Dark matter and spacetime symmetry restoration

被引:1
|
作者
Magueijo, Joao [1 ]
机构
[1] Imperial Coll, Blackett Lab, Theoret Phys Grp, Prince Consort Rd, London SW7 2BZ, England
关键词
TIME;
D O I
10.1103/PhysRevD.109.124026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine local physics in the presence of global variables: variables associated with the whole of the spacelike surfaces of a foliation. These could be the (pseudo)constants of nature and their conjugate times, but our statements are more general. Interactions between the local and the global (for example, dependence of the local action on global times dual to constants) degrades full space-time diffeomorphism invariance down to spatial diffeomorphism invariance, and so an extra degree of freedom appears. When these presumably primordial global interactions switch off, the local action recovers full invariance and so the usual two gravitons, but a legacy matter component is left over, bearing the extra degree of freedom. Under the assumption that the preferred foliation is geodesic, this component behaves like dark matter, except that 3 of its 4 local degrees of freedom are frozen, forcing its rest frame to coincide with the preferred foliation. The nonfrozen degree of freedom (the number density of the effective fluid) is the survivor of the extra "graviton " present in the initial theory and keeps memory of all the past global interactions that took place in a given location in the preferred foliation. Such "painted-on " dark matter is best distinguished from the conventional one in situations where the preferred frame would be preposterous if all 4 degrees of freedom of dark matter were available. We provide one example: an outflowing halo of legacy matter with exact escape speed at each point and a very specific profile, surrounding a condensed structure made of normal matter.
引用
下载
收藏
页数:12
相关论文
共 50 条
  • [1] Spacetime and dark matter from spontaneous breaking of Lorentz symmetry
    Zlosnik, Tom
    Urban, Federico
    Marzola, Luca
    Koivisto, Tomi
    CLASSICAL AND QUANTUM GRAVITY, 2018, 35 (23)
  • [2] Dark Energy and Spacetime Symmetry
    Dymnikova, Irina
    UNIVERSE, 2017, 3 (01)
  • [3] Electroweak symmetry non-restoration from dark matter
    Matsedonskyi, Oleksii
    Unwin, James
    Wang, Qingyun
    JOURNAL OF HIGH ENERGY PHYSICS, 2021, 2021 (12)
  • [4] Electroweak symmetry non-restoration from dark matter
    Oleksii Matsedonskyi
    James Unwin
    Qingyun Wang
    Journal of High Energy Physics, 2021
  • [5] Is galaxy dark matter a property of spacetime?
    Carmeli, M
    INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 1998, 37 (10) : 2621 - 2625
  • [6] Dark matter from spacetime nonlocality
    Saravani, Mehdi
    Aslanbeigi, Siavash
    PHYSICAL REVIEW D, 2015, 92 (10):
  • [7] Plasticity of spacetime as an alternative to dark matter
    Feoli, Antonio
    MODERN PHYSICS LETTERS A, 2018, 33 (33)
  • [8] Dark matter effects in vacuum spacetime
    Rizzi, Luca
    Cacciatori, Sergio L.
    Gorini, Vittorio
    Kamenshchik, Alexander
    Piattella, Oliver F.
    PHYSICAL REVIEW D, 2010, 82 (02):
  • [9] Is Galaxy Dark Matter a Property of Spacetime?
    Moshe Carmeli
    International Journal of Theoretical Physics, 1998, 37 : 2621 - 2625
  • [10] Spherical symmetry in a dark energy permeated spacetime
    Radicella, Ninfa
    Sereno, Mauro
    Tartaglia, Angelo
    CLASSICAL AND QUANTUM GRAVITY, 2012, 29 (11)