|  String Theory Phenomenology | 
Particle Physics in General > s.a. axions; CPT symmetry;
  GUTs; higher-spin fields; neutrino;
  yang-mills theory.
  * Idea: The lowest excited modes of
    open strings correspond to massless spin-1 particles (the photon, \(W^\pm\), \(Z\)
    and gluons); Those of closed strings are massless spin-2 particles (the graviton).
  * Enhançon:
    A hypersurface (spherical in the initial proposal), apparently made of D-branes,
    which arises in string theory studies of large-N SU(N) pure gauge
    theories with eight supercharges.
  @ General references: Faraggi ht/97-proc,
      ht/99-proc;
    Quevedo NPPS(98)hp/97;
    Ibáñez CQG(00)hp/99-proc;
    Sudarsky et al PRD(03) [bounds from low-energy data];
    Dine PT(07)dec [rev];
    Antoniadis IJMPA(10) [rev];
    Ibáñez a1204-ln [rev];
    Ibáñez & Uranga 12;
    Faraggi a1404-conf;
    Kane IJMPA(15) [how to make contact with the 4D world];
    Kane a1601 [string theory is testable];
    Quevedo a1612-conf.
  @ And QCD: Aharony ht/02-ln;
    Evans pw(03)may;
    Mateos CQG(07)-a0709-ln;
    Lüst IJMPA(10).
  @ And gauge theory: Polyakov NPPS(98)ht/97 [confinement],
    IJMPA(99);
    Ghilencea & Groot Nibbelink CQG(03) [corrections to couplings];
    Imeroni PhD(03)ht;
    Sugimoto & Takahashi JHEP(04)ht [and QED];
    Caselle et al JHEP(05)hl [Nambu-Goto string and interquark potential];
    Heckman CP(10) [F-theory GUTs and experiment].
  @ Accelerator physics: Dudas & Mourad NPB(00)ht/99;
    Antoniadis & Benakli IJMPA(00),
    Antoniadis IJMPA(06)in [also branes];
    Distler et al PRL(07)hp/06
     + sr(07)jan [prediction and falsifiability in W-boson scattering];
     Anchordoqui et al NPB(09);
     Anchordoqui et al PRD(14)-a1407 [hadron colliders].
  @ Enhançon: Jarv & Johnson PRD(00)ht;
    Johnson PRD(01)ht/00;
    Astefanesei & Myers JHEP(02)ht/01,
    Dyson et al JHEP(02)ht/01 [non-spherical];
    Merlatti NPB(02)ht/01 [fractional branes].
And Gravity > s.a. brane world; covariant quantum
  gravity and other approaches; quantum-gravity phenomenology.
  * Idea: While the matter content of
    the theory is dependent on the compactification, in string theory the presence of
    gravity in the spectrum is universal; General relativity is recovered in the sense
    of an effective interaction between strings in scattering processes; Early suggestions
    were from Scherk & Schwarz &(74) and Yoneya &(74); The first correction
    to the action for general relativity  is a Gauss-Bonnet term; String theory yields
    ultraviolet finite scattering amplitudes in theories of gravity coupled to matter.
  * Questions: Get black holes (and
    black-hole evaporation); Planck-scale behavior (Are there singular solutions?
    Are they generic? Singularity theorems?).
  * Problem: Conformal ambiguity
    in the physical metric.
  * Black-hole information paradox: It is
    resolved by the picture of quantum black-hole microstates as horizon-sized objects called
    'fuzzballs' instead of vacuum regions with a central singularity; Causality requires that
    the wavefunctional has an important component not present in the semiclassical picture,
    virtual fuzzballs; The large mass of the fuzzballs suppresses their virtual fluctuations,
    but this suppression is compensated by the large number exp\([S_{\rm B}(M)]\) of possible
    fuzzballs, which are extended compression-resistant objects; The presence of these objects
    in the vacuum wavefunctional alters the physics of collapse when a horizon is about to form,
    avoiding the information paradox; > s.a. Fuzzballs.
  @ Books, reviews: Giddings hp/05-ln;
    Yoneya a0901-ch [hist, 1969-1974];
    Blau & Theisen GRG(09) [open questions];
    Elvang & Horowitz a1311-ch;
    Ortín 15.
  @ General references:
    Boulware & Deser PRL(85);
    Sannan PRD(86);
    Banks & Lykken NPB(90);
    Smolin gq/96;
    Branson et al PLB(97)ht/96;
    Porrati LMP(99) [and general relativity];
    Green CQG(99)A;
    Aharony et al PRP(00) [and large-N field theories];
    Wessling & Wise PLB(01)ht;
    Polyakov IJMPA(02)ht/01  [thoughts];
    Siegel ht/03 [weakening at short scales];
    Horowitz NJP(05)gq/04 [spacetime];
    Arkani-Hamed et al JHEP(07)ht/06 [string landscape and quantum gravity];
    Roberts ht/06 [unified field theory];
    Damour & Lilley a0802-ln;
    Wadia a0809-in [rev, semi-technical];
    Deo et al G&C(09) [quantum gravity];
    Basu CQG(16)
    + CQG+ [one-loop gravitational interactions].
  @ Gravitational waves:
    Brustein ht/96 [background];
    Allen & Brustein PRD(97)gq/96 [and LIGO];
    Ungarelli & Vecchio AIP(00)gq/99;
    Cartier et al NPB(01) [string cosmology].
    @ Black holes: Gimon & Hořava PLB(09)-a0706 [superspinning, violating the Kerr bound];
    Mathur a1812-proc [virtual fuzzballs];
    Pietri a1911-PhD;
    > s.a. quantum black holes.
  @ Solutions: Coley PRL(02) [vanishing curvature invariants];
    Petri gq/04 [holographic];
    Hernández et al G&C(09) [stationary axisymmetric];
    > s.a. black holes.
  @ Supergravity: Witten NPB(95)ht;
    Aspinwall NPPS(96)ht/95;
    Stelle ht/05-proc [divergence structure];
    Deo IJMPA(06)ht/05 [derivation];
    Gaillard a1602-in;
    Reid-Edwards & Riccombeni JHEP(17)-a1701 [superstring field theory].
  > Related topics: see corrections
    to newtonian gravity; graviton; quantum spacetime;
    spacetime; schwarzschild spacetime;
    uncertainty.
Astrophysics and Other Areas > s.a. anthropic
  principle; string cosmology.
  * Landscape: The name refers
    to a plot shaped like a mountainous landscape, where altitude represents the
    cosmological constant, with its value settling on a low point somewhere between the peaks
    of the landscape; But there could be on the order of 10500
    possible such low points, and no obvious reason for the universe to pick the one we observe;
    Seen either as a virtue (e.g., in parallel worlds scenarios) or as a sign of inability
    to make predictions.
  @ General references: Kane PT(97)feb;
    Musser SA(02)oct;
    Gates PT(06)jun;
    editorial pw(07)sep;
    Kane PT(10)nov.
  @ Astronomy / astrophysics: Mavromatos JPCS(09)-a0903 [high-energy gamma rays];
    Ellis et al PRD(19)-a1810 [D-particles and the hydrogen 21-cm line].
  @ Applications to other areas: 
    Borsten et al PRL(10)
    + wired(10)sep
      [and four-qubit entanglement classification];
    McGreevy Phy(10)
    + nat(10)oct [strange metals];
    > s.a. condensed matter physics.
  @ Landscape:
    Quevedo pw(03)nov;
    Bousso & Polchinski SA(04)sep;
    Douglas ht/06-conf;
    Schellekens phy/06 [general audience];
    Conlon CP(06);
    Acharya & Douglas ht/06 [finite?];
    Rej a0909-FQXi
      [decidability, computability and complexity];
    Smolin FP(13)-a1202 [historical roots and speculative scenarios];
    Banks a1208.
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