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Quantum mechanics without spacetime: a case for noncommutative geometry

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arxiv gr-qc/0510042 v1 pith:3R5EJIMT submitted 2005-10-09 gr-qc hep-thquant-ph

classification gr-qchep-thquant-ph
keywords quantumclassicalmechanicsspacetimeformulationnon-lineartheoryapproach
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Quantum mechanics in its presently known formulation requires an external classical time for its description. A classical spacetime manifold and a classical spacetime metric are produced by classical matter fields. In the absence of such classical matter fields, quantum mechanics should be formulated without reference to a classical time. If such a new formulation exists, it follows as a consequence that standard linear quantum mechanics is a limiting case of an underlying non-linear quantum theory. A possible approach to the new formulation is through the use of noncommuting spacetime coordinates in noncommutative differential geometry. Here, the non-linear theory is described by a non-linear Schrodinger equation which belongs to the Doebner-Goldin class of equations, discovered some years ago. This mass-dependent non-linearity is significant when particle masses are comparable to Planck mass, and negligible otherwise. Such a non-linearity is in principle detectable through experimental tests of quantum mechanics for mesoscopic systems, and is a valuable empirical probe of theories of quantum gravity. We also briefly remark on the possible connection our approach could have with loop quantum gravity and string theory.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Black hole entropy from trace dynamics and non-commutative geometry

    gr-qc 2019-09 reject novelty 4.0 of 10

    A speculative calculation that recovers black hole entropy by identifying the trace-dynamics partition function result with the Euclidean gravitational action, after several assumptions that make the microstate count cancel.

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