Finslerian dipolar modulation of the CMB power spectra at scales $$2<l<600$$ 2 < l < 600

Finslerian dipolar modulation of the CMB power spectra at scales $$2<l<600$$ 2 < l < 600

Abstract A common explanation for the CMB power asymmetry is to introduce a dipolar modulation at the stage of inflation, where the primordial power spectrum is spatially varying. If the universe in the stage of inflation is Finslerian, and if the Finsler spacetime is non-reversible under parity fli...

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Bibliographic Details
Main Authors: Xin Li, Hai-Nan Lin
Format: Article
Language:English
Published: SpringerOpen 2017-05-01
Series:European Physical Journal C: Particles and Fields
Subjects:
Cosmic Microwave Background
Background Spacetime
Inflation Model
Power Asymmetry
Gravitational Field Equation
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-4897-3

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http://link.springer.com/article/10.1140/epjc/s10052-017-4897-3

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