Paul LaViolette will give one-day seminar in Amsterdam on March 27th, which will cover a broad range of subjects: Subquantum Kinetics, Ether Physics, Continuous Creation Cosmology, Free Energy and Gravity Control Technologies, Advanced science encoded in ancient creation myths, and much more.
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1) The Pleistocene extinction. Dr. LaViolette's paper presenting evidence that the Pleistocene megafaunal extinction had a solar flare cause has been published in the June issue of the journal Radiocarbon;(1) see press release. LaViolette needs funds to attend a scientific conference to present its findings.
2) Ice core and ocean sediment analysis to study the solar flare event that terminated the Pleistocene extinction episode. As a follow up to the discoveries published in study (2) above,(1) Starburst would like to carry out a detailed chemical analysis of Greenland ice and ocean sediment cores to look for evidence that the Pleistocene extinction was terminated by an intense solar cosmic ray storm and that this event was also responsible for depositing ET indicators found in the YDB layer at the base of the black mat in the southwestern U.S. and in the Usello Horizon in Europe. P. LaViolette has identified an acidic layer in the Summit, Greenland polar ice core record that dates around 12,887±10 years before 2000 (b2k) which he believes registers the impact of a solar coronal mass ejection strong enough to overpower the Earth's magnetosheath and allow vast quantities of solar cosmic ray radiation to enter the atmosphere and produce lethal radiation levels at the Earth's surface. For this project we would measure the concentrations of cosmic dust indicators such as iridium, nickel, and gold in 20 samples spanning this part of the ice record. This could be done by using either neutron activation analysis or inductively coupled plasma mass spectrometry. We would also carry out a scanning electron microscope study of the dust found in this part of the ice core to search for the presence of cosmic spherules similar to those found in the YDB layer overlying the terminal extinction boundary. Further, we would analyze the beryllium-10 concentrations in these samples using accelerator mass spectrometry. We also would like to measure radiocarbon and Be-10 concentrations in 6-month sample intervals spanning two sections of the Cariaco Basin ocean sediment record corresponding to the 12,887 and 12,689 years b2k radiocarbon spurts. These two projects would be conducted with other researchers expert in Be-10 and radiocarbon analysis. It is expected that the study could take two years to plan and complete.
3) Publishing papers on climatology/geology. With proper funding, Dr. LaViolette could publish additional scientific papers about Galactic superwaves and their effects on the Earth's climate and biosphere. See references 2-13 for past publications. He has several papers that are in the process of being made ready for publication. These present the following:
a) a discussion of his discovery of heavy metals in polar ice (tin, antimony, gold, silver, and iridium whose results were presented in his dissertation, but never published,
b) Evidence of solar-induced global warming at the end of the last ice age, and that this warming was caused by the passage of a Galactic superwave,
c) A discussion of the glacier wave concept of continental flooding and the new interpretation it offers for Heinrich events.Once these papers are written and edited they would be ready to be submitted for publication. They may encounter substantial resistance from conservative climatology and geology journals since their proposed hypotheses challenge existing climatological, geological, and astronomical theories.
4) Superwave periodicity. With the volunteer help of a company in Seattle, Starburst has conducted a fast Fourier transform analysis of beryllium-10 peaks found at various depths in the Vostok ice core. This has allowed us to estimate the periodicity of superwaves. Analysis should also be performed on the Vostok ice core data that Liritzis and Grigori analyzed to compare with the periods that they have reported. The findings need to be written up and published in a scientific journal.
5) Communicating the superwave theory. Additional funds would support Starburst's efforts to network with other scientists who are doing work relevant to the superwave theory and to present papers on the superwave theory at scientific conferences. Starburst will also contact Federal government personnel to make them aware of the superwave phenomenon. Starburst also would like to continue the updating of Dr. LaViolette's Ph.D. thesis which is available on CD.
6) Public relations. Writing and sending out press releases about LaViolette's discoveries, contacting the media, emailing scientists preprints of LaViolette's papers.
7) Networking with alternative technology groups and superwave survival groups. A part time volunteer assistant could be hired to network with groups around the world who are preparing alternative technologies that will assist independent living (energy and food independence) and to network with groups preparing for superwave survival. Although there is no definite indication of claims that a superwave will arrive in 2012, it is advisable to encourage preparedness. This project could also be responsible for networking with prayer groups around the world to be ready to organize mass prayers in the event of a superwave arrival.
8) Public lecturing. Public lectures could be organized that would inform people about galactic superwaves, subquantum kinetics, and exotic energy and propulsion technologies. This budget would include traveling and lodging expenses not covered by the lecture host and time for the speaker to prepare the lecture.
Simulations carried out by Matt Pulver.
3D simulation showing a subatomic particle forming from an X potential ZPE fluctuation
This is a one-dimensional cross section of a spherically symmetric particle extending radially in three dimensions. Simulation parameters: Reaction volume radius = 50 spatial units, vacuum boundary conditions, X potential seed fluctuation: 1 sigma in space, 3 sigma in time.
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3D simulation showing subatomic particle autogenesis (vertically expanded view)
This is a one-dimensional cross section of a spherically symmetric particle extending radially in three dimensions. Simulation parameters: Reaction volume radius = 50 spatial units, vacuum boundary conditions, X potential seed fluctuation: 1 sigma in space, 3 sigma in time.
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3D simulation showing particle with higher core diffusion coefficient
This is a one-dimensional cross section of a spherically symmetric particle extending radially in three dimensions. Simulation parameters: Reaction volume: 3D, Radius = 50 spatial units, vacuum boundary conditions, X potential seed fluctuation: 1 sigma in space, 3 sigma in time. Diffusion coefficient = 2 at center and decreases to 1 with sigma = 1.5 spatial units.
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3D simulation showing particle with lower core diffusion coefficient
This is a one-dimensional cross section of a spherically symmetric particle extending radially in three dimensions. Simulation parameters: Reaction volume radius = 50 spatial units, vacuum boundary conditions, X potential seed fluctuation: 1 sigma in space, 3 sigma in time. Diffusion coefficient = 0.5 at center and increases to 1 with sigma = 1.5 spatial units.
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2D simulation showing a subatomic particle forming from an X potential ZPE fluctuation
This is a one-dimensional cross section of circularly symmetric particle extending radially in two dimensions. Simulation parameters: Reaction volume radius = 50 spatial units, vacuum boundary conditions, X potential seed fluctuation: 1 sigma in space, 3 sigma in time.
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This is a one-dimensional plot of a particle formed in a one-dimensional reaction volume. Simulation parameters: Reaction volume radius = 50 spatial units, vacuum boundary conditions, X potential seed fluctuation: 1 sigma in space, 3 sigma in time.
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This is a one-dimensional plot of a particle formed in a one-dimensional reaction volume. Simulation parameters: Reaction volume radius = 50 spatial units, vacuum boundary conditions, X potential seed fluctuation: 1 sigma in space, 3 sigma in time.
Next Page: Particle Bound States
The Starburst Foundation is a nonprofit research institute based in Schenectady, New York and Athens, Greece.
It was incorporated in the state of Oregon in January of 1984 for the purpose of carrying out scientific research and public education directed to the betterment of humanity and the planet. The Foundation's research activities are carried out with the intention of:
Starburst serves as a vehicle through which donors may support high-quality leading-edge research necessary to mankind's survival in this new age.
History has shown that the most significant scientific breakthroughs were not deduced from the existing theoretical framework, but rather arose as marked departures from conventional thinking. Generally such new views challenged long-cherished assumptions espoused by the established paradigm and were therefore actively resisted by the old guard.
The peer review process, which normally is relied on to determine which ideas out of the many should become funded, is often subject to this bias. As a result, new ideas that could potentially produce scientific breakthroughs are generally refused funding. Thus most work carried out in today's research institutions tends to be traditional, rather than innovative.
The Starburst Foundation was formed to circumvent this problem. It serves as a vehicle through which donors may fund high-quality leading-edge research that otherwise would have great difficulty finding financial support. By greasing the wheels of change, the Starburst Foundation helps to create new concepts and tools necessary to mankind's survival in the new age that is now upon us.
Outside the supermassive core, the gravity potential field
varies inversely with radial distance (φG ~ 1/r) as shown above.
But inside, it varies approximately as r2, plateauing at the core's center.
The luminous cosmic ray emitting source at the center of our Galaxy is a celestial orb that is about 4.3 million times the mass of our Sun and the most massive object in our Galaxy. Currently it is seen to radiate about 20 million times as much electromagnetic energy as our Sun. By one estimate, it radiates most of its energy as cosmic ray electrons and protons, giving it a total luminosity 2.5 billion times that of the Sun (LaViolette, Subquantum Kinetics, 2012). Based on early radio observations, it was given the designation Sagittarius A*.
Stars orbit this body with velocities as high as 50% of the speed of light. Gas and dust also orbits Sgr A* but does not fall toward it. It is instead seen to be moving radially outward from this source. After long intervals, the matter/energy generation process within the Sagittarius A* becomes unstable and it explodes with intense luminosity. Such galactic core explosions pose a potential threat to our planet.
Would Galileo be able to pursue his hypothesis today?
History has shown that many of man's greatest discoveries came about because someone dared to challenge the assumed knowledge of the time.
The path which such visionaries followed was by no means easy since members of the old guard fought them at every turn.
Were it not for the generous support private wealthy patrons gave to these innovators, timely scientific breakthroughs would have been lost.
Since Galileo's days, modern society unfortunately has made little progress in facilitating the funding of new ideas.
Today's institutionalized funding process consistently rewards conventional thinkers and works against the maverick whose research starts from a different hypothesis.
Even the most rigorous standards and most carefully wrought data cannot overcome the resistance built into the peer review system.
Consequently most work carried out in today's research institutions tends to be traditional, rather than innovative.
The Starburst Foundation was formed to circumvent this problem.
Starburst needs funds to support ongoing scientific research activities spanning many disciplines.
Money is also needed to finance our research, participation in scientific conferences, information networking with government and research organizations around the world, public lectures, and video documentary production.
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