Line 18a3s Linear Frame Dragging Black Hole Rotating UFO LARES Minkowski Wormholes WOW SETI

Black Hole Rotational Frame Dragging

Kerr Black Hole

Line 18a3s Linear Frame Dragging Black Hole Rotating UFO LARES Minkowski Wormholes WOW SETI

part 122 of 100 videos there are more videos after this one i’ll post all then update the #.
Math Equation Wow Seti 1977 radio signal alien

14/

3/4/4/1/1/1/1/11=0.017
14/0.017=823.5294

Feb 13 2012 803 pm est

This caught my eye because it’s talking about rotation and propulsion for a space craft

Then it goes into results from previous testing from the gravity Probe B which was mentioned in another line of data.

Looking for accuracy a new test is scheduled for 2012.

In the last line of data we were looking at creating “anti-gravity” so that the ship can proceed quickly at a high rate of speed without having to deal with “frame dragging?”

The LARES Satellite from the Italian Space Agency is conducting tests to measure the Lense-Thirring effect. I’m going to look it up to see what it means…

Feb 13 2012 836 pm est
My thoughts:

Looking at the diagram above

Reminds me of my sketch of the UFO Engine we desire to build

Rotating body on the outside and a core circle in the middle that floats on the inside.

Could it be that this is the technology required to make such a thing?

Nonlinear gravitodynamics: the lense-thirring effect, a documentary Remo Ruffini, Costantino Sigismondi

How computers can help us in creating an intuitive access to relativity
Hanns Ruder1, Daniel Weiskopf2, Hans-Peter Nollert1 and Thomas Müller2

Minkowski diagrams showing two spatial dimensions, extended wormhole visualization, and the illustration of accretion discs

notes
Black Hole Rotational Frame Dragging

quote
The arm extended toward the black hole will be torqued spinward. The arm extended away from the black hole will be torqued anti-spinward. She will therefore be rotationally sped up, in a counter-rotating sense to the black hole.

This is the opposite of what happens in everyday experience.

If she is already rotating at some speed when she extends her arms, inertial effects and frame-dragging effects will balance and her spin will not change.

Due to the Principle of Equivalence gravitational effects are locally indistinguishable from inertial effects, so this rotation rate, at which when she extends her arms nothing happens, is her local reference for non-rotation.

This frame is rotating with respect to the fixed stars and counter-rotating with respect to the black hole. A useful metaphor is a planetary gear system with the black hole being the sun gear, the ice skater being a planetary gear and the outside universe being the ring gear. See Mach’s principle.

Another interesting consequence is that, for an object constrained in an equatorial orbit, but not in freefall, it weighs more if orbiting anti-spinward, and less if orbiting spinward.

For example, in a suspended equatorial bowling alley, a bowling ball rolled anti-spinward would weigh more than the same ball rolled in a spinward direction. Note, frame dragging will neither accelerate or slow down the bowling ball in either direction. It is not a “viscosity”.

Similarly, a stationary plumb-bob suspended over the rotating object will not list. It will hang vertically. If it starts to fall, induction will push it in the spinward direction.

Linear frame dragging is the similarly inevitable result of the general principle of relativity, applied to linear momentum.

Although it arguably has equal theoretical legitimacy to the “rotational” effect, the difficulty of obtaining an experimental verification of the effect means that it receives much less discussion and is often omitted from articles on frame-dragging (but see Einstein, 1921).[4]

Static mass increase is a third effect noted by Einstein in the same paper.[5] The effect is an increase in inertia of a body when other masses are placed nearby. While not strictly a frame dragging effect (the term frame dragging is not used by Einstein), it is demonstrated by Einstein that it derives from the same equation of general relativity.

Keplerian orbital elements are more affected by the non-gravitational perturbations like the direct solar radiation pressure: the use of the active, drag-free technology would be required.

Recently, an indirect test of the gravitomagnetic interaction accurate to 0.1% has been reported by Murphy et al. with the Lunar laser ranging (LLR) technique,[50] but Kopeikin questioned the ability of LLR to be sensitive to gravitomagnetism.[51]

The Gravity Probe B experiment[52][53] was a satellite-based mission by a Stanford group and NASA, used to experimentally measure another gravitomagnetic effect, the Schiff precession of a gyroscope,[54][55] to an expected 1% accuracy or better.

Unfortunately such accuracy was not achieved. The first preliminary results released in April 2007 pointed towards an accuracy of[56] 256–128%, with the hope of reaching about 13% in December 2007.[57] 

In 2008 the Senior Review Report of the NASA Astrophysics Division Operating Missions stated that it was unlikely that Gravity Probe B team will be able to reduce the errors to the level necessary to produce a convincing test of currently-untested aspects of General Relativity (including Frame-dragging).[58][59] 

On May 4, 2011, the Stanford-based analysis group and NASA announced the final report[60], and in it the data from GP-B demonstrated the frame-dragging effect with an error of about 19 percent.[61] The findings were accepted for publication in the journal Physical Review Letters.[62]

Recently, the Italian Space Agency (ASI) has announced that the LARES satellite should be launched with a Vega rocket at the beginning of 2012.[64] The goal of LARES is to measure the Lense–Thirring effect to 1%, but there are doubts that this can be achieved,[65][66][67][68][69] mainly due to the relatively low orbit which LARES should be inserted into bringing into play more mismodelled even zonal harmonics.[clarification needed] 

That is, spherical harmonics of the Earth’s gravitational field caused by mass concentrations (like mountains) can drag a satellite in a way which may be difficult to distinguish from frame-dragging.

In the case of stars orbiting close to a spinning, supermassive black hole, frame dragging should cause the star’s orbital plane to precess about the black hole spin axis. This effect should be detectable within the next few years via astrometric monitoring of stars at the center of the Milky Way galaxy.[70] 

By comparing the rate of orbital precession of two stars on different orbits, it is possible in principle to test the no-hair theorems of general relativity, in addition to measuring the spin of the black hole.[71]

Pasted from

worm hole black hole math equations diagram wow seti the idea girl says

Feb 13 2012 803 pm est

This caught my eye because it’s talking about rotation and propulsion for a space craft

Then it goes into results from previous testing from the gravity Probe B which was mentioned in another line of data.

Looking for accuracy a new test is scheduled for 2012.

In the last line of data we were looking at creating “anti-gravity” so that the ship can proceed quickly at a high rate of speed without having to deal with “frame dragging?”

The LARES Satellite from the Italian Space Agency is conducting tests to measure the Lense-Thirring effect. I’m going to look it up to see what it means…

Google Lense-Thirring effect

Nonlinear gravitodynamics the lense-thirring effect, a documentary ...remo ruffini costantino sigismondi book cover

Nonlinear gravitodynamics: the lense-thirring effect, a documentary …
 

Remo Ruffini, Costantino Sigismondi
0 Reviews
World Scientific, 2003 - Science - 509 pages
This book gives a detailed, up-to-date account of the Lense-Thirring effect and its implications for physics and astrophysics.

Starting from a profound intuition of Lense and Thirring in 1918, based on a simple solution to the linearized Einstein field equations, this has emerged in the past four decades as a phenomenon of extraordinary importance in cosmology, radio jets in quasars, and the physics of neutron stars and black holes, besides leading to some of the most sophisticated experiments ever performed in the space surrounding our planet.

The book contains the contributions presented at the “Third William Fairbank Meeting,” which have been expanded by adding a complete set of classical and prominent contemporary papers on this subject and a general introduction by R Ruffini.

Pasted from

quote
Google
NASA Astrophysics Division Operating Missions

Held every two years, the Operating Mission Senior Review evaluates proposals from operating missions for continued funding.

The Astrophysics Division uses the Senior Review to maximize scientific productivity of operating missions that have completed prime operations.

A total of 9 projects have been invited to participate in the Astrophysics 2012 Senior Review to be held on February 28-March 2, 2012: Chandra, Fermi, Hubble, Kepler, Planck, Swift, Suzaku, Spitzer, and XMM-Newton.

Pasted from

Patent US20060073976 – Method of gravity distortion and … - Google
www.google.com/patents/US20060073976
Block all www.google.com results
… a method to take advantage of the Lense-Thirring effect, to simulate the effect … the effect of two point masses on nearly radial orbits…http://www.google.com/ …

Pasted from

Application number: 10/954,767
Publication number: US 2006/0073976 A1
Filing date: Oct 1, 2004

Method of gravity distortion and time displacement
 Marlin B. Pohlman

Pasted from

A method for employing sinusoidal oscillations of electrical bombardment on the surface of one Kerr type singularity in close proximity to a second Kerr type singularity in such a method to take advantage of the Lense-Thirring effect, to simulate the effect of two point masses on nearly radial orbits in a 2+1 dimensional anti-de Sitter space resulting in creation of circular timelike geodesics conforming to the van Stockum under the Van Den Broeck modification of the Alcubierre geometry (Van Den Broeck 1999) permitting topology change from one spacelike boundary to the other in accordance with Geroch’s theorem (Geroch 1967) which results in a method for the formation of G{umlaut over ( )}odel-type geodesically complete spacetime envelopes complete with closed timelike curves.

Inventor: Marlin B. Pohlman
Current U.S. Classification: 505/166; 73/382.00G; 434/300; 505/164; 505/180

View patent at USPTO
Search USPTO Assignment Database

Claims
1. A method for the generation of a pseudo 2+1 dimensional anti-de Sitter space comprising the steps of:
creating two Kerr type positively charged rotating dilation singularities, including the steps of
maintaining one of the singularities as a axis of rotation reference singularity,
maintaining the other of the singularities as a target singularity, and
subjecting the target singularity to a differential electron flow so as to simultaneously pass the differential electron flow above a photosphere of said target singularity in a direction of rotation thereof and contrary to the direction of rotation thereof, in order to release a directed flow of gravitons in a sinusoidal oscillation simulating a rotational effect of the target singularity around the axis of rotation provided by the reference singularity.
2. A method of generating a force around a body, comprising the steps of: employing sinusoidal oscillations of electrical bombardment on the surface of one Kerr type reference singularity in close proximity to a second Kerr type target singularity to take advantage of the Lense-Thirring effect,

wherein the electrical currents employed in the bombardment are passed simultaneously across the photosphere of said reference singularity in its direction of rotation and contrary to its direction of rotation to release a directed flow of gravitons in a sinusoidal oscillation simulating a rotational effect of the target singularity around the axis of rotation provided by the reference singularity;

creating timelike curves in a compact time-oriented manifold of G{umlaut over ( )}odel-type geodesically complete spacetime envelope under the Van Den Broeck modification of the Alcubierre geometry, resulting in the creation of timelike curves in a compact time-oriented manifold permitting topology change from one spacelike boundary to the other in accordance with Geroch’s theorem.

Pasted from

us 2006 007 3976 a1 patent number invention method of gravity distortion and time displacement ufo engine components the idea girl says youtub

Feb 13 2012 836 pm est
My thoughts:

Looking at the diagram above

Reminds me of my sketch of the UFO Engine we desire to build

Rotating body on the outside and a core circle in the middle that floats on the inside.

Could it be that this is the technology required to make such a thing?

us 2006 007 3976 a1 patent number invention method of gravity distortion and time displacement ufo engine components martin b pohlman the idea girl says youtub

New J. Phys. 10 (2008) 125014
doi:10.1088/1367-2630/10/12/125014

How computers can help us in creating an intuitive access to relativity
Hanns Ruder1, Daniel Weiskopf2, Hans-Peter Nollert1 and Thomas Müller2

1 Theoretical Astrophysics, University of Tübingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
2 VISUS (Visualization Research Center), Universität Stuttgart, Nobelstr. 15, 70569 Stuttgart, Germany
E-mail: nollert@tat.physik.uni-tuebingen.de
Received 13 August 2008
Published 1 December 2008

Abstract. Computers have added many new possibilities to the tool box used for visualizing science in general and relativity in particular.

We present some new results from our own work: (2 + 1) dimensional Minkowski diagrams showing two spatial dimensions, extended wormhole visualization, and the illustration of accretion discs by using the approximation via a rigidly rotating disc of dust.

We also discuss some related examples from our earlier work, such as interactive and immersive visualization, or the visualization of the warp drive metric.

Contents
• 1. Introduction
• 2. Theory of special relativity
• 2.1. (2 + 1) dimensional Minkowski diagrams
• 2.2. First-person perspective: interactive and immersive installations
• 3. Theory of general relativity
• 3.1. Wormholes
• 3.1.1. Interactive visualization of wormhole geometries
• 3.2. Warp drive bubbles
• 3.3. Discs in relativistic astrophysics
• 4. Technical and logistic challenges
• Acknowledgments
• References

Pasted from

Figure 1. Multiple and coordinated views of different visualization paradigms of the same scene

Figure 1. Multiple and coordinated views of different visualization paradigms of the same scene: (left) three-dimensional (3D) rendering of the static spatial scene, (top-right) ego-centric view from the fast moving camera, (bottom-right) the respective (2 + 1) dimensional Minkowski diagram.

Pasted from

Figure 9. Left Doppler effect resulting from motion at a velocity of 95% of the speed of light

Null geodesics in a Morris–Thorne wormhole space-time

Figure 10. Null geodesics in a Morris–Thorne wormhole space-time: light rays separated by Δξ = 5° (where ξ = 0 denotes the radial direction) in the observer’s frame may originate from the same side or from the other side of the wormhole.

Pasted from

Figure 18 shows a hypothetical machine creating a non-rotating Morris–Thorne wormhole and another one for a rotating wormhole

A Morris–Thorne wormhole has no angular momentum, but it may be generalized to describe a rotating wormhole in a way similar to going from a Schwarzschild metric to a Kerr metric [15].

Figure 18 shows a hypothetical machine creating a non-rotating Morris–Thorne wormhole and another one for a rotating wormhole. A rotating wormhole may contain an ergoregion [15].

Even more interesting for someone passing through may be the fact that the exotic matter which is necessary for stabilizing any traversable wormhole need not be distributed evenly around the throat, as it has to be for a non-rotating wormhole. Therefore there may be trajectories through the wormhole which do not touch exotic matter.

Pasted from

The null geodesics are computed for the Schwarzschild 

Pasted from

Looks like

UFO

Figure 22. Visualization of an accretion disc around a black hole. Colours correspond to temperatures on the surface of the disc.

Figure 22. Visualization of an accretion disc around a black hole. Colours correspond to temperatures on the surface of the disc.

The hydrodynamics equations are solved using an SPH code in a Newtonian space-time.

The differences from a fully relativistic simulation are probably small enough to be hardly visible in a picture like this. Image reprinted from Nollert et al  [10].

Pasted from

The hydrodynamical SPH simulation has been performed in a completely non-relativistic environment, i.e. using a Newtonian gravitational field for the dynamics of the disc.

Self-gravitation of the disc is neglected completely.

The major problem in doing a relativistic simulation is not that the hydrodynamics equations become more complicated on a relativistic background, but rather the fact that no covariant definition of viscosity exists [17].

Pasted from

Figure 23. Abstract visualization of the rotating disc of dust with varying value μ = 0.2, 0.8, 1.5 (from left to right).

Pasted from

Acknowledgments
We thank Roland Speith for providing the data for the surface image of an accretion disc around a black hole. Marc Borchers provided figures 5 and 7–9, Heinrich H Bülthoff of the Max Planck Institute for Biological Cybernetics, Tübingen granted permission to use their 3D model of the old city of Tübingen in generating these figures. Oliver Fechtig created the images for figure 18.

Pasted from

Figure 23. Abstract visualization of the rotating disc of dust with varying value μ = 0.2, 0.8, 1.5 (from left to right).