imaged.
Supermassive Blackhole Eats Light
Dark Matter punches massive holes through trails of stars.
A
dark matter galaxy?
Gravitational Waves
:Read about the detection of gravitational waves by LIGO.
Visit the CERN website for inofmration on the
Discovery of the Higgs Boson.
Science Daily reports on the
LUX experiment which will search for Dark Matter.
Science Daily reports on using gravitational
lensing to detect the most
Distant Galaxy.
The CERN Courier   
The history of QCD
is a nice article in the October 2012 edition of this magazine from CERN.
Particle Physics and Cosmology   
Want to learn about the Higgs Boson? Check out The Infinity Puzzle by Frank
Close. Information can be found on the book's
website.
There is also a higher-level article written by a member of the CERN teams that
discovered the Higgs that can be found on the physics preprint server.
Particle Physics and Cosmology   
Check out The New Cosmic Onion: Quarks and the Nature of the Universe
by Frank Close. It is in the
CMU library and can be purchased from
Amazon.com.
The Search for QCD Exotics   
Read the following
article in
American Scientist. You can learn more about the Gluonic
Excitations experiment at
www.gluex.org. This experiment will be performed at the Thomas Jefferson
National Accelerator Laboratory
JLab in Newport News, Virgina.
LIGO   
How do you measure gravitational waves? Take a look at the LIGO experiment.
Additional information on this experiment can be found at their web site
at www.ligo.org. There
is also a very informative site on what they are doing and what they
hope to measure at
UIUC. This latter site is VERY INTERESTING READING.
The Law of Gravitation   
The inverse square law for gravity is an empirical result. Well, just how
good is it? The Nuclear Physics group at the University of Washington
(Seattle) is exploring just this question. Visit their website at
www.npl.washington.edu/eotwash to learn more about this.
Dark Matter   
We believe that most of the matter in the universe is dark, i.e. cannot be detected
from the light which it emits (or fails to emit). This is "stuff" which cannot be seen
directly -- so what makes us think that it exists at all? Its presence is inferred
indirectly from the motions of astronomical objects, specifically stellar, galactic, and
galaxy cluster/supercluster observations. It is also required in order to enable gravity to
amplify the small fluctuations in the Cosmic Microwave Background enough to form the
large-scale structures that we see in the universe today. See
http://cdms.berkely.edu and
http://wmap.gsfc.nasa.gov for more information.
The Universie, Big and Small
How small is small? How big is big? Check out this interactive web
application that
goes from the smallest distance scales to the largest.