witam cosmo-torun
Cosmo workshop
WHEN: Fri 15:00 12.03.2010
WHO: boud
TITLE: Liu and Li arXiv:1003.1073 ("The origin of the WMAP quadrupole")
ABSTRACT: The WMAP quadrupole is apparently
mostly a pointing error. The true quadrupole is much
closer to zero. The missing fluctuations problem has
just got much worse for the infinite-flat-universe hypothesis.
Liu and Li arXiv:1003.1073 ("The origin of the WMAP quadrupole") have
posted a very interesting article (presumably submitted to Nature,
guessing from the style and length). The best estimate of the CMB
quadrupole is apparently... zero!
They claim that the WMAP quadrupole comes from a single error - an
antenna direction representation error by half of an observational
angular interval. The discussion concerns quaternions, but don't
be frightened - it presumably uses the imaginary part only, to
represent X, Y, Z directions. You can think of them as vectors
in R^3 if you like.
Order of magnitude check of their calculation:
Liu and Li say that the error is by 7' and that this causes
incorrect subtraction of the dipole in the time-ordered-date (TOD).
The direction of the error varies as the direction of observation
varies, so it's reasonable that it doesn't give a simple offset
detectable by post-processing in the analysis pipeline, IMHO
(though Bartek may have another opinion).
The dipole is about 3.3mK (e.g. section 7 Bennett et al 2003).
sin(7') * 3.3mK = 0.002 * 3.3mK = 6.7 microK
Liu and Li say 10-20 microK, just slightly higher, but their Eq.(1)
is a motivational equation - it is not used as an entry to
their data analysis pipeline.
Figures 1 and 2 should the effect very dramatically. Rephrasing what
they've said:
Figure 1 left: difference between Liu Li analysis, using the same wrong
method that the WMAP team used. This is a check that their pipeline
does the same thing that the WMAP team does. |Difference| < 2 or so microK.
Figure 1 right: Liu Li using correct antenna directions on WMAP Q1 3yr data.
They get a strong quadrupole!
Figure 2 left: The effect of using a wrong dipole, calculated using *only the
directional information* from the time-ordered-data from the spacecraft,
with *no CMB data*. See paragraph 2, page 4: "only the spacecraft attitude
information is used to compute d' ."
Figure 2 right: official WMAP5 V+W quadrupole.
Figures 1 right, and 2 left look very, very similar to Figure 2 right.
There seems to be a slight difference in angular position visible by eye,
but the coincidence is striking.
Can we really believe that the CMB quadrupole just by chance happens to be very
strongly aligned with and of nearly identical amplitude to a map made
using only the time-ordered-data of the spacecraft direction
("attitude") and the spacecraft orbit around the Sun, and the Sun's
motion with respect to the CMB?
Since this is a Nature-type article, the authors are forced to exclude almost
all interesting details from the article, but info like the spacecraft
attitude quaternions and interpolation method should not be too difficult to
find.
* Bennett et al 2003: arXiv:astro-ph/0302207
http://arXiv.org/abs/astro-ph/0302207
* Liu, Li 2010: arXiv:1003.1073
http://arXiv.org/abs/1003.1073
The good thing about this is that it shows that a lot of very
intelligent people - those in a mega-collaboration plus many outside
of the official group - can spend 7 years looking closely at an
important set of observational data without finding what appears to be
a very elementary error in the analysis details, with a very
fundamental consequence.
The fundamental consequence is that a lower quadrupole makes Infeld's
(1949) prediction of the equivalent of the low l cutoff due to the
shape of the Universe even stronger! Liu & Li suggest an inflationary
argument, but their interpretation is not what is important - they
don't want the referee to make a fuss about interpretations, since
their observational argument is so strong.
pozdr
boud
witam cosmo-torun
Our colleagues in the optical group have got together
with some galaxy formation people and are organising a simulation
workshop this northern summer (July 2010):
http://supercomputing.astri.umk.pl/
Ben Moore is one of the key people doing galaxy simulational work
since a long time ago. Romain Teyssier does adaptive tree code
work AFAIK - his program RAMSES is here:
http://irfu.cea.fr/Projets/Site_ramses/RAMSES.html
It is wolne oprogramowanie, under the CECILL licence, which is
GPL-compatible under section 5.3.4 of the CECILL licence:
http://www.cecill.info/licences/Licence_CeCILL_V2-fr.txt
i think that many of us could be interested in participating or at
least listening to a few talks. i'm sure that Michal Hanasz and the
doktoranci will tell us if they prefer us to formally register or not,
though of course, i'm sure there wouldn't be things like registration
fees for local participants. We should think of organisers' practical
side of making sure that there are enough seats or computers
available, etc. but i don't expect that that would be a huge problem -
e.g. eduroam access for laptops should presumably be available at the
Maths building.
pozdr
boud
hi Karolina,
Here are two books that would be useful to buy. The first one has what
seems to be the first statement of the "nothing-can-be-bigger-than-the-Universe"
argument in terms of density perturbations. Apparently, the first
scientist(s) to state the argument were not Starobinsky (1993) and
Stevens et al (1993), but rather... a Polish physicist: Leopold Infeld in 1949!
The second book synthesises recent papers on the Einstein-equation exact-solution
approach to what i have repeatedly said in our cosmology group several
times (and Helena is working on this :). In simple words: "the simplest explanation
for dark energy may be the failure to do the maths carefully enough".
(1) Albert Einstein: philosopher-scientist, edited by Paul Arthur Schilpp , 1949
(republished 1970) e.g.
http://searchworks.stanford.edu/view/1066168http://www.questia.com/library/book/albert-einstein-philosopher-scientist-b…
(2) Bolejko et al 2009:
Title: Structures in the Universe by Exact Methods
Author: Krzysztof Bolejko, Andrzej Krasinski, Charles Hellaby, Marie-Noelle Celerier
ISBN: 9780521769143
http://assets.cambridge.org/assets/bookpageresult.jsf?conversationId=1165892
The first book is apparently cheap, the second one expensive. Both would be useful IMHO.
pozdr
boud