Quantum gravity in timeless configuration space
On the path towards quantum gravity we find friction between temporal relations in quantum mechanics
(QM) (where they are fixed and field-independent), and in general relativity (where they are field-dependent
and dynamic). This paper aims to attenuate that friction, by encoding gravity in the timeless configuration
space of spatial fields with dynamics given by a path integral. The framework demands that boundary conditions
for this path integral be uniquely given, but unlike other approaches where they are prescribed — such
as the no-boundary and the tunneling proposals — here I postulate basic principles to identify boundary conditions
in a large class of theories. Uniqueness arises only if a reduced configuration space can be defined
and if it has a profoundly asymmetric fundamental structure. These requirements place strong restrictions
on the field and symmetry content of theories encompassed here; shape dynamics is one such theory. When
these constraints are met, any emerging theory will have a Born rule given merely by a particular volume
element built from the path integral in (reduced) configuration space. Also as in other boundary proposals,
Time, including space-time, emerges as an effective concept; valid for certain curves in configuration space
but not assumed from the start. When some such notion of time becomes available, conservation of (positive)
probability currents ensues. I show that, in the appropriate limits, a Schroedinger equation dictates the
evolution of weakly coupled source fields on a classical gravitational background. Due to the asymmetry
of reduced configuration space, these probabilities and currents avoid a known difficulty of standard WKB
approximations for Wheeler DeWitt in minisuperspace: the selection of a unique Hamilton-Jacobi solution to
serve as background. I illustrate these constructions with a simple example of a full quantum gravitational
theory (i.e. not in minisuperspace) for which the formalism is applicable, and give a formula for calculating
gravitational semi-classical relative probabilities in it.

Suppressed SUSY for the SU(5) Grand Unified Supergravity Theory
This paper starts with the most basic SU(5) Grand Unified Theory, coupled to Supergravity. Then it
builds a new theory, incorporating the ideas of Suppressed SUSY. Suppressed SUSY is an alternative to
the spontaneous breaking of SUSY. It does not need an invisible sector or explicit soft breaking of SUSY.
It varies the content of the supermultiplets while keeping the restrictive nature of SUSY. For the simple
model and sector constructed here, Suppressed SUSY has only three dimensionless parameters, plus the
Planck mass. At tree level, this predicts a set of 8 different new masses, along with a cosmological constant
that is naturally zero. The X and Y vector bosons get Planck scale masses 2√
10g5MP. The five scalar multiplets that accompany the Higgs, and the Gravitino, all get colossally huge ‘SuperPlanck’ scale masses
of order MSP ≈ 1017MP from a see-saw mechanism that arises from the theory. This new mass spectrum,
the well-known SU(5) weak angle problem, and the cosmological constant value, should serve as guides for
further modifications for the new Action.

Beyond the Cosmological Standard Model
After a decade and a half of research motivated by the accelerating universe, theory and experiment
have a reached a certain level of maturity. The development of theoretical models beyond
Λ or smooth dark energy, often called modified gravity, has led to broader insights into a path
forward, and a host of observational and experimental tests have been developed. In this review
we present the current state of the field and describe a framework for anticipating developments
in the next decade. We identify the guiding principles for rigorous and consistent modifications
of the standard model, and discuss the prospects for empirical tests.
We begin by reviewing recent attempts to consistently modify Einstein gravity in the infrared,
focusing on the notion that additional degrees of freedom introduced by the modification
must “screen” themselves from local tests of gravity. We categorize screening mechanisms into
three broad classes: mechanisms which become active in regions of high Newtonian potential,
those in which first derivatives of the field become important, and those for which second derivatives
of the field are important. Examples of the first class, such as f(R) gravity, employ the
familiar chameleon or symmetron mechanisms, whereas examples of the last class are galileon
and massive gravity theories, employing the Vainshtein mechanism. In each case, we describe
the theories as effective theories and discuss prospects for completion in a more fundamental
theory. We describe experimental tests of each class of theories, summarizing laboratory and
solar system tests and describing in some detail astrophysical and cosmological tests. Finally,
we discuss prospects for future tests which will be sensitive to different signatures of new physics
in the gravitational sector.
The review is structured so that those parts that are more relevant to theorists vs. observers/experimentalists
are clearly indicated, in the hope that this will serve as a useful reference
for both audiences, as well as helping those interested in bridging the gap between them.

Computational complexity of the string-landscape/multiverse II – Cosmological considerations
We propose a new approach for multiverse analysis based on computational
complexity, which leads to a new family of “computational” measure factors. By
defining a cosmology as a space-time containing a vacuum with specified properties (for
example small cosmological constant) together with rules for how time evolution will
produce the vacuum, we can associate global time in a multiverse with clock time on a
supercomputer which simulates it. We argue for a principle of “limited computational
complexity” governing early universe dynamics as simulated by this supercomputer,
which translates to a global measure for regulating the infinities of eternal inflation.
The rules for time evolution can be thought of as a search algorithm, whose details
should be constrained by a stronger principle of “minimal computational complexity.”
Unlike previously studied global measures, ours avoids standard equilibrium considerations
and the well-known problems of Boltzmann Brains and the youngness paradox.
We also give various definitions of the computational complexity of a cosmology, and
argue that there are only a few natural complexity classes.

Taking up superspace—what would it take to be a realist about superspace?
Supersymmetry is a crucial part of the string theoretic framework for a theory of
quantum gravity. Supersymmetric theories (including those outside the context of
string theory) present an interesting interpretative challenge. As a result of consistency
conditions on the algebra of the supersymmetry (SUSY) generators, one is led to the
idea that SUSY, although traditionally defined as a dynamical symmetry between
bosons and fermions, could also be thought of as a spacetime symmetry in some
extended spacetime, known as superspace. This paper focuses on what it would take
to argue for an interpretation that favours the superspace formulation. I introduce
a toy model of a supersymmetric field theory and argue for a special case of a more
general thesis—that one needs some pre-existing philosophical commitment to favour
one mathematical formulation over another. I then consider some extant positions
from the literature on the philosophy of spacetime as candidates for such a position in
the context of supersymmetric theories.

Liouville Action as Path-Integral Complexity: From Continuous Tensor Networks to AdS/CFT
Abstract: We propose an optimization procedure for Euclidean path-integrals that
evaluate CFT wave functionals in arbitrary dimensions. The optimization is performed
by minimizing certain functional, which can be interpreted as a measure of
computational complexity, with respect to background metrics for the path-integrals.
In two dimensional CFTs, this functional is given by the Liouville action. We also
formulate the optimization for higher dimensional CFTs and, in various examples,
find that the optimized hyperbolic metrics coincide with the time slices of expected
gravity duals. Moreover, if we optimize a reduced density matrix, the geometry becomes
two copies of the entanglement wedge and reproduces the holographic entanglement
entropy. Our approach resembles a continuous tensor network renormalization
and provides a concrete realization of the proposed interpretation of AdS/CFT
as tensor networks. The present paper is an extended version of our earlier report
arXiv:1703.00456 and includes many new results such as evaluations of complexity
functionals, energy stress tensor, higher dimensional extensions and time evolutions
of thermofield double states.

D–Branes and T–Duality
Recent developments in string theory have shown that p–brane solutions
and duality symmetries play an important role in understanding the nonperturbative
behaviour of the theory. An important example of a duality
symmetry is the T–duality [1] which states that a string compactified on a
torus with radius R is equivalent to a string compactified on a torus with
radius α
′/R where α
′
is the inverse string tension.
It turns out that the p–brane solutions whose charge are carried by a RR
(Ramond/Ramond) gauge field of the type II supergravity theories have a
natural place within open string theory as D–branes [2]. The relation is
established via the requirement that the endpoints of the open string are
constrained to live on the p+ 1–dimensional worldvolume of the Dirichlet p–
brane. Such a (ten–dimensional) open string state is described by Dirichlet
boundary conditions for the 9−p transverse directions and Neumann boundary
conditions for the p + 1 worldvolume directions. Since under T–duality
Dirichlet and Neumann boundary conditions are interchanged it follows that
all Dirichlet p–branes (p = 0, · · · , 9) are T-dual versions of each other. A
discussion of how this T–duality between D–branes arises in string theory
can be found in the recent review article [3].
Since all D–branes are T–dual to each other it is natural to expect that
this T–duality is also realized on the underlying p–brane solutions of the
IIA/IIB supergravity theories. Furthermore, the T–duality should also be
realized on the Dirichlet p–brane actions which act as source terms of the
p–brane solutions. It is the purpose of this letter to give the details of this
T–duality between Dirichlet p–brane solutions and their source terms and
to point out a few subtleties that occur in establishing T–duality.

Timelike duality, M′-theory and an exotic form of the Englert solution
Through timelike dualities, one can generate exotic versions of M-theory with different
spacetime signatures. These are the M∗
-theory with signature (9, 2, −), the M′
-theory,
with signature (6, 5, +) and the theories with reversed signatures (1, 10, −), (2, 9, +) and
(5, 6, −). In (s, t, ±), s is the number of space directions, t the number of time directions,
and ± refers to the sign of the kinetic term of the 3 form.
The only irreducible pseudo-riemannian manifolds admitting absolute parallelism are,
besides Lie groups, the seven-sphere S
7 ≡ SO(8)/SO(7) and its pseudo-riemannian version
S
3,4 ≡ SO(4, 4)/SO(3, 4). [There is also the complexification SO(8, C)/SO(7, C),
but it is of dimension too high for our considerations.] The seven-sphere S
7 ≡ S
7,0
has been found to play an important role in 11-dimensional supergravity, both through
the Freund-Rubin solution and the Englert solution that uses its remarkable parallelizability
to turn on non trivial internal fluxes. The spacetime manifold is in both cases
AdS4 ×S
7
. We show that S
3,4
enjoys a similar role in M′
-theory and construct the exotic
form AdS4 × S
3,4 of the Englert solution, with non zero internal fluxes turned on. There
is no analogous solution in M∗
-theory.

Axion wormholes in AdS compactifications
Euclidean wormholes [1–3] are extrema of the action in Euclidean quantum gravity that
connect two distant regions, or even two disconnected asymptotic regions. Despite much
work over many years it remains unclear whether wormholes can provide valid saddle point
contributions to the Euclidean path integral and therefore have physical implications (see
e.g. [4–8]).
The Weak Gravity Conjecture (WGC) [9] adds a new dimension to this question.
This is because its generalization to instantons implies the existence of super-extremal
instantons which, when sourced by axions, correspond to Euclidean axion wormholes. It
has been argued that such instanton contributions can destroy the flatness of the potential
in models of large field inflation based on axions [10], although there is no consensus on
this [11].
It is therefore important to elucidate the physical meaning - if any - of wormholes.
To this end it is clearly of interest to find wormhole solutions in string theory and in
particular in AdS compactifications, where the AdS/CFT dual partition function provides
an alternative description of the gravitational path integral. Axionic wormholes [1] provide
natural candidates for wormhole solutions in string theory. However axions are always
accompanied by dilatons in string theory compactifications, and the existence of regular
wormhole solutions depends delicately on the number of scalars and their couplings [4]. In
a single axion-dilaton system coupled to gravity, for instance, the dilaton coupling must be
sufficiently small in order for wormholes to exist.
In [12] Calabi-Yau compactifications were found which allow for regular axionic wormhole
solutions in flat space. The situation is more subtle however in compactifications to
AdS. Type IIB on AdS5 × S5 does not admit axionic wormholes [5]. On the other hand,
in [4] it was argued there are approximate wormhole solutions in Type IIB compactified on AdS3 × S3 × T4.
However no clean derivation was given to determine the exact axion - dilaton content of this compactification.1 The validity of those solutions therefore remains somewhat uncertain. Specifically, their smoothness depends on the specific Wick rotation
that was used in [4], but it remains unclear whether this particular Wick rotation is the
one selected by AdS/CFT. The goal of this paper is to construct exact, regular axionic wormhole solutions in
an AdS compactification where the Wick rotation to the Euclidean theory can be made rigorous using AdS/CFT. The wormholes we find are solutions to Euclidean IIB string theory on AdS5 × S5/Zk, whose field theory duals are certain N = 2 quiver theories [13].
The dual operators that are turned on are exactly marginal operators, which enables us
to identify the Wick rotation selected by AdS/CFT and therefore rigorously determine the
nature of the scalar fields in the theory. Our results further sharpen the paradox with
AdS/CFT and the apparent uniqueness of quantum gravity. One is left wondering what is
pathological about axionic wormholes.

String Compactification and Global Orientifolded Quivers with Inflation
Abstract: We describe global embeddings of fractional D3 branes at orientifolded singularities
in type IIB flux compactifications. We present an explicit Calabi-Yau example
where the chiral visible sector lives on a local orientifolded quiver while non-perturbative
effects, α0 corrections and a T-brane hidden sector lead to full closed string moduli stabilisation
in a de Sitter vacuum. The same model can also successfully give rise to inflation
driven by a del Pezzo divisor. Our model represents the first explicit Calabi-Yau example
featuring both an inflationary and a chiral visible sector.

A Supersymmetric D-Brane Model of Space-Time Foam
We present a supersymmetric model of space-time foam with two stacks of eight D8-branes
with equal string tensions, separated by a single bulk dimension containing D0-brane particles
that represent quantum fluctuations in the space-time foam. The ground-state configuration
with static D-branes has zero vacuum energy. However, gravitons and other closed-string states
propagating through the bulk may interact with the D0-particles, causing them to recoil and
the vacuum energy to become non-zero. This provides a possible origin of dark energy. Recoil
also distorts the background metric felt by energetic massless string states, which travel at less
than the usual (low-energy) velocity of light. On the other hand, the propagation of chiral
matter fields anchored on the D8-branes is not affected by such space-time foam effects.

“Semi-Realistic” F-term Inflation Model Building in Supergravity
We describe methods for building “semi-realistic” models of F-term inflation. By semirealistic
we mean that they are built in, and obey the requirements of, “semi-realistic”
particle physics models. The particle physics models are taken to be effective supergravity
theories derived from orbifold compactifications of string theory, and their requirements
are taken to be modular invariance, absence of mass terms and stabilization
of moduli. We review the particle physics models, their requirements and tools and
methods for building inflation models.

Open string T-duality in double space
The role of double space is essential in new interpretation of T-duality and consequently
in an attempt to construct M-theory. The case of open string is missing
in such approach because until now there have been no appropriate formulation of
open string T-duality. In the previous paper [1], we showed how to introduce vector
gauge fields ANa and ADi at the end-points of open string in order to enable open string
invariance under local gauge transformations of the Kalb-Ramond field and its T-dual "restricted general coordinate transformations”. We demonstrated that gauge fields ANa and ADi are T-dual to each other. In the present article we prove that all above
results can be interpreted as coordinate permutations in double space.

E(lementary)-Strings in Six-Dimensional Heterotic F-theory
Using E-strings, we can analyze not only six-dimensional superconformal field theories
but also probe vacua of non-perturabative heterotic string. We study strings made of
D3-branes wrapped on various two-cycles in the global F-theory setup. We claim that
E-strings are elementary in the sense that various combinations of E-strings can form Mstrings
as well as heterotic strings and new kind of strings, called G-strings. Using them,
we show that emissions and combinations of heterotic small instantons generate most of
known six-dimensional superconformal theories, their affinizations and little string theories.
Taking account of global structure of compact internal geometry, we also show that
special combinations of E-strings play an important role in constructing six-dimensional
theories of D- and E-types. We check global consistency conditions from anomaly cancellation
conditions, both from five-branes and strings, and show that they are given in
terms of elementary E-string combinations.

On the origin of generalized uncertainty principle from compactified M5-brane
In this paper, we demonstrate that compactification in M-theory can lead to a deformation of
field theory consistent with the generalized uncertainty principle (GUP). We observe that the matter
fields in the M3-brane action contain higher derivative terms. We demonstrate that such terms can
also be constructed from a reformulation of the field theory by the GUP. In fact, we will construct
the Heisenberg algebra consistent with this deformation, and explicitly demonstrate it to be the
Heisenberg algebra obtained from the GUP. Thus, we use compactification in M-theory to motivate
for the existence of the GUP.

Target Space Duality in String Theory
String theory (see for example [158]) assumes that the elementary particles are one dimensional
extended objects rather than point like ones. String theory also comes equipped with a scale
associated, nowadays, with the Planck scale (10−33 cm). The standard model describing the
color and electro-weak interactions is based on the point particle notion and is successful at the
Fermi scale of about 100 Gev (10−16 cm) which is 10−17 smaller than the Planck scale.
The correspondence principle requires thus that string theory when applied to these low
energies resembles a point particle picture. In fact string theory has an interpretation in terms
of point-like field theory whose spectrum consists of an infinity of particles, all except a finite
number of which have a mass of the order of the Planck scale. Integrating out the massive
modes leads to an effective theory of the light particles.
There exists another class of theories whose spectrum consists as well of an infinite tower
of particles; this is the Kaluza-Klein type. In such a class of theories [182, 199, 12], gravity
is essentially the sole basic interaction, and space-time is assumed to have, in addition to four
macroscopic dimensions, extra microscopic dimensions, characterized by some small distance
scale. The standard model is assumed to be a low-energy effective action of the light particles
resulting from the purely gravitational higher dimensional system.
String theory can also be viewed in many cases as representing a space-time with extra
dimensions. Nevertheless, the effective low-energy theory, emerging from string theory, turns
out to be different from that resulting from a field theory with an infinite number of particles;
it possesses many more symmetries.
String theory shows also differences when physics is probed at a scale much smaller than the
Planck one. In fact, there are various hints that in string theory physics at a very small scale
cannot be distinguished from physics at a large scale. A very striking example of that feature
is that a string cannot tell if it is propagating on a space-time with one circular dimension of
radius R (a dimensionless number) times the Planck scale or 1/R the Planck scale (see figure
1.A). The discrete symmetry apparent in the example is termed target space duality. Moreover,
there are indications that string theory possesses an extremely large symmetry of that nature.
A study of that symmetry is the subject of the review.

The Disconnect Between Quantum Mechanics and Gravity
Abstract: There is a serious disconnect between quantum theory and gravity. It occurs at the level of the very foundations of quantum theory, and is far deeper than just the matter of trying to quantize a non-linear theory. We shall examine some of the physical reasons for this disconnect
and show how it manifests itself at the beginning, at the level of the equivalence principle.

No Universe without Big Bang
According to Einstein's theory of relativity, the curvature of spacetime was infinite at the big bang. In fact, at this point all mathematical tools fail, and the theory breaks down. However, there remained the notion that perhaps the beginning of the universe could be treated in a simpler manner, and that the infinities of the big bang might be avoided. This has indeed been the hope expressed since the 1980s by the well-known cosmologists James Hartle and Stephen Hawking with their "no-boundary proposal", and by Alexander Vilenkin with his "tunnelling proposal". Now scientists at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute/AEI) in Potsdam and at the Perimeter Institute in Canada have been able to use better mathematical methods to show that these ideas cannot work. The big bang, in its complicated glory, retains all its mystery.
One of the principal goals of cosmology is to understand the beginning of our universe. Data from the Planck satellite mission shows that 13.8 billion years ago the universe consisted of a hot and dense soup of particles. Since then the universe has been expanding. This is the main tenet of the hot big bang theory, but the theory fails to describe the very first stages themselves, as the conditions were too extreme. Indeed, as we approach the big bang, the energy density and the curvature grow until we reach the point where they become infinite.
As an alternative, the "no-boundary" and "tunneling" proposals assume that the tiny early universe arose by quantum tunnelling from nothing, and subsequently grew into the large universe that we see. The curvature of spacetime would have been large, but finite in this beginning stage, and the geometry would have been smooth - without boundary (see Fig. 1, left panel). This initial configuration would replace the standard big bang. However, for a long time the true consequences of this hypothesis remained unclear. Now, with the help of better mathematical methods, Jean-Luc Lehners, group leader at the AEI, and his colleagues Job Feldbrugge and Neil Turok at Perimeter Institute, managed to define the 35 year old theories in a precise manner for the first time, and to calculate their implications. The result of these investigations is that these alternatives to the big bang are no true alternatives. As a result of Heisenberg's uncertainty relation, these models do not only imply that smooth universes can tunnel out of nothing, but also irregular universes. In fact, the more irregular and crumpled they are, the more likely (see Fig. 1, right panel). "Hence the "no-boundary proposal" does not imply a large universe like the one we live in, but rather tiny curved universes that would collapse immediately", says Jean-Luc Lehners, who leads the "theoretical cosmology" group at the AEI.
Hence one cannot circumvent the big bang so easily. Lehners and his colleagues are now trying to figure out what mechanism could have kept those large quantum fluctuations in check under the most extreme circumstances, allowing our large universe to unfold.

Inflation from Supersymmetry Breaking
We explore the possibility that inflation is driven by supersymmetry breaking with the superpartner of the goldstino (sgoldstino) playing the role of the inflaton. Moreover, we impose an R-symmetry that allows to satisfy easily the slow-roll conditions, avoiding the so-called η-problem, and leads to two different classes of small field inflation models; they are characterised by an inflationary plateau around the maximum of the scalar potential, where R-symmetry is either restored or spontaneously broken, with the inflaton rolling down to a minimum describing the present phase of our Universe. To avoid the Goldstone boson and remain with a single (real) scalar field (the inflaton), R-symmetry is gauged with the corresponding gauge boson becoming massive. This framework generalises a model studied recently by the present authors, with the inflaton identified by the string dilaton and R-symmetry together with supersymmetry restored at weak coupling, at infinity of the dilaton potential. The presence of the D-term allows a tuning of the vacuum energy at the minimum. The proposed models agree with cosmological observations and predict a tensor-to-scalar ratio of primordial perturbations 10 − 9 <∼ r <∼ 10 − 4 and an inflation scale 1010 GeV <∼ H ∗ <∼ 1012 GeV. H ∗ may be lowered up to electroweak energies
only at the expense of fine-tuning the scalar potential.

Intrinsic Non-Commutativity of Closed String Theory
One of the annoying technicalities of string theory is the presence of co-cycles in the physical vertex operators. In the standard account, these co-cycles are required in order to maintain locality on the worldsheet, i.e., to obtain mutual locality of physical vertex insertions. For example, they appear in standard discussions [1] of compactified strings, and rapidly lead to both technical and conceptual issues. In this paper, we re-analyze these issues carefully, and show that the space of string zero modes surprisingly is best interpreted as non-commutative, with the scale of non-commutativity set
by α". A by-product of this realization is that the operator algebra becomes straightforward (albeit with a non-commutative product), with no need for co-cycles. This is not inconsistent with our usual notion of space-time in decompactification limits, but it does significantly impact the interpretation of compactifications in terms of local effective field theories. This is a central ingredient that has been overlooked in any of the attempts at duality symmetric formulations of string theory. Indeed, in a follow-up paper we will show that one can obtain a simple understanding of exotic backgrounds
such as asymmetric orbifolds [2] and T-folds [3]. Much of the usual space-time interpretation that we use in string theory is built in from the
beginning. Its origins, for example, as an S-matrix theory in Minkowski space-time is emblematic of its interpretation in terms of a collection of particle states propagating in a fixed space-time background. We typically view other solutions of string theory in a similar way, with a well-defined distinction between what is big and what is small. Each such case can be viewed as a classical or semi-classical approximation to a deeper quantum theory in which the notion of a given space-time is not built in from the beginning, but is an emergent property of a given classical limit. It is natural to ask under what circumstances a local effective field theory is obtained. Of course, we know many such instances, and we also know many examples where this does not occur, such as cases where non-commutative field theories are thought to emerge. Perhaps the avatar for the absence of a fixed space-time picture is given by duality-symmetric formulations (of which double field theories [4] and our own metastring theory [5–10], are examples). We are in fact working towards a new notion of quantum space-time, in which non-commutativity plays a central role, much as it does in ordinary quantum mechanics. In the present paper then, we uncover an important step towards such an understanding of quantum space-time.

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