Quantum Bit Error Avoidance
Qubit errors might be avoided by using the quantum Zeno effect to inhibit evolution.
arXiv subjects
Publications and source records attributed to A. Y. Shiekh.
Qubit errors might be avoided by using the quantum Zeno effect to inhibit evolution.
It is argued that it takes an infinite amount of external time for a freely falling test particle to reach the event horizon of a classical black hole (which happens in finite faller time), and that in this time the black hole would have evaporated due to Hawking radiation; so the freely falling test particle would itself evaporate at the event horizon, and so not pass through.
It may be possible to use operator regularization with Feynman diagrams, which would greatly simplify its use as it has so far been limited to the more complicated Schwinger approach. Operator regularization, unlike $ζ$-function regularization, is not limited to one-loop order, and preserves supersymmetry unlike dimensional regularization. In practice the use of operator regularization in the context of Feynman diagrams is found not to complicate the calculation.
It may be possible to extend the Grover search algorithm by taking a divide and conquer approach using auxiliary solutions to achieve an exponential speed-up.
A proposal for an experiment to look at some possibly novel aspects of quantum interference is presented, along with some Engineering applications that might result.
An apparent paradox for unitarity non-conservation is investigated for the case of destructive quantum interference.
Faster than light communication might be possible using the collapse of the quantum wave-function without any accompanying paradoxes.
In a recent paper the author proposed the possibility of an experiment to perform faster-than-light communication via the collapse of the quantum wave-function. This was analyzed by Bassi and Ghirardi, and it is believed that this analysis itself merits a detailed examination.
An experiment is proposed to test the interference aspect of the Quantum Interference Computer approach
An error correcting mechanism is proposed in the context of the Quantum Interference Computer approach
Quantum interference is proposed as a tool to augment Quantum Computation.
It is well known that Einstein gravity is non-renormalizable; however this does not preclude the existence of a quantum form.
It is well known that Einstein gravity is non-renormalizable; however a generalized approach is proposed that leads to Einstein gravity {\it after} renormalization. This them implies that at least one candidate for quantum gravity treats all matter on an equal footing with regard to the gravitational behaviour.
A preferred form for the path integral discretization is suggested that allows the implementation of canonical transformations in quantum theory.
A suggestion is made for quantizing gravity perturbatively, and is illustrated for the example of a massive scalar field with gravity.
A scalar field theory is investigated within the context of orthodox quantum gravity.
Besides having some very interesting perturbatively unstable orbits, it seems that for a Schwarzschild black hole, below $r=3M$, the force always increases inward with increasing angular momentum. Here this previously known result is derived with greater simplicity, and a similar analysis is performed for black holes with angular momentum and charge.