In physical cosmology, astronomy and celestial mechanics, dark energy is a hypothetical form of energy that permeates all of space and tends to increase the rate of expansion of the universe.[1] Dark energy is the most accepted theory to explain recent observations that the universe appears to be expanding at an accelerating rate. In the standard model of cosmology, dark energy currently accounts for 73% of the total mass-energy of the universe.[2] , 8 -21 new forms may be added, as is the case with dark energy, a hypothetical form of energy that permeates all of space and tends to increase the rate of expansion of the universe. http://en.wikipedia.org/wiki... , 11 -29 -12 http://en.wikipedia.org/wiki... - Thomas Page

Alpha Magnetic Spectrometer http://en.wikipedia.org/wiki... First Results On 30 March 2013 the first results from the AMS experiment were announced by the CERN press office , 4 -6 http://friendfeed.com/citizen... , [ unrelated 4 -13 dark lightning ?http://www.popsci.com/science... sort 11 -10 Interstellar_(film) http://en.wikipedia.org/wiki... - Thomas Page

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Breakthrough_of_the_Year http://en.wikipedia.org/wiki... - Thomas Page

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1 -3 http://ngm.nationalgeographic.com/2015... - Thomas Page

Wormhole http://en.wikipedia.org/wiki... 11 -26 Blackholes http://en.wikipedia.org/wiki... How seeing a black hole’s shadow will tell us if Einstein was right http://www.pbs.org/newshou... [[ The Event Horizon Telescope is a project to create a telescope array combining data from VLBI stations around the Earth to observe the immediate environment of the Milky Way's supermassive black hole Sagittarius A* http://en.wikipedia.org/wiki... with angular resolution http://en.wikipedia.org/wiki... comparable to the event horizon http://en.wikipedia.org/wiki... . The group proposes till 2022 to combine existing and planned millimeter/submillimeter facilities into a high-sensitivity, high angular resolution Event Horizon Telescope. The effort will include development and deployment of submillimeter dual polarization receivers, highly stable frequency standards to enable VLBI at 230–450 GHz, higher-bandwidth VLBI backends and recorders, as well as commissioning of new submillimeter VLBI sites. [[[[ sort http://en.wikipedia.org/wiki... http://wiki.lmtgtm.org/instrum... sort sort to http://en.wikipedia.org/wiki... 11 -27 http://en.wikipedia.org/wiki... 12 -8 http://blogs.scientificamerican.com/observa... 2 -15 http://www.sciencedaily.com/release... - Thomas Page