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Big Bang - schoolphysics
Big Bang - schoolphysics

... time and space began at that moment. Before the Big Bang there was no space or time – a very difficult idea to grasp. Anyway we do have some idea of what happened after the Big Bang. The temperature in that explosion was unbelievably large – astrophysicists think it may have been as high as 1000 mil ...
dark matter - Aurora City Schools
dark matter - Aurora City Schools

... microwave radiation all throughout the universe, but couldn’t explain where it came from • Only possible source is it’s left over from Big Bang • Later shown not to be “evenly spread” ...
6 Big Bang Nucleosynthesis - Course Pages of Physics Department
6 Big Bang Nucleosynthesis - Course Pages of Physics Department

... occurs at a higher temperature T4 ∼ 0.3 MeV. But we noted earlier that only deuterium stays close to its equilibrium abundance once it gets large. Helium begins to form only when there is sufficient deuterium available, in practice slightly above Td . Helium forms then rapidly. The available number ...
Cosmology and Astrophysics II
Cosmology and Astrophysics II

... duration and space. . . In him are all things contained and moved; yet neither affects the other: God suffers nothing from the motion of bodies; bodies find no resistance from the omnipresence of God. . . As a blind man has no idea of colors so we have no idea of the manner by which the all-wise God ...
The Origins of Physics, Chemistry, and Biology, or Big Bang is the
The Origins of Physics, Chemistry, and Biology, or Big Bang is the

... and antimatter was the cause of present state of the Universe comprising of matter and radiation. Very simple chemistry started in proverbial first three minutes after the Big Bang when hydrogen and helium nuclei were created. After 380 thousand years the expanding Universe cooled down sufficiently ...
Name Origins: Back to the Beginning Video Questions http://www
Name Origins: Back to the Beginning Video Questions http://www

... http://www.pbs.org/wgbh/nova/space/origins-series-overview.html#origins-back-beginning 1. The Big Bang theory has been called the greatest discovery in cosmology. Describe it. ...
Big Bang Theory
Big Bang Theory

... Within the first minute, 98% of all matter in the universe was formed. It began cooling immediately. ...
The Evolution of the Universe: from Cosmic Soup to Earth
The Evolution of the Universe: from Cosmic Soup to Earth

... Big Bang: The initial point from which the universe began developing  approximately 13.7 billion years ago.   Cosmic Microwave Background: the leftover energy that can be detected  from the initial Big Bang.   Element: a pure chemical substance which is determined by the number of  protons in its nu ...
Lecture 33
Lecture 33

... • A few seconds after the Big Bang, the main particle species present were protons, neutrons, neutrinos, and photons ...
Elemental Abundances
Elemental Abundances

... in the harsh environment of stellar interiors • Li abundance comes from measurements in meteorites; it is still lower in the solar photosphere because of destruction by mixing with hotter layers below. • Abundant in primary cosmic rays as a result of fusion and spallation reactions between p and (ma ...
Helium Production in Big Bang Weighing a Galaxy12 Nov 11/12/2010
Helium Production in Big Bang Weighing a Galaxy12 Nov 11/12/2010

... • When T is between 10BK and 3BK, the density drops so that – number of collisions falls & neutrons and protons are no longer in  equilibrium. – Protons no longer change into neutrons. Neutrons decay into  protons. ...
Lecture 9
Lecture 9

... They all have large cross-sections and fast reaction rates ⇒ deuterium efficiently converts to 4 He. ...
Origin of Elements - Madison Public Schools
Origin of Elements - Madison Public Schools

... concentrated in one point. The “Big Bang” refers to the extraordinary explosion from that infinitesimal point. ...
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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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