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[PDF] Top 20 Spin 1/2 in classical general relativity

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Spin 1/2 in classical general relativity

Spin 1/2 in classical general relativity

... Some authors have produced artificial models, parts of which, transform as a spinor see for example the cube within a cube described by Misner, Thorne and Wheeler[6] or the tethered rocks of Hartung [7]. This paper shows ... See full document

10

Linear-Time Algorithm for Quantum 2SAT

Linear-Time Algorithm for Quantum 2SAT

... the classical 2-SAT problem to the quantum case, but is also equivalent to the problem of finding a ground state of 2-local frustration-free Hamiltonians of spin 1/2, a ... See full document

27

Cosmic Dark Energy Density from Classical Mechanics and Seemingly Redundant Riemannian Finitely Many Tensor Components of Einstein’s General Relativity

Cosmic Dark Energy Density from Classical Mechanics and Seemingly Redundant Riemannian Finitely Many Tensor Components of Einstein’s General Relativity

... We determine the limit of the ratio formed by the independent components of the Riemann tensor to the non-zero component as space dimensionality tends to infinity and find it to be 12. Subse- quently we use this result ... See full document

5

Astronomical tests of general relativity

Astronomical tests of general relativity

... at 2 K where some escaping gas caused the gyroscopes to commence spinning up to an average rate of 72 ...the spin axis of the ...6".606 1 x 10 -6 yr -1 ...0.000 2 (Pitjeva, 2005). ... See full document

120

Discretization and Interaction of Fields via the Classical Kaluza Klein Theory

Discretization and Interaction of Fields via the Classical Kaluza Klein Theory

... through general relativity is based on the space-time section of the metric of a five-dimensional hyperspace-time, and that of elec- tromagnetism uses the first four components of its fifth line, or ... See full document

6

Black holes, TeV-scale gravity and the LHC

Black holes, TeV-scale gravity and the LHC

... is classical and described by general relativity, and the black hole emits quantum Hawking ...a classical metric, it must be the case that the Comp- ton wavelengths of the colliding particles ... See full document

16

The Nature of Inertial and Vacuum  Gravitational Field

The Nature of Inertial and Vacuum Gravitational Field

... Newton’s classical theory of gravity [1] [2] or in Einstein’s gener- al theory of relativity [3] [4] ...Newton’s classical theory of gravity and Einstein’s general theory of ... See full document

10

Topics in general relativity

Topics in general relativity

... [7, 2, 8, 9, 10, 11] where it was shown that embeddings are very useful tools to aid in the understanding of the dynamics of black ...the spin of a black hole formed in some process, and other physical ... See full document

120

McTaggart and Contemporary Physics

McTaggart and Contemporary Physics

... of general relativity where time is finite are ones where time goes in a ...by general relativity, the parallels are not as close as a science-minded McTaggartian would ...and general ... See full document

13

Spin, the Classical Theory

Spin, the Classical Theory

... that spin creates the torsion ...intrinsic spin of elementary particles, not orbital angular ...and spin the same parameters that give rise to the fundamental classical fields (other putative ... See full document

8

Tests of General Relativity with GW170817

Tests of General Relativity with GW170817

... In this paper we present a range of tests of general rela- tivity (GR) that have not yet been done with GW170817. Some of these are extensions of tests performed with previously discovered binary black hole ... See full document

14

Tests of general relativity with GW150914

Tests of general relativity with GW150914

... We have checked that if we perform this analysis on NR signals added to LIGO instrumental noise, the null (0, 0) re- sult expected in GR lies within the iso-probability contour that encloses 68% of the posterior roughly ... See full document

17

To the Schwarzschild Solution in General Relativity

To the Schwarzschild Solution in General Relativity

... of General Relativity found in 1916 by K. Schwarzschild [1] [2] which is interpreted in modern physics as the background of the objects referred to as Black ... See full document

13

Tests of General Relativity with GW150914

Tests of General Relativity with GW150914

... general relativity. We find that the final remnant ’ s mass and spin, as determined from the low-frequency (inspiral) and high-frequency (postinspiral) phases of the signal, are mutually consistent ... See full document

20

On Conformally Coupled General Relativity

On Conformally Coupled General Relativity

... arbitrary classical gravitational field in a series of nonlinear plain ...in general relativity, (a)(b) (k) is constrained by the following ... See full document

7

Tests of General Relativity with GW170817

Tests of General Relativity with GW170817

... In this paper we present a range of tests of general relativity (GR) that have not yet been done with GW170817. Some of these are extensions of tests per- formed with previously discovered binary black hole ... See full document

15

General Relativity by Kawaguchi geometry

General Relativity by Kawaguchi geometry

... The standard physical theory of fields is constructed on the fibre bundle structure, with the spacetime being the base manifold, and fields being its section. In such construction, the base manifold is chosen at the ... See full document

6

MACROSTATES THERMODYNAMICS AND ITS STABLE CLASSICAL LIMIT IN GLOBAL ONE  DIMENSIONAL QUANTUM GENERAL RELATIVITY

MACROSTATES THERMODYNAMICS AND ITS STABLE CLASSICAL LIMIT IN GLOBAL ONE DIMENSIONAL QUANTUM GENERAL RELATIVITY

... + 1 decomposed metric of General ...with General Relativity is achieved by the classical limit the Boltzmann gas limit of the macrostates thermodynamics, which is given by the energy ... See full document

26

A Classical Complete Action for a System of Small Point Massive Charged Particles in General Relativity

A Classical Complete Action for a System of Small Point Massive Charged Particles in General Relativity

... The idea of a small-point charged massive particle may be confusing, since in general a point particle is represented as a delta function and generates divergences. In fact, it behaves as a black hole. Therefore, ... See full document

17

Numerical Relativity beyond General Relativity

Numerical Relativity beyond General Relativity

... of general relativity. Since these theories are classical, we can hope to apply the numerical tools used to study GR (a classical theory) to these quantum-gravity-motivated ...around ... See full document

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