Efficient Computation of CMB anisotropies in closed FRW models

Details Efficient Computation of CMB anisotropies in closed FRW models Efficient Computation of CMB anisotropies in closed FRW models

1999-11-10

arxiv.org/abs/astro-ph/9911177v2

Astrophys.J.538:473-476,2000

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure. Corrected/updated references. Accepted by ApJ. For the F90 source code see http://www.mrao.cam.ac.uk/~aml10

Scientific paper

10.1086/309179

We implement the efficient line of sight method to calculate the anisotropy
and polarization of the cosmic microwave background for scalar and tensor modes
in almost-Friedmann-Robertson-Walker models with positive spatial curvature. We
present new results for the polarization power spectra in such models.

Affiliated with

Also associated with

No associations

Rating

Efficient Computation of CMB anisotropies in closed FRW models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Efficient Computation of CMB anisotropies in closed FRW models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Efficient Computation of CMB anisotropies in closed FRW models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-495844