Distortions in the surface of last scattering
- 1. Carnegie Mellon University, Pittsburgh, PA (United States)
- 2. University of Chicago, IL (United States). Enrico Fermi Institute, Kavli Institute for Cosmological Physics
Description
The surface of last scattering of the photons in the cosmic microwave background is not a spherical shell. Apart from its finite width, each photon experiences a different gravitational potential along its journey to us, leading to different travel times in different directions. Since all photons were released at the same cosmic time, the photons with longer travel times started farther away from us than those with shorter times. Thus, the surface of last scattering is corrugated, a deformed spherical shell. We present an estimator quadratic in the temperature and polarization fields that could provide a map of the time delays as a function of position on the sky. The signal to noise of this map could exceed unity for the dipole, thereby providing a rare insight into the universe on the largest observable scales.
Availability note (English)
Available from https://www.osti.gov/servlets/purl/1595730; https://www.osti.gov/biblio/1595730; DOE Accepted Manuscript full text, or the publishers Best Available Version will be available free of charge after the embargo periodAdditional details
Identifiers
Publishing Information
- Journal Title
- Physical Review D
- Journal Volume
- 100
- Journal Issue
- 4
- Journal Page Range
- vp.
- ISSN
- 2470-0010
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 54046435
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- COSMIC PHOTONS; MICROWAVE RADIATION; SCATTERING; SPHERICAL CONFIGURATION; SURFACES
- Descriptors DEC
- BOSONS; CONFIGURATION; COSMIC RADIATION; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; IONIZING RADIATIONS; MASSLESS PARTICLES; PHOTONS; RADIATIONS
Optional Information
- Contract/Grant/Project number
- SC0009924; SC0019248; SC0010118
- Funding organization
- USDOE Office of Science - SC, High Energy Physics (HEP) (United States); National Aeronautics and Space Administration (NASA) (United States); Simons Foundation (United States)
- Secondary number(s)
- OSTIID--1595730