Heat energy photons at high temperature are highly unstable and cannot remain in that state for long time. They combine with gravitational field (at a specific range of temperature) or gravitons to acquire a lower state of energy level. This ...Cosmic Microwave Background
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* 2011 – The BICEP2 telescope will measure B-mode polarization. Adapted from the Wikipedia article Timeline of cosmic microwave background astronomy, under the G. N. U. Free Documentation License. Please also see http://en.wikipedia.org/wiki
Timeline of cosmic microwave background astronomy Adapted from the Wikipedia article Timeline of cosmic microwave background astronomy, under the G. N. U. Free Documentation License. Please also see http://en.wikipedia.org/wiki
* 1896 – Charles Edouard Guillaume estimates the “radiation of the stars” to be 5.6K. * 1926 – Sir Arthur Eddington estimates the non-thermal radiation of starlight in the galaxy “.. by the formula E = σT4 the effective temperature ...
* 1946 – George Gamow calculates a temperature of 50& K (assuming a 3-billion year old Universe), commenting it “.. is in reasonable agreement with the actual temperature of interstellar space”, but does not mention background radiation. * 1948 – ...
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