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Thermochemistry
Thermochemistry

... the potential (location of atoms, forces between the nucleus and the electrons, the forces between the electrons, the forces between the protons and the neutrons, and the forces between the atoms as the bond). What changes significantly in a chemical reaction? The bond. Bonds are broken in chemical ...
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... at 300 K only 1 in 1011 collisions between H2 and N2 results in a reaction! Even at 800 K only 1 in 104 collisions results in a reaction. The collision theory says: Reactions occur when molecules collide with a certain minimum kinetic energy. The more frequent these collisions, the faster the rate o ...
Kinetics of a Reaction
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... and under same condition, products get decomposed into reacants. “A chemical equilibrium is a state in which a reversible chemical reaction is proceeding in both forward and reverse direction with equal rate at given set of conditions.” Foe example, CaCO3 ↔ CaO + CO2 In this reversible chemical reac ...
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Nuclear and Thermal Physics
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Indian National Physics Olympiad – 2014 - HBCSE
Indian National Physics Olympiad – 2014 - HBCSE

... (d) In the figure below mark the approximate locations of the equilibrium point(s) for this system. Justify your answer. Solution: For small δ force on the test charge is upwards while for large δ (eg. at D) force is downwards. So there is a neutral point between O and D. By symmetry there will be n ...
Physics, Chapter 44: Stable Nuclei
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... Investigations with the mass spectrograph have established that there are about 300 different stable isotopes among the 102 known elements. The range of mass numbers runs from 1 to more than 250. The atomic masses of these isotopes differ very little from whole numbers. The number of stable isotopes ...
PRECURSORS AND THE FUSION REACTIONS IN POLARISED Pd/D-D O SYSTEM:
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RTD Part 4 - County Central High School
RTD Part 4 - County Central High School

... Use the following information to answer the next seven questions. There are many different types of propulsion engines for satellites. One type of ion propulsion thrust chamber and the satellite to which it is attached are described below. The cylindrical thrust chamber of the engine has a central ...
KIN1PP - Knockhardy
KIN1PP - Knockhardy

... One can look at the QUALITATIVE and the QUANTITATIVE aspects of how the rate (speed) of a reaction can be changed. Chemical kinetics plays an important part in industrial chemistry because the time taken for a reaction to take place and the energy required are of great economic importance. The kinet ...
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Nuclear fusion



In nuclear physics, nuclear fusion is a nuclear reaction in which two or more atomic nuclei come very close and then collide at a very high speed and join to form a new nucleus. During this process, matter is not conserved because some of the matter of the fusing nuclei is converted to photons (energy). Fusion is the process that powers active or ""main sequence"" stars.The fusion of two nuclei with lower masses than Iron-56 (which, along with Nickel-62, has the largest binding energy per nucleon) generally releases energy, while the fusion of nuclei heavier than iron absorbs energy. The opposite is true for the reverse process, nuclear fission. This means that fusion generally occurs for lighter elements only, and likewise, that fission normally occurs only for heavier elements. There are extreme astrophysical events that can lead to short periods of fusion with heavier nuclei. This is the process that gives rise to nucleosynthesis, the creation of the heavy elements during events such as supernova.Following the discovery of quantum tunneling by Friedrich Hund, in 1929 Robert Atkinson and Fritz Houtermans used the measured masses of light elements to predict that large amounts of energy could be released by fusing small nuclei. Building upon the nuclear transmutation experiments by Ernest Rutherford, carried out several years earlier, the laboratory fusion of hydrogen isotopes was first accomplished by Mark Oliphant in 1932. During the remainder of that decade the steps of the main cycle of nuclear fusion in stars were worked out by Hans Bethe. Research into fusion for military purposes began in the early 1940s as part of the Manhattan Project. Fusion was accomplished in 1951 with the Greenhouse Item nuclear test. Nuclear fusion on a large scale in an explosion was first carried out on November 1, 1952, in the Ivy Mike hydrogen bomb test.Research into developing controlled thermonuclear fusion for civil purposes also began in earnest in the 1950s, and it continues to this day. The present article is about the theory of fusion. For details of the quest for controlled fusion and its history, see the article Fusion power.
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