, where:

= Cosmological Constant (1/m^{2})

, where:

= Angle of Deflection

G = Gravitational Constant (m^{3}/(kg*s^{2}))

M = Mass Causing Gravity (kg)

r = Distance from Mass (m)

c = Speed of Light (m/s)

, where:

= Ricci Curvature Tensor

R = Curvature (m)

= Metric Tensor

Also known as Stefan–Boltzmann-Schwarzschild-Hawking black hole radiation power law,

, where:

P = Power lost by Black Hole (W)

= Dirac's Constant (J*s)

c = Speed of Light (m/s)

= Pi

, where:

P = Power lost (W)

G = Gravitational Constant (m^{3}/(kg*s^{2}))

c = Speed of Light (m/s)

m_{1} = Mass of body 1 (kg)

m_{2} = Mass of body 2 (kg)

r = Distance between bodies (m)