Can Chameleon Fields Be the Source of the Dark Energy Dipole and the Cosmic Microwave Background Dipole?

被引:1
|
作者
Yarahmadi, Muhammad [1 ]
Salehi, Amin [1 ]
机构
[1] Lorestan Univ, Khorramabad, Iran
来源
ASTROPHYSICAL JOURNAL | 2024年 / 964卷 / 01期
关键词
SCALE PECULIAR VELOCITIES; 100 H(-1) MPC; BULK FLOW; ELLIPTIC GALAXIES; LAMBDA-CDM; CLUSTERS; MOTION; SPECTROSCOPY; PHOTOMETRY; ANISOTROPY;
D O I
10.3847/1538-4357/ad1f5f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recent research reveals that the Local Group is in motion toward (l, b) = (276, 30) relative to the cosmic background radiation, manifesting a velocity of 600 km s(-1), a phenomenon recognized as the cosmic background radiation dipole or cosmic microwave background dipole. Despite its well-documented nature, the precise cause of this peculiar motion remains elusive. High mass-density regions, such as galactic superclusters, stand out among the potential contributors to this cosmic flow. This paper employs chameleon fields to investigate anisotropies on both small and large scales. The data utilized in this study comprise Type Ia supernovae from the Pantheon catalog, totaling 1048 supernovae within the redshift range of 0.015 < z < 2.3. The analysis of the bulk flow at various redshifts has yielded noteworthy discoveries. On a smaller scale (less than 150 Mpc), the movement direction of the Local Group coincides with that of the bulk flow. On a larger scale, the bulk flow direction corresponds to the direction of the dark energy dipole. This implies that the anisotropy at the local scale originates from the same source as the anisotropy observed on a larger scale.
引用
收藏
页数:15
相关论文
共 50 条
  • [1] Aspects of the cosmic microwave background dipole
    Kamionkowski, M
    Knox, L
    PHYSICAL REVIEW D, 2003, 67 (06):
  • [2] The dipole anisotropy of the cosmic microwave background radiation
    Melchiorri, B
    Melchiorri, F
    Signore, M
    NEW ASTRONOMY REVIEWS, 2002, 46 (11) : 693 - 698
  • [3] Is the Radio Source Dipole from NVSS Consistent with the Cosmic Microwave Background and ΛCDM?
    Cheng, Yun-Ting
    Chang, Tzu-Ching
    Lidz, Adam
    ASTROPHYSICAL JOURNAL, 2024, 965 (01):
  • [4] DIPOLE ANISOTROPY AND DISTORTIONS OF THE SPECTRUM OF THE COSMIC MICROWAVE BACKGROUND
    DANESE, L
    DEZOTTI, G
    ASTRONOMY & ASTROPHYSICS, 1981, 94 (02) : L33 - L34
  • [5] Cosmic microwave background dipole induced by double inflation
    Langlois, D
    PHYSICAL REVIEW D, 1996, 54 (04): : 2447 - 2450
  • [6] IS THE COSMIC MICROWAVE BACKGROUND ASYMMETRY DUE TO THE KINEMATIC DIPOLE?
    Naselsky, P.
    Zhao, W.
    Kim, J.
    Chen, S.
    ASTROPHYSICAL JOURNAL, 2012, 749 (01):
  • [7] Dipole modulation of cosmic microwave background temperature and polarization
    Ghosh, Shamik
    Kothari, Rahul
    Jain, Pankaj
    Rath, Pranati K.
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2016, (01):
  • [8] Cosmic microwave background dipole induced by double inflation
    Langlois, D.
    Physical Review D Particles, Fields, Gravitation and Cosmology, 54 (04):
  • [9] Cosmic microwave background dipole from an entropy gradient
    Langlois, D
    Piran, T
    PHYSICAL REVIEW D, 1996, 53 (06) : 2908 - 2919
  • [10] Cosmic microwave background dipole from an entropy gradient
    Langlois, D.
    Piran, T.
    (53):