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This is the first newsletter of the post-CCC2
epoch, and was consequently delayed while we
attended to the conference. We have had our
hands full over the past several months! During
this time, it seems that an increasing
proportion of published papers in astrophysics
is resorting to the terms “anomalous”,
“peculiar”, “puzzling”, “problem”, and
“difficult to explain in terms of the model”. It
is also pleasing to see that some CCC2 papers
have already appeared on arXiv.
Redshift
Reference to redshift is ubiquitous in
astrophysical publications, either as a distance
indicator or measure of velocity, or both. CCC2
participant John Hartnett uses Fourier analysis
of galaxy redshifts from large surveys to reveal
an onion skin-like periodicity in number counts.
This is a novel view of redshift quantisation.
Navia, Augusto, and Tsui created a Hubble
diagram of QSOs, AGN, and GRBs which reveals
spectral variability that erodes their
usefulness as standard candles.
Title: Galaxy redshift abundance periodicity
from Fourier analysis of number counts N(z)
using SDSS and 2dF galaxy surveys.
Authors: John. G. Hartnett, Koichi Hirano.
Astro-ph/0711.4885
Title: The Hubble diagram of high redshift
objects, QSOs and AGNs.
Authors: C. E. Navia, C. R. A. Augusto, K.
H. Tsui.
Astro-ph/0807.0590
Nucleosynthesis
Lithium remains the Achilles’ heel of Big Bang
nucleosynthesis. The June newsletter referenced
papers by Burbidge, and by Frebel et al. Here we
mention two more, selected examples of numerous
studies indicating failure of the Big Bang
evolutionary scheme. Cyburt et al report a
“significant discrepancy between the primordial
7Li abundance as predicted by BBN theory and the
WMAP baryon density, and the pre-Galactic
lithium abundance inferred from the observation
of metal-poor stars.”
Title: The Puzzling origin of the 6Li
plateau.
Authors: Carmelo Evoli, Stefania Salvadori,
and Andrea Ferrara.
Astro-ph/0806.4184
Title: A Bitter Pill: The Primordial Lithium
problem.
Authors: Richard H. Cyburt, Brian D. Fields,
and Keith A. Olive.
Astro-ph/0808.2818
Expansion
At the very heart of the Standard Model of
Cosmology is the notion of expansion. Andre
Assis presented a paper at CCC2 illustrating
Edwin Hubble’s own scepticism about universal
expansion and whether his own measurements
supported the idea. Cosmic fractals pioneer
Yurij Baryshev focuses on the physics (or lack
thereof) of expanding space, pointing out the
conceptual problems that arise with the
suggestion that vacuum is continuously created.
Here he develops the theme he presented at CCC1.
Title: Hubble’s Cosmology: From a Finite
Expanding Universe to a Static Endless Universe.
Authors: A.K.T. Assis, M.C.D. Neves, and
D.S.L. Soares.
Astro-ph/0806.4481
Title: Expanding Space: The Root of
Conceptual problems of the Cosmological Physics.
Authors: Yu. V. Baryshev.
Astro-ph/0810.0153
Quasars
QSOs have proven to be enigmatic from their
discovery over 40 years ago. Two recent studies
examine QSO HI absorption along line-of-sight,
comparing foreground and background (Kirkman &
Tytler), and the time scale of QSO size
evolution (L. Fan et al) respectively.
Title: The transverse proximity effect in the
z~2 Lyman-alpha forest suggest QSO episodic
lifetimes of ~1 Myr.
Authors: David Kirkman and David Tytler.
Astro-ph/0809.2277
Title: The dramatic size evolution of
elliptical galaxies and the quasar feedback.
Authors: L. Fan, A. Lapi, G. De Zotti, and
L. Danese.
Astro-ph/0809.4574
Microwave Background
Analyses of the WMAP data continue to pour in
with the release of WMAP5. Many are finding
anomalous results. Whilst sitting fog-bound at
Port Angeles airport after CCC2, John Hartnett
raised the very interesting point that
conventional analysis holds that the radiation
picture is frozen in time. If therefore,
analysts could access the year-by-year WMAP data
separately (data are currently released
cumulatively), a telling comparison between data
sets at different times could be made. According
to the Standard Model, there should be no
differences. In these three examples,
peculiarities are found in the lack of
large-angle correlations (Copi et al),
distortions in the WMAP maps (Liu and Li), and
spatial topology (Gurzadyan et al).
Title: No large-angle correlations on the
non-Galactic microwave sky.
Authors: Craig J. Copi, Dragan Huterer,
Dominik J. Schwarz, and Glenn D. Starkman.
Astro-ph/0809.3767
Title: Statistical and systematical errors in
cosmic microwave background maps.
Authors: Hao Liu and Ti-Pei Li.
Astro-ph/0809.4493
Title: Large Scale Plane-Mirroring in the
Cosmic Microwave Background WMAP5 Maps.
Authors: V.G. Gurzadyan, A.A. Starobinsky, T.
Ghahramanyan, A.L. Kashin, H. Khachatryan, H.
Kuloghliyan, D. Vetrugno, and G. Yegorian.
Astro-ph/0807.3652
Large structure
The observed presence of large-scale structure
is an embarrassment to the LCDM model, which
relies on the Cosmological Principle for uniform
expansion. Several studies have revealed
additional features of large or supposedly
distant structures that defy standard
interpretations. Data from the GOODS NICMOS
survey (Buitrago et al) show a diminishing of
size-evolution above z = 2, and the high
densities of massive galaxies at z = 3 makes
evolution unlikely beyond that point. Another
study (Damjanov et al) supports this more
specifically, with around one third of massive
red objects (“Red Nuggets”) being
extraordinarily compact. A new Kormendy Relation
(stellar mass density vs. size) is introduced
which isolates size evolution from luminosity
and colour evolution. These results fit very
well with Arp’s intrinsic redshift, quasar
ejection model. Three further studies,
including Yurij Baryshev’s collaboration with
N.V. Nabokov, are included in this list that
investigate the implications of structure,
evolution, and velocities.
Title: Size evolution of the most massive
galaxies at 1.7<z<3 from GOODS NICMOS survey
imaging.
Authors: Fernando Buitrago et al.
Astro-ph/0807.4141
Title: Red Nuggets at z~1.5: Compact passive
galaxies and the formation of the Kormendy
relation.
Authors: Ivana Damjanov et al..
Astro-ph/0807.1744
Title: Recent Structural Evolution of
Early-Type Galaxies: Size Growth from z = 1 to z
= 0.
Authors: Arjen van der Wel et al.
Astro-ph/0808.0077
Title: A search for super-large structures in
deep galaxy surveys.
Authors: N.V. Nabokov and Yu. V. Baryshev.
Astro-ph/0809.2390
Title: A measurement of large-scale peculiar
velocities of clusters of galaxies: results and
cosmological implications.
Authors: A. Kashlinsky, F. Atrio-Barandela,
D. Kocevski, and H. Ebeling.
Astro-ph/0809.3734
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