomorphic polynomials on Y, splits with respect to the {T}_{{\mathbb{C}}}-action on Y:
{{{{{\mathcal{R}}}}}}(Y)=\mathop{\bigoplus}\limits_{{{{{{\boldsymbol{p}}}}}}\in {{{{{{\mathcal{C}}}}}}}^{* }\cap {{\mathbb{Z}}}^{3}}{\mathbb{C}}{{{{{{\boldsymbol{z}}}}}}}^{{{{{{\boldsymbol{p}}}}}}},\ \ \ \ {{{{{{\boldsymbol{z}}}}}}}^{{{{{{\boldsymbol{p}}}}}}}:={z}_{1}^{{p}_{1}}{z}_{2}^{{p}_{1}}{z}_{3}^{{p}_{3}},

(39)

where {{{{{{\mathcal{C}}}}}}}^{* } is the “moment polytope” of the affine toric variety Y. {{{{{{\mathcal{C}}}}}}}^{* } can be represented as the convex cone in {({{\mathbb{R}}}^{3})}^{* } whose dual is a convex cone {{{{{\mathcal{C}}}}}}\subset {{\mathbb{R}}}^{3}. To simplify the notation we will identify the dual {({{\mathbb{R}}}^{3})}^{* } with {{\mathbb{R}}}^{3} in the usual way. The Reeb vector fields ξ on Y may be identified with vectors ξ in {{\mathbb{R}}}^{3} lying in the interior of the cone {{{{{\mathcal{C}}}}}}. Denote by λk the corresponding weights \left\langle {{{{{\boldsymbol{\xi }}}}}},{{{{{\boldsymbol{p}}}}}}\right\rangle as p ranges over {{{{{{\mathcal{C}}}}}}}^{* }\cap {{\mathbb{Z}}}^{3}, ordered so that λ1 < λ2... < . We can thus represent the corresponding weight spaces of {{{{{\mathcal{R}}}}}}(Y) as
{H}_{{\lambda }_{k}}(Y)=\mathop{\bigoplus }\limits_{i=1}^{{N}_{k}}{\mathbb{C}}{{{{{{\boldsymbol{z}}}}}}}^{{{{{{\boldsymbol{p}}}}}}},

(40)

where we have enumerated the lattice points {{{{{{\boldsymbol{p}}}}}}}_{1},...,{{{{{{\boldsymbol{p}}}}}}}_{{N}_{k}} in the 2-dimensional convex polytope Pk defined as the intersection of the convex cone {{{{{{\mathcal{C}}}}}}}^{* } with the hyperplane \{\left\langle {{{{{\boldsymbol{\xi }}}}}},\cdot \right\rangle ={\lambda }_{k}\}\!:
{P}_{k}={\lambda }_{k}{P}_{\xi }\cap {{\mathbb{Z}}}^{3},\ \ \ {P}_{\xi }:=\{{{{{{{\mathcal{C}}}}}}}^{* }\cap \left\langle {{{{{\boldsymbol{\xi }}}}}},\cdot \right\rangle =1\},

(41)

(note that the polytope Pξ is denoted by Δ in ref. 9 and called the characteristic polytope). Now assume that Y is Gorenstein and denote by Ω the {T}_{{\mathbb{C}}}-equivariant holomorphic top-form on Y − {y0}. On {T}_{{\mathbb{C}}}\subset Y, we can express
{{\Omega }}={{{{{{\boldsymbol{z}}}}}}}^{{{{{{\boldsymbol{l}}}}}}}{{{\Omega }}}_{0},\ \ \ {{{\Omega }}}_{0}:=\frac{{{{\mathrm{d}}}}{z}_{1}}{{z}_{1}}\wedge \frac{{{{\mathrm{d}}}}{z}_{2}}{{z}_{2}}\wedge \frac{{{{\mathrm{d}}}}{z}_{3}}{{z}_{3}}

(42)

for some {{{{{\boldsymbol{l}}}}}}\in {{\mathbb{Z}}}^{3}, where Ω0 is the standard {T}_{{\mathbb{C}}}-invariant volume form on {T}_{{\mathbb{C}}}. The condition that Ω is homogeneous of degree 3 under the Reeb field ξ translates into the condition \left\langle {{{{{\boldsymbol{l}}}}}},{{{{{\boldsymbol{\xi }}}}}}\right\rangle =3. For example, when Y={{\mathbb{C}}}^{3} with the standard Reeb vector ξ = (1, 1, 1), the cone {{{{{{\mathcal{C}}}}}}}^{* } is the positive octant in {{\mathbb{R}}}^{3} and Pξ bounds the unit-simplex. We will also briefly discuss the case of the conifold below.

We now specialize our proposal to the toric case. First, note that using the bases {{{{{{\boldsymbol{z}}}}}}}^{{{{{{{\boldsymbol{p}}}}}}}_{1}},...,{{{{{{\boldsymbol{z}}}}}}}^{{{{{{{\boldsymbol{p}}}}}}}_{{N}_{k}}} in {H}_{{\lambda }_{k}}(Y) the corresponding Slater determinant {{{\Psi }}}_{\det } may be represented as the following holomorphic function on {T}_{{\mathbb{C}}}^{{N}_{k}}\subset {Y}^{{N}_{k}}\!\!:
{{{\Psi }}}_{\det }({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}})=\mathop{\sum}\limits_{\sigma \in {S}_{{N}_{k}}}{(-1)}^{| \sigma | }{{{{{{\boldsymbol{z}}}}}}}^{{{{{{{\boldsymbol{p}}}}}}}_{\sigma (1)}}\cdots {{{{{{\boldsymbol{z}}}}}}}^{{{{{{{\boldsymbol{p}}}}}}}_{\sigma ({N}_{k})}}

(43)

Accordingly, on the open dense subset {T}_{{\mathbb{C}}}^{N} of YN we can, using formula (42), express
| {{{\Psi }}}_{{N}_{k}}{| }^{2}{({{\Omega }}\wedge \overline{{{\Omega }}})}^{\otimes {N}_{k}}={\rho }_{{N}_{k}}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}){({{{\Omega }}}_{0}\wedge {\overline{{{\Omega }}}}_{0})}^{\otimes {N}_{k}},

(44)

where
{\rho }_{{N}_{k}}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}):={\left|\mathop{\sum}\limits_{\sigma \in {S}_{{N}_{k}}}{(-1)}^{| \sigma | }{{{{{{\boldsymbol{z}}}}}}}^{{{{{{{\boldsymbol{q}}}}}}}_{\sigma (1)}}\cdots {{{{{{\boldsymbol{z}}}}}}}^{{{{{{{\boldsymbol{q}}}}}}}_{\sigma ({N}_{k})}}\right|}^{-2\frac{3}{{\lambda }_{k}}}.

(45)

Here we have defined qi: = pi/λk − l/3, i = 1, …, Nk, corresponding to the discrete points of the scaled and shifted polytope Qk defined as
\begin{array}{lll}{Q}_{k}&\kern-0.5pc:=&\kern-0.5pc{P}_{k}/{\lambda }_{k}-{{{{{\boldsymbol{l}}}}}}/3\subset {{\mathbb{R}}}^{3}\cap {({\mathbb{Z}}/{\lambda }_{k})}^{3}\\ {Q}_{\xi }&\kern-0.5pc:=&\kern-7pc{P}_{\xi }-\ell /3,\end{array}

(46)

where Qξ is the limit of Qk when k → ∞.

From a computational point of view, this explicit expression for {\rho }_{{N}_{k}}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}) is still rather challenging to work with directly. But the construction of a Sasaki–Einstein metric can be simplified by further leveraging the toric structure.

To see this, first recall that, in general, the group {{{{{\mathcal{G}}}}}}(Y,\xi ) of all biholomorphisms of a complex cone Y, commuting with the Reeb vector field ξ and homotopic to the identity, acts transitively on the space of conical Calabi–Yau metrics gY20. In particular, the toric case {{{{{\mathcal{G}}}}}}(Y,\xi ) contains the group {T}_{{\mathbb{C}}} and thus gY is not uniquely determined, but can be taken to be T-invariant. The density {\rho }_{{N}_{k}}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}), on the other hand, is not {T}^{{N}_{k}}-invariant. This is to be expected as the large N-limit should encapsulate all conical Calabi–Yau metrics on Y—not only the T-invariant ones. In order to directly extract a T-invariant conical Calabi–Yau metric gY from the large N-limit we can modify the density {\rho }_{{N}_{k}} on {Y}^{{N}_{k}} to render it {T}^{{N}_{k}}-invariant. This can be achieved in various ways, but from a computational point of view, the most efficient modification appears to replace the density {\rho }_{{N}_{k}}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}) with its tropicalization:
{\rho }_{{{{\mathrm{trop}}}}}^{({N}_{k})}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}):={\left(\mathop{\max }\limits_{\sigma \in {S}_{{N}_{k}}}{\left|{{{{{{\boldsymbol{z}}}}}}}_{1}^{{{{{{{\boldsymbol{q}}}}}}}_{\sigma (1)}}\cdots {{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}^{{{{{{{\boldsymbol{q}}}}}}}_{\sigma ({N}_{k})}}\right|}^{2}\right)}^{-3},

(47)

where, in particular, the sum over {S}_{{N}_{k}} has been replaced with a maximum. In terms of the logarithmic real coordinates
{{{{{\boldsymbol{x}}}}}}=({x}_{1},{x}_{2},{x}_{3}):=\left({{{{\mathrm{log}}}}}\,(| {z}_{1}{| }^{2}),{{{{\mathrm{log}}}}}\,(| {z}_{2}{| }^{2}),{{{{\mathrm{log}}}}}\,(| {z}_{3}{| }^{2})\right)\in {{\mathbb{R}}}^{3}

(48)

this means that
{\rho }_{{{{\mathrm{trop}}}}}^{({N}_{k})}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}):={e}^{-N{E}_{{{{\mathrm{trop}}}}}^{({N}_{k})}({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}})},

(49)

where {E}_{{{{\mathrm{trop}}}}}^{({N}_{k})}({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}}) denotes the following symmetric piece-wise affine convex function on {({{\mathbb{R}}}^{3})}^{{N}_{k}}\!\!:
{E}_{{{{\mathrm{trop}}}}}^{({N}_{k})}({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}})=\; \frac{3}{{N}_{k}}\mathop{\max }\limits_{\sigma \in {S}_{{N}_{k}}}\left(\left\langle {{{{{{\boldsymbol{x}}}}}}}_{1},{{{{{{\boldsymbol{q}}}}}}}_{\sigma (1)}\right\rangle+\cdots \ \right.\\ \left.\cdots +\left\langle {{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}},{{{{{{\boldsymbol{q}}}}}}}_{\sigma ({N}_{k})}\right\rangle \right).

(50)

Hence, the corresponding {T}^{{N}_{k}}-invariant “tropicalized” measure on {Y}^{{N}_{k}} may be expressed as follows
\begin{array}{lll}{\rho }_{{{{\mathrm{trop}}}}}^{({N}_{k})}({{{{{{\boldsymbol{z}}}}}}}_{1},...,{{{{{{\boldsymbol{z}}}}}}}_{{N}_{k}}){({{\Omega }}\wedge \overline{{{\Omega }}})}^{\otimes {N}_{k}} ={e}^{-{N}_{k}{E}_{{{{\mathrm{trop}}}}}^{({N}_{k})}({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}})}{({{{\mathrm{d}}}}{{{{{\boldsymbol{x}}}}}})}^{\otimes {N}_{k}}\otimes {({{{\mathrm{d}}}}{{{{{\boldsymbol{\theta }}}}}})}^{\otimes {N}_{k}},\end{array}

(51)

with dθ denoting the T-invariant probability measure on T. Contracting {{\Omega }}\wedge \overline{{{\Omega }}} with the dilation vector field δ: = −Jξ, as before, thus yields a {T}^{{N}_{k}}-invariant measure on {M}^{{N}_{k}}. By performing a linear change of coordinates on {{\mathbb{R}}}^{3}, we may assume that dilatation on Y corresponds to translations in the x3-variable in {{\mathbb{R}}}^{3}. The contraction in question thus corresponds to replacing {{\mathbb{R}}}^{3} in Eq. (51) by {{\mathbb{R}}}^{2}. However, the integral over {M}^{{N}_{k}} given by the corresponding normalizing constant always diverges due to the diagonal action of the residual symmetry group {T}_{{\mathbb{C}}}/T. This action has the effect of translating the center of mass in {{\mathbb{R}}}^{2} of a configuration ({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}})\in {({{\mathbb{R}}}^{2})}^{{N}_{k}}. The remedy is to break the symmetry in question. This can be achieved by introducing a background radial function (as in Theorem B). But from a computational point of view the most efficient way is to simply impose the constraint that the center of mass in {{\mathbb{R}}}^{2} of ({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}}) vanishes, i.e., that {{{{{{\boldsymbol{x}}}}}}}_{1}+...+{{{{{{\boldsymbol{x}}}}}}}_{{N}_{k}} vanishes. Finally, since the number Nk may scale as o(k2), unless ξ is quasi-regular, we replace Nk with any positive integer N and take q1, ..., qN to be any sequence of points in the polytope Qξ with the property that
\mathop{\lim }\limits_{N\to \infty }\frac{1}{N}\mathop{\sum }\limits_{i=1}^{N}{\delta }_{{{{{{{\boldsymbol{q}}}}}}}_{i}}={\nu }_{{Q}_{\xi }}

(52)

where {\nu }_{{Q}_{\xi }} is the Euclidean measure on Qξ normalized to have unit total mass. In summary, the tropicalized probability measure thus corresponds to the following Boltzmann–Gibbs measure on {({{\mathbb{R}}}^{2})}^{N}:
{\mu }_{{{{\mathrm{trop}}}}}^{(N)}:=\frac{1}{{Z}_{{{{\mathrm{trop}}}}}^{(N)}}{e}^{-N{E}_{{{{\mathrm{trop}}}}}^{(N)}({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{N})}{({{{\mathrm{d}}}}{{{{{\boldsymbol{x}}}}}})}^{\otimes N},

(53)

with
{Z}_{trop}^{(N)}:=\int {e}^{-N{E}_{trop}^{(N)}({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{N})}d{{{{{{\boldsymbol{x}}}}}}}^{\otimes N}

(54)

together with the constraint of vanishing center of mass.

We then have the following result.

Theorem C: {Z}_{{{{\mathrm{trop}}}}}^{(N)} \, < \, \infty for N sufficiently large iff (M, ξ) admits a conical Sasaki–Einstein metric (i.e., iff ξ minimizes the volume functional V(ξ) on the Reeb cone). Moreover, if this is the case then the law of the empirical measure \frac{1}{N}\mathop{\sum }\nolimits_{i = 1}^{N}{\delta }_{{{{{{{\boldsymbol{x}}}}}}}_{i}} on the ensemble \left({({{\mathbb{R}}}^{2})}^{N},{\mu }_{{{{\mathrm{trop}}}}}^{(N)}\right) converges in law, as N → ∞, toward a volume form μSE on {{\mathbb{R}}}^{2}; the normalized volume form of the unique T-invariant Sasaki–Einstein metric on (M, ξ) with vanishing center of mass (when expressed in real logarithmic coordinates on {{\mathbb{R}}}^{2}).

The probability measure μSE on {{\mathbb{R}}}^{2} may be expressed as
{\mu }_{SE}={e}^{-3\phi }{{{\mathrm{d}}}}{{{{{\boldsymbol{x}}}}}},

(55)

where the function ϕ on {{\mathbb{R}}}^{2} corresponds to the Kähler potential r2 of the corresponding T-invariant conical Calabi–Yau metric on Y, i.e., {r}^{2}={e}^{\phi (x)+\left\langle l,x\right\rangle /3}. Theorem C thus provides evidence for Conjecture A. The advantage of the tropicalized setup is that the corresponding energy {E}_{{{{\mathrm{trop}}}}}^{(N)}({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{N}) is continuous. The theorem can be shown using results in ref. 34, where a closely related tropical approach to Kähler–Einstein metrics on toric Fano varieties was introduced. Details will appear elsewhere.

For example, in the homogeneous cases of {{\mathbb{C}}}^{3} and the conifold it is well-known that the polytope Qξ is a translation of the two-dimensional simplex or the unit-square, respectively. In these cases, the function ϕ(x) is given explicitly, modulo an additive constant, by \phi (x)={{{{\mathrm{log}}}}}\,(1+{e}^{{x}_{1}}+{e}^{{x}_{2}})-{x}_{1}/3-{x}_{2}/3 for {{\mathbb{C}}}^{3} and \phi (x)={{{{\mathrm{log}}}}}\,({e}^{-{x}_{1}/2}+{e}^{{x}_{1}/2})+{{{{\mathrm{log}}}}}\,({e}^{-{x}_{2}/2}+{e}^{+{x}_{2}/2}) for the conifold.

Similarly, in the case when Y is {{\mathbb{C}}}^{2} the polytope Qξ is equal to [−1/2, 1/2] and the corresponding one-point correlations can be computed explicitly for any finite N. The result is a polynomial of degree N in e−∣x∣, converging, as N → ∞, toward e−2ϕ(x), where \phi (x)={{{{\mathrm{log}}}}}\,({e}^{-x/2}+{e}^{x/2})-C. Indeed, in this case, the corresponding tropical energy {E}_{{{{\mathrm{trop}}}}}^{(N)} turns out to coincide with the energy of a self-gravitating system in 1D (with a mean-field scaling), to which the exact results in ref. 35 apply.

In general, however, the solution ϕ can not be explicitly computed. An important feature of Theorem C is that it provides an efficient way of obtaining numerical approximations to the solution ϕ and thus to the Sasaki–Einstein metric on M, using Hamiltonian Monte-Carlo. The starting point is the observation that the gradient of the energy N{E}_{{{{\mathrm{trop}}}}}^{(N)} appearing in the Boltzmann–Gibbs measure (51) is, for a generic configuration ({{{{{{\boldsymbol{x}}}}}}}_{1},...,{{{{{{\boldsymbol{x}}}}}}}_{N})\in {{\mathbb{R}}}^{2N}, precisely the discrete optimal transport map matching the points (x1, ..., xN) with the fixed points q1, ...., qN in Qξ36. Thanks to the last years rapid developments of scalable optimal transport solvers this allows one to numerically compute the gradient in nearly {{{{{\mathcal{O}}}}}}(N) operations (efficiently implemented on GPU-hardware37,38). Moreover, since {E}_{{{{\mathrm{trop}}}}}^{(N)} is convex Hamiltonian Monte-Carlo should merely require {{{{{\mathcal{O}}}}}}({N}^{1/4}) gradient evaluations39, suggesting that the total running time of the simulation nearly scales as {{{{{\mathcal{O}}}}}}({N}^{1+1/4}).

Monte-Carlo techniques have previously been applied in ref. 40 to the vacuum moduli space YN/SN in the case Y={{\mathbb{C}}}^{3}, but using a different N-particle BPS-wave function (with a Metropolis algorithm).

We leave the implementation of our simulation scheme for the future.

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Data sharing is not applicable to this article since no data sets were generated or analyzed during the current study.


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Acknowledgements


We are grateful to David Berenstein, Amihay Hanany, and James Sparks for helpful discussions and correspondence. The work of R.J.B. was supported by the Swedish Research Council (grant no. 11253043), the Wallenberg Foundation (grant no. 11253045), and the Göran Gustafsson prize (grant no. 11253042). T.C.C. was supported by NSF CAREER grant (no. DMS-1944952), and an Alfred P. Sloan Fellowship. D.P. was supported by the Swedish Research Council (grant. no 2018-04760), and the Wallenberg AI, Autonomous Systems and Software Program (WASP) funded by the Wallenberg Foundation (grant no. 2020.0173).

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Robert J. Berman & Daniel Persson


Department of Mathematics, Massachusetts Institute of Technology, Cambridge, MA, 02139, USA

Tristan C. Collins
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R.J.B., T.C.C. and D.P. have all contributed equally to this work. Authors are listed alphabetically according to surnames.
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Berman, R.J., Collins, T.C. & Persson, D. Emergent Sasaki-Einstein geometry and AdS/CFT. Nat Commun 13, 365 (2022). https://doi.org/10.1038/s41467-021-27951-9


Received16 October 2020


Accepted27 December 2021


Published18 January 2022


DOIhttps://doi.org/10.1038/s41467-021-27951-9

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