An observer accelerating through a vacuum will observe an increase in this quantity equal to their acceleration times h-bar over quantity Boltzmann's constant times 2 pi c.
An observer accelerating through a vacuum will observe an increase in this quantity equal to their acceleration times h-bar over quantity Boltzmann's constant times 2 pi c. When applying a set of laws about this quantity to a black hole, the place it usually occupies is filled by a constant multiple of kappa, the surface gravity. The energy to erase one bit of information is proportional to this quantity, according to Landauer's principle. In the microcanonical ensemble, the partial derivative of entropy with respect to energy is the reciprocal of this quantity. The power per area of a blackbody equals the Stefan-Boltzmann constant times its fourth power. Gibbs free energy equals enthalpy minus entropy times this quantity. For 10 points, name this quantity which is equal for two bodies at thermal equilibrium.
An observer accelerating through a vacuum will observe an increase in this quantity equal to their acceleration times h-bar over quantity Boltzmann's constant times 2 pi c.
temperature