Universe is 13.73 Billion Years Old

The latest on the "age of the universe" thread of this blog is news from NASA that it's been estimated to be 13.73 billion years old, see WMAP Reveals Neutrinos, End of Dark Ages, First Second of Universe

"NASA released this week five years of data collected by the Wilkinson Microwave Anisotropy Probe (WMAP) that refines our understanding of the universe and its development. ... WMAP measures a remnant of the early universe - its oldest light. The conditions of the early times are imprinted on this light. It is the result of what happened earlier, and a backlight for the later development of the universe. This light lost energy as the universe expanded over 13.7 billion years, so WMAP now sees the light as microwaves. By making accurate measurements of microwave patterns, WMAP has answered many longstanding questions about the universe's age, composition and development.

Microwave light seen by WMAP from when the universe was only 380,000 years old, shows that, at the time, neutrinos made up 10% of the universe, atoms 12%, dark matter 63%, photons 15%, and dark energy was negligible. In contrast, estimates from WMAP data show the current universe consists of 4.6% percent atoms, 23% dark matter, 72% dark energy and less than 1 percent neutrinos.

WMAP cosmic microwave fluctuations over the full sky with 5-years of data. Colors [in the image] represent the tiny temperature fluctuations of the remnant glow from the infant universe: red regions are warmer and blue are cooler."

Big -- Mandelbrot Universe

Watch this fractal unfolding, and listen to it too. (It reminds me a bit of scenes near the end of 2001 A Space Odyssey.)

A Mandelbrot the size of the known universe

"An extremely deep dive into the Mandelbrot zoom. If the final frame were the size of your screen, the full set would be larger than the known universe."

There are more Mandelbrot/fractal animations on the same YouTube page. If you want to get a rigid mathematical explanation of Mandelbrot's accomplishments , be sure to listen to the following one as it unfolds:

Mandelbrot Set Zoom

Is the Universe Finite, or Not?

I've just come across a few interesting items in my quest to understand "life and the universe" and would like to share them with you:

• On A Finite Universe With No Beginning Or End (a PDF document) - by Peter Lynds of New Zealand, with the following abstract:
  
  

  "Based on the conjecture that rather than the second law of thermodynamics inevitably be breached as matter approaches a big crunch or a black hole singularity, the order of events should reverse, a model of the universe that resolves a number of longstanding problems and paradoxes in cosmology is presented. A universe that has no beginning (and no need for one), no ending, but yet is finite, is without singularities, precludes time travel, in which events are neither determined by initial or final conditions, and problems such as why the universe has a low entropy past, or conditions at the big bang appear to be so "special," require no causal explanation, is the result. This model also has some profound philosophical implications."

  If the above paper is too much for you, then from Science a Go Go there's a pair of articles that might make it more digestible: The Universe As Magic Roundabout: Part I plus The Universe As Magic Roundabout: Part II
  
  Here's an earlier paper by Peter Lynds (also a PDF document):
  Time and Classical and Quantum Mechanics: Indeterminacy vs. Discontinuity
  
  
• For another view, this time about multiple universes, there's Towards observable signatures of other bubble universes (another PDF document) with the following abstract:
  
  

  "We evaluate the possibility of observable effects arising from collisions between vacuum bubbles in a universe undergoing false-vacuum eternal inflation. Contrary to conventional wisdom, “typical” observers inside a bubble should have access to a large number of collision events. We calculate the expected number and angular size distribution of such collisions on an observer’s “sky”, finding that for typical observers the distribution is anisotropic and includes many bubbles, each of which will affect the majority of the observer’s sky. After a qualitative discussion of the physics involved in collisions between arbitrary bubbles, we evaluate the implications of our results, and outline possible observable effects. In an optimistic sense, then, the present paper constitutes a first step in an assessment of the effects of other bubble universes on the cosmic microwave background and other observables."