  We review aspects of black hole thermodynamics, and show how entanglement of
a quantum field between the inside and outside of a horizon can account for the
area-proportionality of black hole entropy, provided the field is in its ground
state. We show that the result continues to hold for Coherent States and
Squeezed States, while for Excited States, the entropy scales as a power of
area less than unity. We also identify location of the degrees of freedom which
give rise to the above entropy.
