The imprint of primordial gravitational waves on the CMB intensity profile
We use the induced geometry on the two dimensional transverse cross section of a photon beam propagating on a perturbed Friedmann-Robertson-Walker (FRW) spacetime to find the Cosmic Microwave Background (CMB) photon distribution over a telescope's collecting area today. It turns out that at eac...
Main Author: | Ali Kaya |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2021-06-01
|
Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269321002938 |
Similar Items
-
CMB-S4: forecasting constraints on primordial gravitational waves
by: Abazajian, K, et al.
Published: (2022) -
Primordial gravitational waves measurements and anisotropies of CMB polarization rotation
by: Si-Yu Li, et al.
Published: (2015-12-01) -
Imprint of a scalar era on the primordial spectrum of gravitational waves
by: Francesco D'Eramo, et al.
Published: (2019-08-01) -
Gravitational wave and CMB probes of axion kination
by: Raymond T. Co, et al.
Published: (2022-09-01) -
Detecting Primordial Gravitational Waves: a forecast study on optimizing frequency distribution of next generation ground-based CMB telescope
by: Deliang Wu, et al.
Published: (2020-02-01)