Cosmological constant

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Cosmological constants are observed values for naturally occurring phenomena.  The include but are not limited to the speed of light in a vacuum, the force of gravity in relation to mass, the nuclear strong force, the weak force, and the electromagnetic force. k force, and the electromagnetic force.
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Cosmological constants (also known as physical or universal constants) are observed and measured values for naturally occurring phenomena.  These include, but are not limited to, the speed of light in a vacuum <math>c</math>, the gravitational constant <math>G</math>, Plancks constant <math>\hbar</math>, the elementary charge <math>e</math> and the permittivity of free space ε<sub>0</sub>.
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== Arguments ==
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* [[Fine tuning argument]]

Revision as of 06:53, 12 October 2006

Cosmological constants (also known as physical or universal constants) are observed and measured values for naturally occurring phenomena. These include, but are not limited to, the speed of light in a vacuum <math>c</math>, the gravitational constant <math>G</math>, Plancks constant <math>\hbar</math>, the elementary charge <math>e</math> and the permittivity of free space ε0.

Arguments

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