کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
8188335 | 1528837 | 2013 | 4 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Finsler geometric perspective on the bulk flow in the universe
ترجمه فارسی عنوان
دیدگاه هندسی فینلر بر جریان فشرده در جهان
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موضوعات مرتبط
مهندسی و علوم پایه
فیزیک و نجوم
فیزیک هسته ای و انرژی بالا
چکیده انگلیسی
Astronomical observations showed that there may exist a bulk flow with peculiar velocities in the universe, which contradicts with the ÎCDM model. The bulk flow reveals that the observational universe is anisotropic at large scales. In fact, a more reliable observation on the anisotropy of spacetime comes from the CMB power spectra. The WMAP and Planck satellites both show that there is a hemispherical power asymmetry at large-angular scales. In this Letter, we propose a “wind” scenario to the bulk flow (or the anisotropy of spacetime). Under the influence of the “wind”, the spacetime metric could become a Finsler structure. By resolving the null geodesic equation, we obtain the modified luminosity distance, which has a dipolar form at the leading order. Thus, the “wind” describes well the bulk flow. In addition, we perform a least-Ï2 fit to the data of type Ia supernovae (SNe Ia) in the Union2.1 compilation. The peculiar velocity of the bulk flow has an upper limit vbulkâ²4000km/s, which is compatible with all the existing observational values.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Physics Letters B - Volume 723, Issues 4â5, 25 June 2013, Pages 257-260
Journal: Physics Letters B - Volume 723, Issues 4â5, 25 June 2013, Pages 257-260
نویسندگان
Zhe Chang, Ming-Hua Li, Sai Wang,