New Frontiers in Astronomy

The New Frontiers in Astronomy and Cosmology program has
announced its Award winners!

The $4+ million in awards went to 20 scientists studying Big Questions on fundamental issues and 21 high school and university student essay prize winners.

The awards will be presented at a conference at the Franklin Institute in Philadelphia next week.

The program is funded by the Templeton Foundation as part of its celebration of the centennial of the birth of its founder, John Templeton.

The topics solicited for the Big Questions were very interesting:

  1. What was the earliest state of the universe?
    1. What are the scientific ways to test various theories of the earliest state of the universe (cosmic genesis)?
    2. What kinds of state or “laws” might have “preceded” the existence of spacetime?
    3. If space and time are not fundamental in the deepest scientific description of the universe, how did they emerge?
  2. Is our observable universe unique or is it part of a much larger multiverse?
    1. Can the ideas of multiverse be empirically tested? If so, how? If not, what is the scientific and epistemological status of those domains that cannot be observed?
    2. What are the distinguishing characteristics of multiverses that are based on different quantum cosmologies?
    3. Many multiverse models invoke the idea of infinity as part of their explanatory apparatus. Can the physical world be infinite?
  3. What is the origin of the complexity in the universe?
    1. What are the conditions for the universe to evolve to a high degree of complexity?
    2. What are the key stages of increasing complexity in the universe? How do they come about?
    3. Will the complexity of the universe continue to increase? If so, how long? Are there any theoretical limits to the complexity of the universe?
  4. Are we alone in the universe? Or, are there other life and intelligence beyond the solar system?
    1. What are the signatures of the existence of life and intelligence in the universe?
    2. Would the fine-tunings required for life in the universe also necessarily require that life be rare?
    3. To what degree are such other beings likely to be similar to humans? Are there features in nature which could limit the level of intelligence or the differences we may expect?

These awards are specifially for research on topics that is speculative and beyond the purview of funding by federal agencies.
The list of topics makes for a fascinating reading.

More like this

Yeah, fascinating, especially if you read all the way to the bottom.

The Universe, Some Updates
tags: big bang, mass energy, gravity, inflation expansion, singularity, black hole

What Big Banged To Produce The Universe
From :…
A commonsensible conjecture is that Universe Contraction is initiated following the Big-Bang event, as released moving gravitons (energy) start reconverting to mass (gravity) and eventually returning to black holes, steadily leading to the re-formation of The Universe Singularity, simultaneously with the inflation and expansion, i.e. that universal expansion and contraction are going on simultaneously.
Conjectured implications are that the Universe is a product of A Single Universal Black Hole with an extremely brief singularity of ALL the gravitons of the universe, which is feasible and possible and mandated because gravitation is a very weak force due to the small size of the gravitons, the primal mass-energy particles of the universe.
This implies also that when all the mass of the presently expanding universe is consumed by the present black holes, expansion will cease and be replaced with empansion back to THE Single Universal Black Hole.
Dov Henis (comments from 22nd century)


Universe Inflation And Expansion
Inflation on Trial
Astrophysicists interrogate one of their most successful theories…
Inflation and expansion are per Newton.
Since the Big Bang galactic clusters loose mass at constant rate. Mass, gravitons, continue escaping at constant rate from their Big Bang fragments-clusters thus becoming energy, mass in motion, thus thrusting the clusters. Constant thrust and decreasing galactic clusters weight accelerate the separation of clusters from each other.
Common sense.
Dov Henis (comments from 22nd century)

By Dov Henis (not verified) on 09 Oct 2012 #permalink