|  Geons | 
In General
  > s.a. 3D manifolds [prime factors]; general
  relativity solutions;  Mapping Class.
  * History: A precursor
    was given by the concept of gravitational bag; The original meaning
    of the term, as used by Wheeler, referred to non-topological geons.
  > Similar concepts:
    see defects; Kinks.
Non-Topological > s.a. Boson Stars;
  Galileon Field; solitons.
  * Idea: An object with
    particle-like properties made out of the spacetime metric, and possibly
    other fields.
  @ General references: Wheeler PR(55);
    Power & Wheeler RMP(57) [thermal];
    Brill & Hartle PR(64) [gravitational waves].
  @ Modified gravity: Vollick CQG(08)-a0807,
    CQG(10)-a1004 [1+1 Jackiw-Teitelboim theory with higher-order corrections];
    Afonso et al JCAP(17)-a1705 [Born-Infeld gravity].
  @ Gravity + scalar field: Barreto et al PRD(96)gq/05 [turning point instability];
    Sones gq/05 [+ electromagnetism].
  @ Related topics: Cooperstock et al MPLA(95) [non-existence],
    IJMPD(96)gq/95 [critical analysis of Brill-Hartle geon];
    Perry & Cooperstock CQG(99)gq/98 [stability];
    > s.a. anti-de sitter spacetime [instability].
Topological (More recent meaning) > s.a. CPT symmetry;
  measurement in quantum theory; spin-statistics theorem.
  * Idea: An object with
    particle-like properties made out of spatial geometry; Part of the motivation
    is that one may be able to account for some non-gravitational charges (e.g.,
    electric charge) using topology.
  * Remark: The concept is
    similar to that of gravitational "kink", but the latter is used
    to describe a topologically non-equivalent metric tensor fields defined
    on a given fixed manifold.
  * Types: They can be spinorial,
    fermionic, possibly chiral; Some can switch between bosonic and fermionic
    behavior after interactions.
  * Question: Can they be preons?
  * Example: Wheeler's "single
    wormhole mouth" (not "quasi-localized").
  @ General references: Finkelstein & Misner AP(59);
    Finkelstein JMP(66);
    Cohen & Wald JMP(72);
    Sorkin JPA(77);
    Shastri et al IJTP(80);
    Whiston JPA(81) [classification, including fermionic];
    Williams & Finkelstein IJTP(84);
    Bais et al NPB(87);
    Sorkin in(86),
    in(89);
    Bugajska IJTP(87);
    Dunn et al JMP(91);
    Williams & Zvengrowski JMP(92);
    Dunn et al JMP(96) [geodesic incompleteness];
    Anderson & Brill PRD(97)gq/96;
    Balachandran et al GRG(11)-a1009 [and non-commutative spacetimes].
  @ Phenomenology: Srivastava PRD(87);
    Olmo & Rubiera-García JCAP(14) [at particle accelerators].
  @ Solutions: Harriott & Williams GRG(03) [4D rotating kink];
    Louko et al CQG(05)gq/04 [with spin and charge];
    > s.a. black-hole solutions.
  @ With cosmological constant: Dunn & Williams JMP(89),
    et al JMP(94) [locally de Sitter].
  @ In 1+1 dimensions: Vasilić & Vukašinac
      CQG(96);
    Klösch & Strobl PRD(98)gq/97.
  @ In 2+1 dimensions: Harriott & Williams NCB(05) [kink number];
    Stevens et al CQG(09)-a0809 [no asymptotically flat ones];
    Galloway et al CMP(12)-a1005 [non-existence result].
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  send feedback and suggestions to bombelli at olemiss.edu – modified 26 jun 2018