Showing posts with label dark matter. Show all posts
Showing posts with label dark matter. Show all posts

Sunday, March 15, 2009

Future of physics

The future of physics and cosmology was discussed at length at a recent conference held by the foundational physics research institute FQXi, particularly considering what may be ultimately possible and impossible for physics.

Theoretical physics has been progressing in many areas but there is still a strong need for observational evidence and/or alternative theories to support or disprove the existing ones. Luckily, much anticipated experimental evidence may be available in the next few years from the Large Hadron Collider (LHC), Planck Satellite, Pierre Auger Observatory and other observational astrophysics projects. For example, the Planck Satellite aims to look farther back in time than has been seen so far with the Cosmic Background Explorer (COBE), earlier than the 400,000 year old universe. It is theorized that B-modes, primordial gravitational waves from inflation, may be visible in the very early universe, which would provide additional proof of the inflationary phase occurring directly after the big bang.

Composition of dark energy to be known soon?
Another specific example for which observational evidence may be obtained in the next few years is regarding the composition of dark energy, whether it is vacuum energy made up of axion particles as one multiverse theory predicts or quintessence made up of supersymmetric WIMPs.

Many outstanding physics questions
Some other key issues are how our universe was created in the first place (a quantum theory of creation), proof for multiverse theories and possibly detecting bubble universe collisions, more about post-big bang inflation, why there is so much more antimatter than matter (the antimatter problem), why the weak force is 1032 times stronger than gravity (vs. say a more acceptable 3-4 orders of magnitude; the hierarchy problem), the existence, size and parameters of any additional dimensions of space, not to mention the usual unification of general relativity and quantum mechanics in a quantum theory of gravity, and finally the vexing Boltzmann brain problem, that consciousness could potentially arise from nothing but quantum fluctuations.

Next-gen astrophysics tools critical
Much progress has been made with accelerators, space-based telescopes, terrestrial array telescopes, and adaptive optics but the next era of astrophysics tools could be even more revolutionary. Accelerators are an expensive $5 billion or more and take years if not decades for fundraising, permitting, building and rendering operational. One alternative could be different kinds of accelerators which are smaller, quicker and cheaper to build, notably plasma wakefield accelerators, laser accelerators, and benchtop accelerators. Another way for tools to evolve could be with computational astrophysics and simulations such as MICA's Newtonian N-body simulation (featured by UgoTrade). As computing power continues to grow, accelerator and telescope datasets could be the inputs to large-scale simulation, prediction and test. As nearly every other science has moved into informatics and rigorous math-based prediction, simulation and experimentation, so too could astrophysics, fostering much quicker cycles and a tighter linkage between theoretical and experimental physics.

The FQXi community
Curiosity-driven physics researchers, especially those investigating risky areas on the boundaries of institutional acceptance are encouraged to apply for FQXi grants, and those understanding the value of fundamental physics research funding are encouraged to participate as donors and in the FQXi website community.

NOTE: The author is an advisor to FQXi.

Sunday, January 16, 2005

How Long is a Long Time?

Time is of course subjective, it flows fast when you are having a good time and slow when you are waiting for something or having a not so good time. But what is a really long time? We are starting to put some long time frame events in a definitive timetable.

One long-term way of thinking is in terms of Russian astronomer Kardashev's Type I, II & II societies. Type I societies have fully harnessed all forms of their planetary energy including volcanoes, earthquakes, weather, hydrothermal vents, etc. We are currently a Type 0.7 society. Michio Kaku, talking about his new book, Parallel Worlds, thinks we are about 100 years from becoming a Type I society, as compared with Freeman Dyson suggesting a few years ago that we are 200 years away. No doubt the 2004 tsunami may help hasten the speed to a Type I society.

Other long-dated events on the horizon include:
-5 billion years to the engulfment of Earth by the sun
-10 billion years to the Andromeda galaxy collision w/ the Milky Way
-x billion/trillion+(?) years to the heat death of the universe when the accelerated expansion of the universe has driven all of the heat out

These events imply that human intelligence must take action to survive, first to get off Earth, then to get out of the galaxy and finally to get out of this universe. Or we could learn to control these events or manage around them such as by learning to live without heat/make heat unconventionally w/ dark matter/energy, better understand and manipulate physics, etc.

It seems likely that science will lead us to achieve these survival outcomes as a byproduct of other goals and imperatives occurring first.

One or more singularities may also supersede the timetable.