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Fusion of atoms releases energy, and that process drives the nuclear furnaces at the heart of stars.
The idea for a hydrogen bomb, based on the fusion of atoms, apparently originated with Enrico Fermi, the Italian physicist, in 1941, a year before Dr. Fermi's team achieved the first fission chain reaction at the University of Chicago, opening the way for developing the atomic bomb.
With energy produced through the fusion of atoms rather then their splitting, the "Castle Bravo" test detonated with the force of 15 million tons of TNT -- 1,000 times more powerful than either of the bombs dropped on Japan.
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It is true that there are many fusions of atoms, but these are all the same cloud.
Lewis's first objection is that it positing clouds as well as cloud-constituting fusions of atoms is metaphysically extravagant.
Such blobs, astronomers believe, could only arise deep within the core of the blast from the flash fusion of silicon atoms into unstable atoms of nickel, a process that lasts a fraction of a second and requires temperatures of at least 5 billion degrees.
The temperature at the core of the Sun is too low for nuclear fusion of helium atoms through the triple-alpha process, so these atoms do not contribute to the net energy generation that is needed to maintain hydrostatic equilibrium of the Sun.
In late 1998, Polish physicist Robert Smolańczuk published calculations on the fusion of atomic nuclei towards the synthesis of superheavy atoms, including ununoctium.
In late 1998, Polish physicist Robert Smolańczuk published calculations on the fusion of atomic nuclei towards the synthesis of superheavy atoms, including ununoctium and livermorium.
They believed that when squeezed into the palladium, the hydrogen atoms would fuse together, releasing a burst of energy, just as the fusion of hydrogen atoms in the sun produces heat and light.
In contrast, the hydrogen bomb depends on the fusion of light atoms, mainly forms of hydrogen.
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