I can do a bit of Eric's job for him again. I know a bit about the CMB alignments. There's a survey of them here (including things I've heard of and things new to me.)
http://arxiv.org/abs/1510.07929
(Note that the paper includes an overview, which I encourage Lerner not to skip, of the many, many CMB statistics that have *tested and confirmed* LCDM predictions.) But it's true: among the hundreds of aspects of the CMB that precisely match the basic LCDM hypothesis, there are a few that appear somewhat unlikely (at the 2% to 0.1% level) to have arisen in a random sampling of LCDM primordial fluctuations. The paper overviews ideas for new hypotheses where the initial conditions are different.
Note that non-LCDM cosmologies (plasma, steady-state, etc.) have not yet come up with a proposal in which a roughly uniform blackbody background exists at all, much less one where this background has isentropic fluctuations at the 10^-5 level, much less one where the fluctuation angular power shows a damped acoustic-wave-like spectrum, much less etc. etc. etc..
Some of the authors of the above are also on this paper:
http://arxiv.org/abs/1512.05356
which is like the bizarro-world version of the Crisis In Cosmology Conference---this is what it sounds like when people who actually understand LCDM look for opportunities to break it. Interesting reading.
http://arxiv.org/abs/1510.07929
(Note that the paper includes an overview, which I encourage Lerner not to skip, of the many, many CMB statistics that have *tested and confirmed* LCDM predictions.) But it's true: among the hundreds of aspects of the CMB that precisely match the basic LCDM hypothesis, there are a few that appear somewhat unlikely (at the 2% to 0.1% level) to have arisen in a random sampling of LCDM primordial fluctuations. The paper overviews ideas for new hypotheses where the initial conditions are different.
Note that non-LCDM cosmologies (plasma, steady-state, etc.) have not yet come up with a proposal in which a roughly uniform blackbody background exists at all, much less one where this background has isentropic fluctuations at the 10^-5 level, much less one where the fluctuation angular power shows a damped acoustic-wave-like spectrum, much less etc. etc. etc..
Some of the authors of the above are also on this paper:
http://arxiv.org/abs/1512.05356
which is like the bizarro-world version of the Crisis In Cosmology Conference---this is what it sounds like when people who actually understand LCDM look for opportunities to break it. Interesting reading.
