Black Holes
... light that hits the horizon, reflecting nothing, just like a perfect black body in thermodynamics. • Quantum mechanics predicts that event horizons emit radiation like a black body with a finite temperature. ...
... light that hits the horizon, reflecting nothing, just like a perfect black body in thermodynamics. • Quantum mechanics predicts that event horizons emit radiation like a black body with a finite temperature. ...
PHYSICS 015
... For the most massive stars, the Schwarzschild radius is already too big. For example, if you wanted to allow a 10-solar-mass star to settle down as a neutron star, about 10 km in diameter, it already inside its Schwarzschild radius and is doomed to collapse! Stars can’t ‘know’ that they should shed ...
... For the most massive stars, the Schwarzschild radius is already too big. For example, if you wanted to allow a 10-solar-mass star to settle down as a neutron star, about 10 km in diameter, it already inside its Schwarzschild radius and is doomed to collapse! Stars can’t ‘know’ that they should shed ...
