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Quantum theory
Given a point in 4-dimensional Minkowski spacetime, its celestial (or heavenly) sphere is the space of lines in its light cone, hence the projective space of its light cone.
We can equivalently speak of rays in the past light cone (or rays in the future light cone); then your celestial sphere (the one around the point where your head is) is the sphere of which you directly perceive a portion when you look. (Since our eyes face forward, we actually see only a small portion of this sphere, but some birds see the entire sphere.) If you take the point to be Earth, then this celestial sphere is the sphere of the heavens as it appeared to the ancients.
By the exceptional spin isomorphism
one may identify points in Minkowski spacetime with Hermitean matrices
(where denote the generators of the Clifford algebra given by the Pauli matrices). This is such that the Lorentz metric norm is just the determinant of this matrix
From this one finds that is lightlike precisely if there is a spinor , hence a pair of complex numbers
such that
Therefore the celestial sphere is equivalently the space of such pairs of complex numbers, modulo rescaling for . This identifies the celestial sphere with the complex projective space
the Riemann sphere.
The celestial sphere may be given as a coset space of the Lorentz group. For the moment see here at n-sphere.
See also:
Last revised on January 19, 2023 at 13:36:02. See the history of this page for a list of all contributions to it.