Scientists / Open questions

基普·索恩

Kip S. Thorne

广义相对论、黑洞、引力波

2017 年诺贝尔物理学奖

28 个问题

Feasibility of the Braginsky–Polnarev–Thorne South Pole Foucault-pendulum measurement of the Earth's gravitomagnetic precession
Quantum-field-theoretic realizability and stability of traversable-wormhole time machines: the open questions of Morris, Thorne, and Yurtsever
Completing the dynamical stability picture of Melvin's magnetic universe: unrestricted finite-amplitude and nonradial perturbations, the toroidal magnetic geon, and the flux-resistance principle
Do vacuum fluctuations prevent the creation of closed timelike curves? (chronology protection for wormhole time machines)
The physical status of Thorne's C-energy: the torus–Schwarzschild mass relation, comparison with other energy prescriptions, and generalization to non-asymptotically-flat spacetimes (the open questions of Thorne 1965)
Robustness of the Thorne limit: the asymptotic spin and accretion efficiency of a black hole growing by disk accretion under realistic magnetic, radiative, and geometric conditions
Does a mechanical oscillator's initial quantum state influence classical-force monitoring by a strongly nonlinear (null-detector) meter?
Completing the Maxwell-like formulation of post-Newtonian gravity: the explicit 1PN energy-conservation law
Experimental realization of quantum nondemolition (back-action-evading) measurement of a harmonic oscillator with sensitivity below the standard quantum limit for weak-force detection
Finite curvature-coupling remainder of the renormalized stress-energy tensor near the horizon of a rotating black hole, and the regularity of the mirror-modified Hartle-Hawking state
Observational detection of gravitational-wave memory: first definitive evidence for the permanent strain offset of a gravitational-wave burst with memory
Realization of Pure Laboratory Tests of Relativistic Gravity with Controlled Laboratory Sources: Magnetic-Type Gravity, Stress-Produced Gravity, and Related Post-Newtonian Effects
Self-force-consistent transition from inspiral to plunge for generic (inclined, eccentric) orbits around a Kerr black hole
Environmental noise budget and practical feasibility of the Earth-orbiting 'skyhook' tether gravitational-wave detector (Braginsky–Thorne, 1985)
Seismic gravity-gradient (Newtonian) noise at the LIGO sites: site-specific determination and quantitative feasibility of monitoring-and-correction and moat shielding
Physical admissibility of spacetimes with closed timelike curves: self-consistency, benignness genericity, and chronology protection
Quantum propagation through a wormhole time machine beyond the free nonrelativistic case: relativistic and interacting extensions, singularity excision, and the probability prescription when unitarity fails
Schiff's conjecture: does the weak equivalence principle imply the Einstein equivalence principle for every complete, self-consistent theory of gravity?
Physical feasibility of macroscopic traversable wormholes: quantum energy inequalities and higher-dimensional bulk support
Does infinitesimal rotation prevent naked singularity formation in nonspherical relativistic collapse? The open reach of the Apostolatos–Thorne cylindrical bounce
Multiplicity of self-consistent solutions for a billiard ball in a wormhole time-machine spacetime: existence and classification
Testing black-hole MACHO (primordial black hole) binaries with gravitational waves: coalescence-rate prediction, primordial-spectrum consistency, and discrimination from neutron-star binaries
Validation of the Brady-Creighton-Thorne co-rotating minimal-strain scheme for the Intermediate Binary Black Hole (IBBH) problem
Explicit relations among the classical definitions of multipole moments for stationary isolated systems in general relativity (Thorne, 1980)

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Feasibility of the Braginsky–Polnarev–Thorne South Pole Foucault-pendulum measurement of the Earth's gravitomagnetic precession

Quantum-field-theoretic realizability and stability of traversable-wormhole time machines: the open questions of Morris, Thorne, and Yurtsever

Completing the dynamical stability picture of Melvin's magnetic universe: unrestricted finite-amplitude and nonradial perturbations, the toroidal magnetic geon, and the flux-resistance principle

Do vacuum fluctuations prevent the creation of closed timelike curves? (chronology protection for wormhole time machines)

The physical status of Thorne's C-energy: the torus–Schwarzschild mass relation, comparison with other energy prescriptions, and generalization to non-asymptotically-flat spacetimes (the open questions of Thorne 1965)

Robustness of the Thorne limit: the asymptotic spin and accretion efficiency of a black hole growing by disk accretion under realistic magnetic, radiative, and geometric conditions

Does a mechanical oscillator's initial quantum state influence classical-force monitoring by a strongly nonlinear (null-detector) meter?

Completing the Maxwell-like formulation of post-Newtonian gravity: the explicit 1PN energy-conservation law

Experimental realization of quantum nondemolition (back-action-evading) measurement of a harmonic oscillator with sensitivity below the standard quantum limit for weak-force detection

Finite curvature-coupling remainder of the renormalized stress-energy tensor near the horizon of a rotating black hole, and the regularity of the mirror-modified Hartle-Hawking state

Observational detection of gravitational-wave memory: first definitive evidence for the permanent strain offset of a gravitational-wave burst with memory

Realization of Pure Laboratory Tests of Relativistic Gravity with Controlled Laboratory Sources: Magnetic-Type Gravity, Stress-Produced Gravity, and Related Post-Newtonian Effects

Self-force-consistent transition from inspiral to plunge for generic (inclined, eccentric) orbits around a Kerr black hole

Environmental noise budget and practical feasibility of the Earth-orbiting 'skyhook' tether gravitational-wave detector (Braginsky–Thorne, 1985)

Seismic gravity-gradient (Newtonian) noise at the LIGO sites: site-specific determination and quantitative feasibility of monitoring-and-correction and moat shielding

Physical admissibility of spacetimes with closed timelike curves: self-consistency, benignness genericity, and chronology protection

Quantum propagation through a wormhole time machine beyond the free nonrelativistic case: relativistic and interacting extensions, singularity excision, and the probability prescription when unitarity fails

Schiff's conjecture: does the weak equivalence principle imply the Einstein equivalence principle for every complete, self-consistent theory of gravity?

Physical feasibility of macroscopic traversable wormholes: quantum energy inequalities and higher-dimensional bulk support

Does infinitesimal rotation prevent naked singularity formation in nonspherical relativistic collapse? The open reach of the Apostolatos–Thorne cylindrical bounce

Multiplicity of self-consistent solutions for a billiard ball in a wormhole time-machine spacetime: existence and classification

Testing black-hole MACHO (primordial black hole) binaries with gravitational waves: coalescence-rate prediction, primordial-spectrum consistency, and discrimination from neutron-star binaries

Validation of the Brady-Creighton-Thorne co-rotating minimal-strain scheme for the Intermediate Binary Black Hole (IBBH) problem

Explicit relations among the classical definitions of multipole moments for stationary isolated systems in general relativity (Thorne, 1980)