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- Alberto Carlini, Akio Hosoya, Tatsuhiko Koike, Yosuke Okudaira
- Physical review letters
- 2006

We present a general framework for finding the time-optimal evolution and the optimal Hamiltonian for a quantum system with a given set of initial and final states. Our formulation is based on the variational principle and is analogous to that for the brachistochrone in classical mechanics. We reduce the problem to a formal equation for the Hamiltonian… (More)

- A. Carlini
- 1995

We consider quantization of the Baierlein-Sharp-Wheeler form of the gravita-tional action, in which the lapse function is determined from the Hamiltonian constraint. This action has a square root form, analogous to the actions of the rela-tivistic particle and Nambu string. We argue that path-integral quantization of the gravitational action should be based… (More)

- A. Carlini, V. P. Frolov, H. H. Soleng
- 1996

We consider the action principle to derive the classical, non-relativistic motion of a self-interacting particle in a 4-D Lorentzian spacetime containing a wormhole and which allows the existence of closed time-like curves. For the case of a 'hard-sphere' self-interaction potential we show that the only possible trajectories (for a particle with fixed… (More)

- A Carlini, J Greensite
- 1993

We expand on the idea that spacetime signature should be treated as a dy-namical degree of freedom in quantum field theory. It has been argued that the probability distribution for signature, induced by massless free fields, is peaked at the Lorentzian value uniquely in D=4 dimensions. This argument is reviewed, and certain consistency constraints on the… (More)

- A. Carlini
- 1996

We consider the action principle to derive the classical, relativistic motion of a self-interacting particle in a 4-D Lorentzian spacetime containing a wormhole and which allows the existence of closed time-like curves. In particular, we study the case of a pointlike particle subject to a 'hard-sphere' self-interaction potential and which can traverse the… (More)

- A. Carlini, J. Greensite
- 1996

The classical field equations of general relativity can be expressed as a single geodesic equation, describing the free fall of a point particle in superspace. Based on this formulation, a " worldline " quantization of gravity, analogous to the Feynman-Schwinger treatment of particle propagation, is proposed, and a hidden mass-shell parameter is identified.… (More)

The phase of scalar field driven wormholes at one loop in the path integral formulation for Euclidean quantum gravity Abstract We here calculate the one-loop approximation to the Euclidean Quantum Gravity coupled to a scalar field around the classical Carlini and Miji´c wormhole solutions. The main result is that the Euclidean partition functional Z EQG in… (More)

- A. Carlini
- 1992

We consider the effect of vacuum polarization around the horizon of a 4 dimensional axionic stringy black hole. In the extreme degenerate limit (Q a = M), the lower limit on the black hole mass for avoiding the polarization of the surrounding medium is M ≫ (10 −15 ÷ 10 −11)m p (m p is the proton mass), according to the assumed value of the axion mass (m a ≃… (More)

- A. Carlini, A. Hosoya
- 2001

Grover's quantum algorithm for an unstructured search problem and the Count algorithm by Brassard et al. are generalized to the case when the initial state is arbitrarily and maximally entangled. This ansatz might be relevant with quantum subroutines, when the computational qubits and the environment are coupled, and in general when the control over the… (More)

- A. Carlini
- 1995

We consider the quantum analogues of wormholes obtained by Carlini and Miji´c (CM), who analytically continued closed universe models. To obtain wormholes when the strong energy condition (γ > 2/3) is satisfied, we are able to simplify the Wheeler-DeWitt (WDW) equation by using an equivalent scalar potential which is a function of the scale factor. Such… (More)