The big constant out, the small constant in

Gregory Gabadadze

    Research output: Contribution to journalArticle

    Abstract

    Some time ago, Tseytlin has made an original and unusual proposal for an action that eliminates an arbitrary cosmological constant. The form of the proposed action, however, is strongly modified by gravity loop effects, ruining its benefit. Here I discuss an embedding of Tseytlin's action into a broader context, that enables to control the loop effects. The broader context is another universe, with its own metric and dynamics, but only globally connected to ours. One possible Lagrangian for the other universe is that of unbroken AdS supergravity. A vacuum energy in our universe does not produce any curvature for us, but instead increases or decreases the AdS curvature in the other universe. I comment on how to introduce the accelerated expansion in this framework in a technically natural way, and consider the case where this is done by the self-accelerated solutions of massive gravity and its extensions.

    Original languageEnglish (US)
    Pages (from-to)263-268
    Number of pages6
    JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
    Volume739
    DOIs
    StatePublished - Dec 2 2014

    Fingerprint

    universe
    curvature
    gravitation
    supergravity
    embedding
    proposals
    vacuum
    expansion
    energy

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Cite this

    The big constant out, the small constant in. / Gabadadze, Gregory.

    In: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Vol. 739, 02.12.2014, p. 263-268.

    Research output: Contribution to journalArticle

    @article{fc2db957b85b4aa68ec22496dd2af8e8,
    title = "The big constant out, the small constant in",
    abstract = "Some time ago, Tseytlin has made an original and unusual proposal for an action that eliminates an arbitrary cosmological constant. The form of the proposed action, however, is strongly modified by gravity loop effects, ruining its benefit. Here I discuss an embedding of Tseytlin's action into a broader context, that enables to control the loop effects. The broader context is another universe, with its own metric and dynamics, but only globally connected to ours. One possible Lagrangian for the other universe is that of unbroken AdS supergravity. A vacuum energy in our universe does not produce any curvature for us, but instead increases or decreases the AdS curvature in the other universe. I comment on how to introduce the accelerated expansion in this framework in a technically natural way, and consider the case where this is done by the self-accelerated solutions of massive gravity and its extensions.",
    author = "Gregory Gabadadze",
    year = "2014",
    month = "12",
    day = "2",
    doi = "10.1016/j.physletb.2014.10.064",
    language = "English (US)",
    volume = "739",
    pages = "263--268",
    journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",
    issn = "0370-2693",
    publisher = "Elsevier",

    }

    TY - JOUR

    T1 - The big constant out, the small constant in

    AU - Gabadadze, Gregory

    PY - 2014/12/2

    Y1 - 2014/12/2

    N2 - Some time ago, Tseytlin has made an original and unusual proposal for an action that eliminates an arbitrary cosmological constant. The form of the proposed action, however, is strongly modified by gravity loop effects, ruining its benefit. Here I discuss an embedding of Tseytlin's action into a broader context, that enables to control the loop effects. The broader context is another universe, with its own metric and dynamics, but only globally connected to ours. One possible Lagrangian for the other universe is that of unbroken AdS supergravity. A vacuum energy in our universe does not produce any curvature for us, but instead increases or decreases the AdS curvature in the other universe. I comment on how to introduce the accelerated expansion in this framework in a technically natural way, and consider the case where this is done by the self-accelerated solutions of massive gravity and its extensions.

    AB - Some time ago, Tseytlin has made an original and unusual proposal for an action that eliminates an arbitrary cosmological constant. The form of the proposed action, however, is strongly modified by gravity loop effects, ruining its benefit. Here I discuss an embedding of Tseytlin's action into a broader context, that enables to control the loop effects. The broader context is another universe, with its own metric and dynamics, but only globally connected to ours. One possible Lagrangian for the other universe is that of unbroken AdS supergravity. A vacuum energy in our universe does not produce any curvature for us, but instead increases or decreases the AdS curvature in the other universe. I comment on how to introduce the accelerated expansion in this framework in a technically natural way, and consider the case where this is done by the self-accelerated solutions of massive gravity and its extensions.

    UR - http://www.scopus.com/inward/record.url?scp=84909594845&partnerID=8YFLogxK

    UR - http://www.scopus.com/inward/citedby.url?scp=84909594845&partnerID=8YFLogxK

    U2 - 10.1016/j.physletb.2014.10.064

    DO - 10.1016/j.physletb.2014.10.064

    M3 - Article

    VL - 739

    SP - 263

    EP - 268

    JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

    JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

    SN - 0370-2693

    ER -