NEWSALERT: Saturday, December 13, 2003 @ 2327 GMT --------------------------------------------------------------------- The latest news from Astronomy Now and Spaceflight Now
HAS XMM-NEWTON CAST DOUBT OVER DARK ENERGY? ------------------------------------------- In a survey of distant clusters of galaxies, European Space Agency's XMM-Newton observatory has found puzzling differences between today's clusters of galaxies and those present in the Universe around seven thousand million years ago.
Alain Blanchard of the Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrenees and his team use the results to calculate how the abundance of galaxy clusters changes with time. Blanchard, knowing that this conclusion will be highly controversial, said: "To account for these results you have to have a lot of matter in the Universe and that leaves little room for dark energy."
http://spaceflightnow.com/news/n0312/12darkenergy/
[...]
----- End of forwarded message from NewsAlert -----
witam,
So Burbidge/Hoyle/Narlikar "Reloaded" have got some media coverage. Fine.
"Omega_matter = 1 (was Re: gas question)" http://www.astro.uni.torun.pl/sympa/shape-univ/2003-11/msg00005.html
The article by Blanchard et al: http://arxiv.org/abs/astro-ph/0311381
Look carefully at the figures. The triple-dotted-dashed line is the model for an (Om_m=0.3, Om_Lambda=0.7). It's hard to find, but once you find it, you'll see it matches the observations very, very nicely.
According to the authors, this triple-dotted-dashed line is for eq.~(6), which replaces eq.~(2). The difference between the dtwo eqns is a factor of (1+z).
The authors' derivation of eq.~(2), in other papers, obtains this (1+z) factor from the density of the Universe at the time that the cluster virialises. So unless you throw out rho = rho_0 (1+z)^3 , it's hard to change the derivation.
However, if you just look at another derivation of the equivalent of eq.~(2), i.e. a T-M relation, and look at the z evolution of, e.g. equation (73) of
Niayesh Afshordi, Renyue Cen http://arxiv.org/abs/astro-ph/0105020
then the (1+z) factor becomes essentially (1+ not much) over the relevant redshift range.
In other words, Blanchard et al's figures, with Afshordi & Cen's version of the T-M relation, give the concordance model.
Again in simpler words, Blanchard et al think that clusters form in one way, Afshordi & Cen think they form in a somewhat different way, leading to moderately different T-M relations and hence totally different local curvature parameter inferences.
It's good to have dissidents around :). Sometimes they're right, sometimes they're wrong.
pozd boud
On Tue, 16 Dec 2003, Andrzej Marecki wrote:
NEWSALERT: Saturday, December 13, 2003 @ 2327 GMT
The latest news from Astronomy Now and Spaceflight Now
HAS XMM-NEWTON CAST DOUBT OVER DARK ENERGY?
In a survey of distant clusters of galaxies, European Space Agency's XMM-Newton observatory has found puzzling differences between today's clusters of galaxies and those present in the Universe around seven thousand million years ago.
Alain Blanchard of the Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrenees and his team use the results to calculate how the abundance of galaxy clusters changes with time. Blanchard, knowing that this conclusion will be highly controversial, said: "To account for these results you have to have a lot of matter in the Universe and that leaves little room for dark energy."
http://spaceflightnow.com/news/n0312/12darkenergy/
[...]
----- End of forwarded message from NewsAlert -----
-- Andrzej
BTW, this stuff is highly important for OCRA analyses - whichever way it works out. We'll (hopefully) have lots of clusters and maybe we'll use cosmology to understand cluster physics rather than the other way around, but either way, getting all the bits of the puzzle to be consistent is the challenge.
BTW(2) - Motyl proposes that we work on the grant proposal tomorrow afternoon (Wed 17 Dec) @radio astronomy.
pozd boud
On Tue, 16 Dec 2003, Boud Roukema wrote:
Niayesh Afshordi, Renyue Cen http://arxiv.org/abs/astro-ph/0105020
then the (1+z) factor becomes essentially (1+ not much) over the relevant redshift range.
In other words, Blanchard et al's figures, with Afshordi & Cen's version of the T-M relation, give the concordance model.
Again in simpler words, Blanchard et al think that clusters form in one way, Afshordi & Cen think they form in a somewhat different way, leading to moderately different T-M relations and hence totally different local curvature parameter inferences.
witam, We just had a long discussion regarding possibilities for the next grant proposal. Here is what i remember and understood in the discussion.
* We haven't yet got a reply from Sebastian.
* It's not obvious how easy or wise it would be to include Jarek, given that: OCRA has its own funding, so including stuff relevant to OCRA might be used as an argument against the grant proposal; and Jarek is not yet a PhD student, and has not yet decided to do a PhD in Torun, or decided between TCfA and CAMK.
* In both cases, there are still a few weeks for discussion (but not much more).
* From our previous proposal:
http://www.astro.uni.torun.pl/sympa/cosmo-torun/2003-01/thrd1.html http://www.astro.uni.torun.pl/sympa/cosmo-torun/2003-02/thrd1.html
we had one referee very positive, two quite negative. One of the negatively commenting referees failed to understand how AGNs can be used to test topology, but the other simply felt that AGNs and topology are separate fields and should not be combined.
* The AGN evolution observations of motyl + magda + andrzej together make a very tight knit project and would be self-sufficient for a grant proposal alone.
* It is important to maximise the chances of the grant proposal being accepted in order to get the money.
* There was consensus that
(1) We should have AGN observations as the main focus of the proposal (not topology).
(2) That given (1), andrzej should be PI since he is much, much, much more experienced in AGN observations than boud.
(3) We still have some time (e.g. till 7 Jan) to decide further basic questions before getting heavily into the paperwork, printing, signing, etc.
* The two most likely scenarios are:
(4) (4a) andrzej + magda + motyl -> theme = AGN observations - birth/death/HYMORs AND [(4b) boud + bartek either (4b.1) make an independent grant proposal on another theme at the same time OR (4b.2) wait till the following grant period (Jul 2004) to avoid the chance of the grant committee creating bad feeling by giving a grant to one "group" (or neither) and not the other. ]
OR
(5) andrzej + magda + motyl + boud + bartek -> theme = AGN observations - birth/death/HYMORs - plus theoretical tools to use these to test AGN evolution hypotheses in terms of a cosmologically realistic galaxy evolution model, including sensitivity to different hypotheses on how the non-baryonic dark matter particles behave:
general discussion (please modify, correct, add links): http://adjani.astro.uni.torun.pl/cgi-bin/twiki/view/Cosmo/GalaxyAGNFormation
ArFus GPL software package: http://adjani.astro.uni.torun.pl/cgi-bin/twiki/view/Cosmo/ArFus
i personally think the idea of us "competing" against each other for basic research funding is ridiculous. The history of science constantly shows that it's only a long term point of view (50 years or so) which can seriously judge which science is best or most relevant, and even this generally oversimplifies the fact that most of science is integrated and that both the independent cross-checking by many scientists, not just by "superior" scientists, and also the high profile, "breakthroughs", are just as important for science as a whole to progress.
In any case, competition became impractical with special relativity and the atom bomb.
See also: http://en2.wikipedia.org/wiki/Game_theory http://en.wikipedia.org/wiki/Prisoner%27s_dilemma
However, for the moment the Polish astro community, and the Polish research community in general, is not well enough organised (nor would have a common point of view) to shift the grant system to something more intelligent and cooperative.
So we need to make a decision by early/mid January.
My feeling is that we have a good chance of coming to a decision by "formal consensus" on the above proposals (4) and (5) (or modified versions of them) at another meeting during early/mid January.
This means something like: - we are clear on what the different proposals are (see above) - any of us (whether mgr or dr or nearly-hab ;) can *block* any of the proposals, but can only do so on the basis of what she/he thinks is a fundamental reason (e.g. science and/or money), not based on (e.g.) seniority or some unstated intuition
("formal" doesn't mean bureaucratic, it means that we are clear about what we are saying and how we decide)
i personally don't have objections to any of the options, except that i might block (4b.1) unless people think that there would be a good chance of two "competing" proposals being simultaneously accepted.
pozd boud
PS: please corrrect, comment, whatever.
On Tue, 16 Dec 2003, Andrzej Marecki wrote:
BTW(2) - Motyl proposes that we work on the grant proposal tomorrow afternoon (Wed 17 Dec) @radio astronomy.
Let's say at 13:00. Is that OK for everyone?
A.