Type IIB Supergravity
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Type IIB Supergravity
In supersymmetry, type IIB supergravity is the unique supergravity in ten dimensions with two supercharges of the same chirality (physics), chirality. It was first constructed in 1983 by John Henry Schwarz, John Schwarz and independently by Paul Howe and Peter West (physicist), Peter West at the level of its equations of motion. While it does not admit a fully covariant action (physics), action due to the presence of a Hodge star operator, self-dual field, it can be described by an action if the self-duality condition is imposed by hand on the resulting equations of motion. The other types of supergravity in ten dimensions are type IIA supergravity, which has two supercharges of opposing chirality, and type I supergravity, which has a single supercharge. The theory plays an important role in modern physics since it is the effective field theory, low-energy limit of type II string theory, type IIB string theory. History After supergravity was discovered in 1976, there was a conce ...
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Supersymmetry
Supersymmetry is a Theory, theoretical framework in physics that suggests the existence of a symmetry between Particle physics, particles with integer Spin (physics), spin (''bosons'') and particles with half-integer spin (''fermions''). It proposes that for every known particle, there exists a partner particle with different spin properties. There have been multiple experiments on supersymmetry that have failed to provide evidence that it exists in nature. If evidence is found, supersymmetry could help explain certain phenomena, such as the nature of dark matter and the hierarchy problem in particle physics. A supersymmetric theory is a theory in which the equations for force and the equations for matter are identical. In theoretical physics, theoretical and mathematical physics, any theory with this property has the ''principle of supersymmetry'' (SUSY). Dozens of supersymmetric theories exist. In theory, supersymmetry is a type of Spacetime symmetries, spacetime symmetry betwe ...
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