|  The Cosmological-Constant Problem | 
In General
  > s.a. boundaries in field theory; branes;
  quintessence; vacuum.
  * Idea: The current formulation
    of the problem is, Why is the observed value of the cosmological constant so small
    (e.g., after so many phase transitions)? [Before 1997-1998, the question usually
    was, Why is its observed value zero?]
  * Second problem: The coincidence
    between the epoch of galaxy formation tgal
    and the epoch of Λ-domination tcc;
    > s.a. Coincidence Problem.
  @ Reviews: Adler et al AJP(95)jul;
    Dolgov ap/97-proc;
    Weinberg ap/00-conf;
    Straumann ap/00-conf,
      ap/02-conf,
      gq/02-conf;
    Brax CP(04);
    Banks PT(04)mar;
    Nobbenhuis PhD(06)gq [approaches];
    Solà JPCS(13)-a1306 [pedagogical];
    Burgess a1309-ln [the naturalness problem and microphysics];
    Padilla a1502-ln;
    Ng a1706-proc [approaches].
  @ And the equivalence principle: Bertolami IJMPD(09) [violation]; Ginat a2105-GRF [the equivalence principle helps].
Higher-Dimensional Proposed Solutions
  * Idea: Many proposals
    have been made; 2000, recent ones include large extra dimensions
    (> see brane cosmology).
  @ Strings / M-theory: Witten MPLA(95)ht,
    Kane et al PLB(05) [string vacua];
    McGuigan ht/06,
    ht/06 [seesaw];
    Hawking & Hertog PRD(06)
    + pn(06)jun;
    de Alwis PLB(07)ht/06;
    Bousso ht/06-talk [local values and the landscape];
    Barvinsky PRL(07);
    Kiefer et al CQG(11)-a1010 [landscape-motivated];
    Avilán & Roldán a1011;
    Bousso a1203-proc [and the string theory landscape];
    Sumitomo & Tye JCAP(12)-a1204 [simple stringy mechanism];
    > s.a. string phenomenology.
  @ Brane world:
    Burgess et al PLB(00);
    Förste et al JHEP(00);
    Chen et al JHEP(00);
    Arkani-Hamed et al PLB(00)ht;
    Kakushadze PLB(00)ht,
    PLB(00)ht,
    PLB(00)ht;
    de Alwis NPB(01);
    Flanagan et al PRD(01) [and hierarchy];
    Tye & Wasserman PRL(01);
    Nojiri et al RMF(02)ht/01;
    Corradini et al MPLA(03),
    IJMPA(03)ht/02;
    Sorkin BJP(05)gq-proc [the value of Λ would be too small];
    Ellwanger MPLA(05);
    Steinhard & Turok Sci(06)ap
    + pw(06)may
      [cyclic universe with decreasing cosmological constant],
    comment Vilenkin Sci(06)ap;
    Diakonos & Saridakis JCAP(09)-a0708;
    Shao & Chen PRD(10)-a1005.
  @ Other higher-dimensional: Wesson & Liu IJMPD(01)gq [Kaluza-Klein theory];
    Erdem JPA(07)gq/06-conf,
    JPA(08)-a0712 [symmetries];
    Hertzberg & Masoumi JCAP(16)-a1509.
Quantum Gravity and Modified-Gravity Solutions
  > s.a. modified general relativity; time in quantum theory.
  * Conformal gravity: The
    theory naturally quenches the amount by which the cosmological constant
    gravitates, rather than its value.
  @ Quantum cosmology: Hawking PLB(84);
    Weiss PLB(87),
    Duff PLB(89) [criticism];
    Wu PLB(08)-a0709;
    Shaw & Barrow PRD(11)-a1010 [value depends on observation time];
    Larsen et al PRD(11)-a1107 [in the quantum multiverse];
    Jalalzadeh et al PDU-a1709 [q-deformed];
    > s.a. quantum gravity phenomenology [including wormholes, baby universes].
  @ Lattice-type approaches:
    Vergeles ht/04 [lattice quantum gravity];
    Loll et al NPB(06) [2D causal, with topology change].
  @ And discrete spacetime: Mok ap/01;
    Trout a1208,
    a1208;
    Miković & Vojinović EPL(15)-a1407 [quantum Regge calculus approach].
  @ Other quantum gravity: Özer NPB(91) [third quantization];
    Alexander & Calcagni PLB(09)-a0806 [superconducting lqg];
    Mannheim MPLA(11)-a1005-conf [intrinsically quantum-mechanical gravity];
    Miao & Zhao IJMPD(14)-a1312 [and gup];
    Moffat a1407-proc [finite, unitary non-local formulation];
    Carlip PRL(19)-a1809,
    comment Wang & Unruh a1911,
    reply Carlip a1911,
    comment Piattella a2007
      [high curvature at Planck scales, hidden at observable scales];
    Hogan a2003
      [gravitational drag from coherent energy flows];
    > s.a. approaches to quantum gravity [gravity
      as condensate]; non-commutative cosmology.
  @ Related proposals:
    Linde PLB(88) [two universes];
    Özer gq/00
      [from gravity + electromagnetism unification];
    Sundrum PRD(04)ht/03 [fat gravitons];
    Alexander et al ht/04 [vacuum gravitational instability];
    Novello PoS-ap/05 [and graviton mass];
    Prokopec gq/06 [semiclassical general relativity + matter];
    Nojiri et al PLB(11)-a1010 [non-local gravity];
    García-Aspeitia a1011 [2D spacetime and Planck scale];
    Aslanbeigi et al PRD(11)-a1106,
    Wondrak a1705-conf [gravitational aether];
    Wilson JModP(13)-a1111;
    Finazzi et al PRL(12)
    + news at(12)feb,
    PhysOrg(12)mar [analog gravity and BECs];
    Mannheim a1703-GRF
      [fully quantum-mechanically consistent conformal gravity];
    Carroll & Remmen PRD(17)-a1703 [non-local constraint on the action];
    Vasak et al a1802 [covariant canonical gauge theory of gravity];
    Xiong a1805;
    Appleby & Linder a2009 [well tempering];
    > s.a. Übergravity.
Other Proposed Solutions > s.a. cosmological constant
  [scale dependence, variation, etc]; particle statistics [quons].
  * Remark: Supersymmetry doesn't help, it is broken!
  @ From vacuum fluctuations: Gurzadyan & Xue MPLA(03)ap/01,
    ap/05;
    Padmanabhan CQG(05)ht/04;
    Qi ht/05 [QED];
    Samuel & Sinha PRL(06)cm [surface tension analog];
    Beck & Mackey PhyA(07)ap/06 [measurability];
    Doran & Jaeckel JCAP(06)ap [and measurements];
    Maggiore PRD(11);
    Wang et al PRD(17)-a1703 [gravitating vacuum energy];
    Wetterich PLB(17)-a1704 [graviton fluctuations];
    Pejhan et al PLB(18)-a1808 [from the Krein-Gupta-Bleuler vacuum];
    Brax & Valageas a1903 [cancellation mechanism];
    Carlip a1905-GRF [hidden by spacetime foam];
    Bengochea et al a1906 [problematic];
    Viaggiu FP-a1910 [and metric averaging  procedure];
    Leonhardt a2001 [in Lifshitz theory];
    Lozano & Mazzitelli a2008 [oscillating universe from random fluctuations].
  @ Supersymmetric: Jejjala et al GRG(03)ht-GRF [holography and supersymmetry];
    Froggatt et al NPB(06) [supergravity models].
  @ And holography: Arzano et al PLB(07)gq/06;
    Carneiro IJMPD(03)gq-GRF;
    > s.a. holography.
  @ Other fields:
    Barr et al PRD(06) [cancellation by cosmon];
    Klinkhamer & Volovik JETPL(10)-a0907 [extension of standard model];
    Popławski AdP(11)-a1105 [quarks and torsion];
    Emelyanov & Klinkhamer PRD(12)-a1107,
    PRD(12)-a1109,
    Klinkhamer PRD(12) [two massless vector fields];
    Padmanabhan & Padmanabhan IJMPD(13)-a1302 [inflation and particle physics parameters];
    Nojiri MPLA(16)-a1601 [topological field theory];
    Ahluwalia a2008 [spin-1/2 boson].
  @ Other proposals:
    Duncan & Jensen NPB(90) [4-form dynamics];
    Ghoroku CQG(91);
    Ng IJMPD(92);
    Squires PLA(92);
    Sivaram MPLA(99) [early-universe phase transition];
    Nobbenhuis FP(06)gq/04;
    Jackiw et al PLA(05)ht [λφ4 field in AdS];
    Triay IJMPD(05)gq;
    Nishino & Rajpoot MPLA(06) [Hodge duality];
    Freese et al PLB(06) [devaluation];
    't Hooft & Nobbenhuis CQG(06)gq [complex transformations];
    Shapiro & Solà JPA(07)gq/06-conf;
    Comelli IJMPA(08)-a0704 [modified Lagrangian];
    O'Connell PLA(07) [causality-based];
    Rodrigo CQG(07)-a0705 [void bubbles];
    Andrianov et al PLB(07) [and spontaneous symmetry breaking];
    Urban & Zhitnitsky JCAP(09)-a0906 [standard-model physics];
    Linde & Vanchurin a1011 ["non-anthropic"];
    Koksma & Prokopec a1105 [Lorentz invariance of the vacuum];
    Maia IJMPcs(11)-a1107-talk [and spacetime deformation];
    Darabi a1107;
    Astashenok & Del Popolo CQG(12)-a1203 [with volume averaging];
    Jain et al IJMPA(15)-a1408 [conformal symmetry breaking];
    Kourkoulou et al a2101 [non-trivial cancellations, analog model].
Other Proposed Solutions > s.a. dynamical
  wave-function collapse; Topos Theory.
  * Anthropic approach:
    There is a probability distribution of values of the cosmological constant
    in different regions, and we live in one that is conducive to life.
  @ Anthropic approach:
    in Barrow & Tipler 86, ch6;
    Weinberg PRL(87);
    Efstathiou MNRAS(95);
    Garriga et al PRD(00)ap/99;
    Donoghue JHEP(00);
    Förste et al PLB(00)gq;
    Garriga & Vilenkin PRD(00)ap/99,
    PRD(01)ht/00;
    Barrow et al PRD(02)ap/01;
    Banks et al JHEP(01);
    Vilenkin in(03)ht/01;
    Graesser et al PLB(04)ht;
    Garriga & Vilenkin PTPS(06)ht/05;
    Loeb JCAP(06)ap [observational test];
    Starkman & Trotta PRL(06)ap,
    Trotta & Starkman AIP(06)ap [against];
    Pogosian & Vilenkin JCAP(07)ap/06 [and WMAP-3 data];
    Bousso et al PRD(07)ht [causal entropic principle];
    Miralda-Escudé ap/07 [stryngbohtyk model];
    Peacock MNRAS(07)-a0705;
    Olum & Schwartz-Perlov JCAP(07)-a0705 [in a large toy landscape];
    Maor et al PRL(08)-a0709 [criticism];
    Mersini-Houghton & Adams CQG(08)-a0810 [limitations];
    Maia & Capistrano IJMPA(09)-a0905;
    Iorio MNRAS(10)-a0911 [the Sun's motion through the Milky Way];
    Hong et al PRD(12)-a1110 [and primordial density perturbations];
    Hartle & Hertog PRD(13)-a1309 [anthropic bounds from the no-boundary quantum state];
    Berolami & Páramos GRG(20) [non-minimally coupled].
  @ No zero-point energy contributions: Kimpton & Padilla JHEP(12)-a1112;
    Bernard & LeClair PRD(13)-a1211;
    Kaloper & Padilla PRL(14)-a1309,
    PRD(104)-a1406 [sequestering];
    Fujii a1403;
    Balitsky & Kiselev PRD(14)-a1406 [vacuum energy suppression];
    Barrow & Cotsakis a1907 [traceless f(R) gravity];
    Yargic et al PRD-a2001
      [only part of the stress-energy tensor gravitates];
    Donoghue a2009 [in perturbation theory];
    > s.a.  canonical quantization [covariant].
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