Witam,
http://cosmo.torun.pl/GPLdownload/dodec/circles-0.1.17.tar.gz
jest przygotowy.
Mo�esz u�ywa� opcja -D �eby produkowa� wykresy i wtedy najintersuj�ce s�
gs s_rot_*[tf].ps
Pokazuj� S i \sigma dla rozwi�zanie w astro-ph/0402608, oko�o tych 6 okr�gi, ale zamiast tylko fazy -36.0 deg, 0.0 deg i +36.0 deg, jest dla
-36.0 deg + beta
gdzie beta jest faza miedzy 0 i 360 deg. Je�li hypoteza jest dobra, musi by� maksimum S na 0 i minimum \sigma na 0 deg. Wydaje mi si� �e jest to prawda: maks S i min \sigma s� na 0 deg. Oczywi�cie, to nie *wystarczy* pokazywa� �e hypoteza jest dobra, ale najmniej jest to sp�jny.
s_rot_stat.ps -> S s_rot_diff.ps -> \sigma
BTW, tu jest program warsztatu w Pary�u - Bartek i ja b�dziemy tam.
pozdr boud
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Workshop "Cosmic Topology between WMAP and PLANCK : Facts and Theories" Observatoire de Paris-Meudon, CIAS 8-10 march 2005
Preliminary Program
Tuesday 8 March : Topology and CMB
10.00 - J.-P. Luminet : Opening address - Cosmic topology, New Challenges
10.45 - Coffee break
11.00 - G. Starkman : Looking for the topology=20 of the universe using circles in the sky
11.45 - B. Roukema : The Poincar=E9 dodecahedral=20 manifold and matched circles in the first-year=20 WMAP ILC data
12.30 - Discussion and Lunch
14.30 - S. Lustig: CMB Anisotropy of Spherical Spaces
15.15 - A. Riazuelo : The State-of-the-Art of CMB=20 simulations in multiconnected spaces.
16.00 - Coffee Break
16.15 - F. Steiner: CMB Anisotropy of Hyperbolic Spaces
17.00 - General Discussion
Wednesday 9 March. Mathematical Methods for Multiconnected Spaces.
10.00 - J. Weeks : Mathematics of Multipoles - Ideas New and Old
10.45 - Coffee break
11.00 - M. Lachieze-Rey : A few remarks on Multipole Vectors
11.45 - J . Gundermann : Eigenmodes in spherical=20 spaces, the case of S3, S3/I*, S3/T* and S3/O*.
12.30 - Discussion and Lunch
14.30 - M. Lachieze-Rey : Mathematical methods=20 for eigenmodes in spherical spaces
15.15 - S. Caillerie : Computation of eigenmodes=20 in Spherical Dodecahedral Space
16.00 - Coffee Break and Discussion
Thursday 10 March. Crystallography and Other Methods. Open Discussion.
10.00 - M. Reboucas : title to come
10.45 - Coffee break
11.00 - G. Starkman : The statistical isotropy=20 of the microwave background, or is the low-l=20 microwave background really cosmic?
11.45 - B. Lew : Tests of non-gaussian features=20 of CMBR in WMAP map as hints for non trivial=20 topology
12.30 - Discussion and Lunch
14.30 - B. Roukema : Cosmic crystallography using=20 short-lived objects - active galactic nuclei
15.15 - A. Riazuelo : CMB Polarization in multiconnected spaces.
16.00 - Final Discussion ----------------------------------------------------------------------------= ----------------------------------------------------------------------
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Boud Roukema