6,782 research outputs found
Species and Strings
Based on well-known properties of semi-classical black holes, we show that
weakly-coupled string theory can be viewed as a theory of N = 1/g_s^2 particle
species. This statement is a string theoretic realization of the fact that the
fundamental scale in any consistent D-dimensional theory of gravity is not the
Planck length l_D, but rather the species scale L_N = N^1/(D-2) l_D. Using this
fact, we derive the bound on semi-classical black hole entropy in any
consistent theory of gravity as S > N, which when applied to string theory
provides additional evidence for the former relation. This counting also shows
that the Bekenstein-Hawking entropy can be viewed as the entanglement entropy,
without encountering any puzzle of species. We demonstrate that the counting of
species extends to the M-theory limit. The role of the species scale is now
played by the eleven-dimensional Planck length, beyond which resolution of
distances is gravitationally-impossible. The conclusion is, that string theory
is a theory of species and gets replaced by a pure gravitational theory in the
limit when species become strongly coupled and decouple.Comment: 20 page
Strong Coupling Holography
We show that whenever a 4-dimensional theory with N particle species emerges
as a consistent low energy description of a 3-brane embedded in an
asymptotically-flat (4+d)-dimensional space, the holographic scale of
high-dimensional gravity sets the strong coupling scale of the 4D theory. This
connection persists in the limit in which gravity can be consistently
decoupled. We demonstrate this effect for orbifold planes, as well as for the
solitonic branes and string theoretic D-branes. In all cases the emergence of a
4D strong coupling scale from bulk holography is a persistent phenomenon. The
effect turns out to be insensitive even to such extreme deformations of the
brane action that seemingly shield 4D theory from the bulk gravity effects. A
well understood example of such deformation is given by large 4D Einstein term
in the 3-brane action, which is known to suppress the strength of 5D gravity at
short distances and change the 5D Newton's law into the four-dimensional one.
Nevertheless, we observe that the scale at which the scalar polarization of an
effective 4D-graviton becomes strongly coupled is again set by the bulk
holographic scale. The effect persist in the gravity decoupling limit, when the
full theory reduces to a 4D system in which the only memory about the
high-dimensional holography is encoded in the strong coupling scale. The
observed intrinsic connection between the high-dimensional flat space
holography and 4D strong coupling suggests a possible guideline for
generalization of AdS/CFT duality to other systems.Comment: 26 pages, Late
Self-Completeness of Einstein Gravity
We argue, that in Einsteinian gravity the Planck length is the shortest
length of nature, and any attempt of resolving trans-Planckian physics bounces
back to macroscopic distances due to black hole formation. In Einstein gravity
trans-Planckian propagating quantum degrees of freedom cannot exist, instead
they are equivalent to the classical black holes that are fully described by
lighter infra-red degrees of freedom and give exponentially-soft contribution
into the virtual processes. Based on this property we argue that pure-Einstein
(super)gravity and its high-dimensional generalizations are self-complete in
deep-UV, but not in standard Wilsonian sense. We suggest that certain
strong-coupling limit of string theory is built-in in pure Einstein gravity,
whereas the role of weakly-coupled string theory limit is to consistently
couple gravity to other particle species, with their number being set by the
inverse string coupling. We also discuss some speculative ideas generalizing
the notion of non-Wilsonian self-completeness to other theories, such as the
standard model without the Higgs.Comment: 40 pages, Late
The Confining String from the Soft Dilaton Theorem
A candidate for the confining string of gauge theories is constructed via a
representation of the ultraviolet divergences of quantum field theory by a
closed string dilaton insertion, computed through the soft dilaton theorem. The
resulting (critical) confining string is conformally invariant, singles out
naturally dimensions, and can not be used to represent theories with
Landau poles.Comment: 13 pages, two figures Clarifying remark added. Typos correcte
Memory and the Infrared
Memory effects in scattering processes are described in terms of the
asymptotic retarded fields. These fields are completely determined by the
scattering data and the zero mode part is set by the soft photon theorem. The
dressed asymptotic states defining an infrared finite S- matrix for charged
particles can be defined as quantum coherent states using the corpuscular
resolution of the asymptotic retarded fields. Im- posing that the net radiated
energy in the scattering is zero leads to the new set of conservation laws for
the scattering S-matrix which are equivalent to the decoupling of the soft
modes. The actual observabil- ity of the memory requires a non vanishing
radiated energy and could be described using the infrared part of the
differential cross section that only depends on the scattering data and the
radiated energy. This is the IR safe cross section with any number of emitted
pho- tons carrying total energy equal to the energy involved in the actual
memory detection
M and F-Theory Instantons, N=1 Supersymmetry and Fractional Topological Charges
We analize instanton generated superpotentials for three dimensional N=2
supersymmetric gauge theories obtained by compactifying on S^1 N=1 four
dimensional theories. In the N_f=1 case, we find that the vacua in the
decompactification limit is given by the singular points of the Coulomb branch
of the N=2 four dimensional theory (we also consider the massive case). The
decompactification limit of the superpotential for pure gauge theories without
chiral matter is interpreted in terms of `t Hooft's fractional instanton
amplitudes.Comment: Latex file. 11 pages. Typos corrected. Section on QCD has been
rewritten, clarifying some points, and a reference has been added. Final
version to appear at Int. Jour. Mod. Phys.
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