- #1
Sundance
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G'day from the land of ozzzzz
Is the universe Expanding or accelerating?
Is the Universe Contracting or deccelerating?
Simple observation of how the parts within the universe work gives us an idea.
Also a few scientific papers add weight.
http://arxiv.org/abs/astro-ph/0408383
The Fueling and Evolution of AGN: Internal and External Triggers
Authors: Shardha Jogee (Space Telescope Science Institute)
(Submitted on 20 Aug 2004 (v1), last revised 10 Jul 2008 (this version, v2))
and
http://arxiv.org/abs/0809.0537
[0809.0537] Cosmographic Hubble fits to the supernova data
Cosmographic Hubble fits to the supernova data
Authors: Celine Cattoen (Victoria University of Wellington), Matt Visser (Victoria University of Wellington)
(Submitted on 3 Sep 2008)
Is the universe Expanding or accelerating?
Is the Universe Contracting or deccelerating?
Simple observation of how the parts within the universe work gives us an idea.
Also a few scientific papers add weight.
http://arxiv.org/abs/astro-ph/0408383
The Fueling and Evolution of AGN: Internal and External Triggers
Authors: Shardha Jogee (Space Telescope Science Institute)
(Submitted on 20 Aug 2004 (v1), last revised 10 Jul 2008 (this version, v2))
Abstract: In this chapter, I review the fueling and evolution of active galactic nuclei (AGN) under the influence of internal and external triggers, namely intrinsic properties of host galaxies (morphological or Hubble type, color, presence of bars and other non-axisymmetric features, etc) and external factors such as environment and interactions. The most daunting challenge in fueling AGN is arguably the angular momentum problem as even matter located at a radius of a few hundred pc must lose more than 99.99 % of its specific angular momentum before it is fit for consumption by a BH. I review mass accretion rates, angular momentum requirements, the effectiveness of different fueling mechanisms, and the growth and mass density of black BHs at different epochs. I discuss connections between the nuclear and larger-scale properties of AGN, both locally and at intermediate redshifts, outlining some recent results from the GEMS and GOODS HST surveys.
and
http://arxiv.org/abs/0809.0537
[0809.0537] Cosmographic Hubble fits to the supernova data
Cosmographic Hubble fits to the supernova data
Authors: Celine Cattoen (Victoria University of Wellington), Matt Visser (Victoria University of Wellington)
(Submitted on 3 Sep 2008)
Abstract: The Hubble relation between distance and redshift is a purely cosmographic relation that depends only on the symmetries of a FLRW spacetime, but does not intrinsically make any dynamical assumptions. This suggests that it should be possible to estimate the parameters defining the Hubble relation without making any dynamical assumptions. To test this idea, we perform a number of inter-related cosmographic fits to the legacy05 and gold06 supernova datasets. Based on this supernova data, the "preponderance of evidence" certainly suggests an accelerating universe. However we would argue that (unless one uses additional dynamical and observational information) this conclusion is not currently supported "beyond reasonable doubt". As part of the analysis we develop two particularly transparent graphical representations of the redshift-distance relation -- representations in which acceleration versus deceleration reduces to the question of whether the relevant graph slopes up or down. Turning to the details of the cosmographic fits, three issues in particular concern us: First, the fitted value for the deceleration parameter changes significantly depending on whether one performs a chi^2 fit to the luminosity distance, proper motion distance or other suitable distance surrogate. Second, the fitted value for the deceleration parameter changes significantly depending on whether one uses the traditional redshift variable z, or what we shall argue is on theoretical grounds an improved parameterization y=z/(1+z). Third, the published estimates for systematic uncertainties are sufficiently large that they certainly impact on, and to a large extent undermine, the usual purely statistical tests of significance. We conclude that the supernova data should be treated with some caution.