Quantum foam, gravitational thermodynamics, and the dark sector

被引:3
|
作者
Ng, Y. Jack [1 ]
机构
[1] Univ N Carolina, Dept Phys & Astron, Inst Field Phys, Chapel Hill, NC 27599 USA
关键词
COSMOLOGICAL-CONSTANT; SPACETIME FOAM; NEWTONIAN DYNAMICS; HOLOGRAPHIC FOAM; X-RAY; GRAVITY;
D O I
10.1088/1742-6596/845/1/012001
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Is it possible that the dark sector (dark energy in the form of an effective dynamical cosmological constant, and dark matter) has its origin in quantum gravity? This talk sketches a positive response. Here specifically quantum gravity refers to the combined effect of quantum foam (or spacetime foam due to quantum fluctuations of spacetime) and gravitational thermodynamics. We use two simple independent gedankan experiments to show that the holographic principle can be understood intuitively as having its origin in the quantum fluctuations of spacetime. Applied to cosmology, this consideration leads to a dynamical cosmological constant of the observed magnitude, a result that can also be obtained for the present and recent cosmic eras by using unimodular gravity and causal set theory. Next we generalize the concept of gravitational thermodynamics to a spacetime with positive cosmological constant (like ours) to reveal the natural emergence, in galactic dynamics, of a critical acceleration parameter related to the cosmological constant. We are then led to construct a phenomenological model of dark matter which we call "modified dark matter" (MDM) in which the dark matter density profile depends on both the cosmological constant and ordinary matter. We provide observational tests of MDM by fitting the rotation curves to a sample of 30 local spiral galaxies with a single free parameter and by showing that the dynamical and observed masses agree in a sample of 93 galactic clusters. We also give a brief discussion of the possibility that quanta of both dark energy and dark matter are non-local, obeying quantum Boltzmann statistics (also called infinite statistics) as described by a curious average of the bosonic and fermionic algebras. If such a scenario is correct, we can expect some novel particle phenomenology involving dark matter interactions. This may explain why so far no dark matter detection experiments have been able to claim convincingly to have detected dark matter.
引用
收藏
页数:13
相关论文
共 50 条
  • [1] Gravitational wave from dark sector with dark pion
    Tsumura, Koji
    Yamada, Masatoshi
    Yamaguchi, Yuya
    [J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2017, (07):
  • [2] Gravitational production of a conformal dark sector
    Redi, Michele
    Tesi, Andrea
    Tillim, Hannah
    [J]. JOURNAL OF HIGH ENERGY PHYSICS, 2021, 2021 (05)
  • [3] Gravitational production of a conformal dark sector
    Michele Redi
    Andrea Tesi
    Hannah Tillim
    [J]. Journal of High Energy Physics, 2021
  • [4] Thermodynamics as a tool for (quantum) gravitational dynamics
    Alonso-Serrano, Ana
    Liska, Marek
    [J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2023, 32 (14):
  • [5] Gravitational wave constraints on dark sector models
    Battye, Richard A.
    Pace, Francesco
    Trinh, Damien
    [J]. PHYSICAL REVIEW D, 2018, 98 (02)
  • [6] Gravitational thermodynamics of spacetime foam in one-loop approximation
    Liu, L
    Ma, YG
    [J]. INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2000, 9 (01): : 91 - 95
  • [7] Gravitational quantum foam and supersymmetric gauge theories
    Maeda, T
    Nakatsu, T
    Noma, Y
    Tamakoshi, T
    [J]. NUCLEAR PHYSICS B, 2006, 735 (1-3) : 96 - 126
  • [8] Gravitational wave signatures from dark sector interactions
    Bernardo, Reginald Christian
    [J]. PHYSICAL REVIEW D, 2021, 104 (02)
  • [9] A Quantum Approach to Dark Matter Sector
    Ennadifi, Salah Eddine
    [J]. AFRICAN REVIEW OF PHYSICS, 2015, 10 : 503 - 506
  • [10] Quantum simulations of dark sector showers
    Chigusa, So
    Yamazaki, Masahito
    [J]. PHYSICS LETTERS B, 2022, 834