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String/M-Theory - Wheaton College
String/M-Theory - Wheaton College

... Some scientists (e.g. Stephen Hawking) are suspicious that determination of a particular choice of ALL of the M-Theory parameters might not be totally determinable, based on Gödel’s Theorem, which says that one cannot formulate a finite system of axioms to prove every result in mathematics. This mea ...
the first three thresholds - McGraw
the first three thresholds - McGraw

... modern big bang cosmology (the modern, scientific explanation of the origin of the universe) shares all these features. Viewed from outside, it may seem quite crazy. It also has poetic or metaphorical qualities because even modern science must sometimes use poetic language when it tries to describe ...
if on the Internet, Press  on your browser to
if on the Internet, Press on your browser to

... For the past 7 years, this German set-up has been looking for gravitational waves -- ripples in space-time thrown off by super-dense astronomical objects such as neutron stars and black holes. GEO600 has not detected any gravitational waves so far. But it might inadvertently have made the most impor ...
Unit 6: The Present Universe
Unit 6: The Present Universe

... sole purpose of which was to balance the attraction of gravity and thus allow for a static universe. Einstein made an error here. His introduced repulsive force could not properly balance gravity. The equilibrium between the two was unstable, like balancing a pencil on its point – an action that is ...
Cosmic Hide and Seek: the Search for the Missing Mass
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Chapter 6 The inflationary universe In this chapter, we encounter a
Chapter 6 The inflationary universe In this chapter, we encounter a

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dark matter. - Gordon State College
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Our Universe—Infinite and Eternal: Its Physics
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... When astronomers estimate the age of the universe, experimentally they come up with the number of about 15 billion years old. As far as we are concerned, this is an infinite amount of time by any scale. The constituents of atoms – electrons, protons, and neutrons (only inside atoms), are known to ha ...
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Beyond the Big Bang - Physics Department, Princeton University
Beyond the Big Bang - Physics Department, Princeton University

... elements — hydrogen, deuterium, helium, and lithium — in the universe today. According to the hot big bang model, these elements were created in the first few minutes after the big bang. For the first second after the bang, the temperature was so hot that even atomic nuclei could not exist. But as t ...
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Scientific Evidence for A
Scientific Evidence for A

... cattle and creeping things and beasts of the earth after their kind”; and it was so. And God made the beasts of the earth after their kind, and the cattle after their kind, and everything that creeps on the ground after its kind; and God saw that it was good. Then God said, “Let Us make man in Our i ...
Cosmological principle and the Cosmic microwave
Cosmological principle and the Cosmic microwave

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Big Bang nucleosynthesis

In physical cosmology, Big Bang nucleosynthesis (abbreviated BBN, also known as primordial nucleosynthesis) refers to the production of nuclei other than those of the lightest isotope of hydrogen (hydrogen-1, 1H, having a single proton as a nucleus) during the early phases of the universe. Primordial nucleosynthesis is believed by most cosmologists to have taken place from 10 seconds to 20 minutes after the Big Bang, and is calculated to be responsible for the formation of most of the universe's helium as the isotope helium-4 (4He), along with small amounts of the hydrogen isotope deuterium (2H or D), the helium isotope helium-3 (3He), and a very small amount of the lithium isotope lithium-7 (7Li). In addition to these stable nuclei, two unstable or radioactive isotopes were also produced: the heavy hydrogen isotope tritium (3H or T); and the beryllium isotope beryllium-7 (7Be); but these unstable isotopes later decayed into 3He and 7Li, as above.Essentially all of the elements that are heavier than lithium and beryllium were created much later, by stellar nucleosynthesis in evolving and exploding stars.
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