Line 18 a3x Neutrinos Split Proton Nuclear Chain Reaction UFO 5g WOW SETI

Fission cross section, measured in barns (a unit equal to 10−28 m2), is a function of the energy of the neutron colliding with a 235U nucleus.

SPECTRUM OF SOLAR-NEUTRINO ENERGIES is plotted with curves showing the sensitivity of the 37Cl detection system now in use (solid line in color)

Line 18 a3x Neutrinos Split Proton Nuclear Chain Reaction UFO 5g WOW SETI
Line 18 a3y Fast Neutrinos Reactors CRESST OPERA CNGS CERN UFO 5g WOW SETI

5g force ufo engine acceleration plasma formulas

part 139 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 9 2012 754 pm est

My Thoughts

Neutron Fission of Uranium 238, fast reactor produces fast neutrons (neutrinos?) to sustain a chain reaction. Add this to a liquid gas formula to achieve the 5G Force Speed?

My Thoughts continued:

We have to look at the data about “elastic” and see if we can add it here to stop the “inelastic scattering that recedes neutron energy.”

Feb 17 2012 11 03 pm est

My thoughts

Based on this data I’ve come up with another formula idea.

Neutrinos + Boron 8 + proton proton Chain reaction + nuclear energy + a 37Ar nucleus + excited state

Feb 17 2012 10 30 pm est

My thoughts

Key words regarding Neutrinos:

The consideration of excited states led to an accurate determination of the probability that 37Cl will capture an 8B neutrino.

plus a positive electron and a neutrino

Arthur M. Poskanzer and his associates at Brookhaven

the fraction of decays of 37Ca that lead to various excited states of 37K.

These were precisely the results needed to calculate the neutrino-capture rate of37Cl with an accuracy of better than 10 percent.

The model predicted that

should decay within 130 milliseconds, on the average, into an excited potassium nucleus the sensitivity of a proposed detection system employing lithium, 7Li

My thoughts continued:

I was surprised to see the word Lithium that’s come up in the actual alien messages of an alloy they use for UFOS

More key words:

The lithium system, however, would be more sensitive than the 37Cl system to neutrinos produced by the pep reaction, 1H + e- + 1H.

Most of the neutrinos expected to be captured by 37Cl are those released by the decay of 8B.

It is convenient to introduce a special unit to express the neutrino-capture rate in solar-neutrino experiments. The unit is the “solar-neutrino unit,” or SNU (which we pronounce “snew”). One SNU equals 10-36 capture per second per target atom.

My thoughts:

According to these test results their saying it takes them roughly six days to capture the neutrinos in a 100,000 gallon tank.

I wonder….

Is there a process that can “speed up” the capture time?

Let’s Google and see.

Quotes:
there are 3 different kinds of neutrinos — electron, mu and tau

The ones that are created in nuclear fusion are the electron version Quantum mechanics is filled with cases of particles doing two (seemingly) mutually exclusive things at the same time.

Experimentally, we have three different kinds of neutrinos: one that interacts with an electron, one that interacts with a muon, and one that interacts with a tau particle.

The energy of a neutrino is, naturally, E=mc^2, which means that if none of the neutrinos have a mass then the energies for all of them are the same and the neutrinos would never change form.

If an electron and a positron (or any other pair) come into contact with one another, they’ll completely annihilate, and in the process, the magic of E=mc^2 turns their mass into a huge amount of energy.

Feb 17 2012 11 00 pm est

I just left a comment on his blog to let him know I’ll be showcasing his article in this video.

Dave features an article about Taylor Wilson. He built a nuclear reactor at age 14.. I wonder if he can help with this neutrino UFO engine idea?

Just a thought…

notes

Line 18 a3y Fast Neutrinos Reactors CRESST OPERA CNGS CERN UFO 5g WOW SETI

Filmed everthing up to green “stopped” my thoughts, tags not on this video need to add to next one. Feb 19 2012 813 pm est

Fission cross section, measured in barns (a unit equal to 10−28 m2), is a function of the energy of the neutron colliding with a 235U nucleus. Fission probability decreases as neutron energy (and speed) increases. This explains why most reactors fueled with 235U need a moderator to sustain a chain reaction and why removing a moderator can shut down a reactor.

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Nuclear Regulatory Commission image of pressurized water reactor vessel heads.

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Quote

This design gives CANDU reactors a positive void coefficient, although the slower neutron kinetics of heavy-water moderated systems compensates for this, leading to comparable safety with PWRs.”[5]

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Quote:

To bring a neutron from the fission energy of E0 2 MeV to an E of 1 eV takes an expected n of 16 and 29 collisions for H2O and D2O, respectively.

Therefore, neutrons are more rapidly moderated by light water, as H has a far higher Σs. However, it also has a far higher Σa, so that the moderating efficiency is nearly 80 times higher for heavy water than for light water.[2]

The ideal moderator is of low mass, high scattering cross section, and low absorption cross section.
Hydrogen Deuterium Beryllium Carbon Oxygen Uranium
Mass of kernels u 1 2 9 12 16 238
Energy decrement ξ 1 0,7261 0,2078 0,1589 0,1209 0,0084
Number of Crushes 18 25 86 114 150 2172

Pasted from

Feb 9 2012 754 pm est

My Thoughts

Neutron Fission of Uranium 238, fast reactor produces fast neutrons (neutrinos?) to sustain a chain reaction. Add this to a liquid gas formula to achieve the 5G Force Speed?

Quote:

Uranium-238 (238U or U-238) is the most common isotope of uranium found in nature. It is not fissile, but is a fertile material: it can capture a slow neutronand after two beta decays become fissile plutonium-239.

 238U is fissionable by fast neutrons, but cannot support a chain reaction because inelastic scattering reduces neutron energy below the range where fast fission is probable.

Pasted from http://en.wikipedia.org/wiki/Uranium-238

My Thoughts continued:

We have to look at the data about “elastic” and see if we can add it here to stop the “inelastic scattering that recudes neutron energy.”

Quote:
Fast fission is fission that occurs when a heavy atom absorbs a high-energy neutron, called a fast neutron, and splits. Most fissionable materials need thermal neutrons, which move slower.

Quote:
Fast neutron reactors use fast fission to produce energy, unlike most nuclear reactors. In a conventional reactor, a moderator is needed to slow down the neutrons so that they are more likely to fission atoms. 

Pasted from http://en.wikipedia.org/wiki/Fast_fission>

Quote

In each cycle two neutrinos are emitted whose maximum energies are greater than 1 MeV. One comes from the radioactive decay of 13N and the other from the decay of 15O.

Pasted from http://www.sns.ias.edu/~jnb/Papers/Popular/Scientificamerican69/scientificamerican69.html

quotes

PROTON PROTON CHAIN is thought to be the dominant source of energy generation in the sun.

The initial proton-proton reaction (1), which produces neutrinos undetectable with37Cl, establishes the basic rate for all subsequent reactions. Detectable neutrinos are released by the “pep” reaction (2), so named because the reactants are proton, electron and proton. Deuterons, 

, produced in these two reactions fuse with protons to form a light isotope of helium, 

 (3). At this point the proton-proton chain breaks into three branches. A few barely detectable neutrinos are produced in the second branch by Reaction 6. The most energetic neutrinos are released (10) in the rare branch involving boron 8.

Moreover, the neutrinos from the decay of 8B can do something that none of the other solar neutrinos can. They are so energetic they produce a 37Ar nucleus that is in an excited state.

This means that the nucleus has more internal energy than it would have in the ground, or normal, state.

The significance of this is that favorable nuclear transitions can be caused by 8B neutrinos that are not possible with the lower-energy neutrinos.

The most important excited state of 37Ar is quite similar to the ground state of 37Cl; it is the nuclear analogue of the ground state of 37Cl.

The consideration of excited states led to an accurate determination of the probability that 37Cl will capture an 8B neutrino.

The chain of argument is based on the symmetry properties of nuclei containing the same number of nucleons and proceeds as follows. The nucleus 

 (I shall again indicate the protons by subscripts) should behave very much like the calcium nucleus 

, which was unknown when I made my nuclear model.

The model predicted that 

 should decay within 130 milliseconds, on the average, into an excited potassium nucleus 

 plus a positive electron and a neutrino. In a nuclear sense this is exactly analogous to the capture of a neutrino by 

, producing 

 plus an electron.

About a year later the isotope 37Ca was observed, and its decay rate was found to be within 25 percent of the value predicted.

More important, subsequent measurements by Arthur M. Poskanzer and his associates at Brookhaven determined the fraction of decays of 37Ca that lead to various excited states of 37K. These were precisely the results needed to calculate the neutrino-capture rate of37Cl with an accuracy of better than 10 percent.

Pasted from

PROTON PROTON CHAIN is thought to be the dominant source of energy generation in the sun. wow seti

quote

SPECTRUM OF SOLAR-NEUTRINO ENERGIES is plotted with curves showing the sensitivity of the 37Cl detection system now in use (solid line in color) and the sensitivity of a proposed detection system employing lithium, 7Li (broken line in color).

Neither system is sensitive in the region below about .8 MeV, where the energies of most of the solar neutrinos would be found. The lithium system, however, would be more sensitive than the 37Cl system to neutrinos produced by the pep reaction, 1H + e- + 1H.

Most of the neutrinos expected to be captured by 37Cl are those released by the decay of 8B. Neutrinos from the proton-proton chain are indicated by solid black lines, neutrinos from the CNO cycle by broken lines. The neutrino fluxes are plotted as the number per square centimeter per second per MeV for continuum sources and as the number per square centimeter per second for line sources.

It is convenient to introduce a special unit to express the neutrino-capture rate in solar-neutrino experiments. The unit is the “solar-neutrino unit,” or SNU (which we pronounce “snew”).

One SNU equals 10-36 capture per second per target atom. This implies that an atom of 37Cl would have to wait 1036 seconds, or roughly 10 billion billion times the age of the observable universe, before capturing a neutrino.

Of course, in the 100,000-gallon tank, which contains about 2 x 1030 atoms of 37Cl, the average waiting time for a single capture when the rate of capture equals 1 SNU is only 5 x 105 seconds, or about six days per capture.

Pasted from

Feb 17 2012 10 30 pm est

My thoughts

Key words regarding Neutrinos:

The consideration of excited states led to an accurate determination of the probability that 37Cl will capture an 8B neutrino.

plus a positive electron and a neutrino

Arthur M. Poskanzer and his associates at Brookhaven

the fraction of decays of 37Ca that lead to various excited states of 37K.

These were precisely the results needed to calculate the neutrino-capture rate of37Cl with an accuracy of better than 10 percent.

The model predicted that 

 should decay within 130 milliseconds, on the average, into an excited potassium nucleus 

 plus a positive electron and a neutrino. In a nuclear sense this is exactly analogous to the capture of a neutrino by 

, producing 

 plus an electron.

and the sensitivity of a proposed detection system employing lithium, 7Li

My thoughts continued:

I was surprised to see the word Lithium that’s come up in the actual alien messages of an alloy they use for UFOS

More key words:

The lithium system, however, would be more sensitive than the 37Cl system to neutrinos produced by the pep reaction, 1H + e- + 1H.

Most of the neutrinos expected to be captured by 37Cl are those released by the decay of 8B.

It is convenient to introduce a special unit to express the neutrino-capture rate in solar-neutrino experiments. The unit is the “solar-neutrino unit,” or SNU (which we pronounce “snew”). One SNU equals 10-36 capture per second per target atom.

My thoughts:

According to these test results their saying it takes them roughly six days to capture the neutrinos in a 100,000 gallon tank.

I wonder….

Is there a process that can “speed up” the capture time?

Let’s Google and see.

there are 3 different kinds of neutrinos – electron, mu and tau

The ones that are created in nuclear fusion are the electron version

 Quantum mechanics is filled with cases of particles doing two (seemingly) mutually exclusive things at the same time.

Experimentally, we have three different kinds of neutrinos: one that interacts with an electron, one that interacts with a muon, and one that interacts with a tau particle.

The energy of a neutrino is, naturally, E=mc^2, which means that if none of the neutrinos have a mass then the energies for all of them are the same and the neutrinos would never change form.

Mu neutrinos, for example, get created by cosmic rays in the upper atmosphere. Electron neutrinos get created by nuclear reactors.

So neutrinos have mass, but, since they’re traveling insanely close to the speed of light, not a lot of it. To give you an idea, the most massive neutrino has a mass probably about ten million times smaller than an electron (the next lightest fundamental particle). 

Pasted from http://io9.com/5859576/whats-the-strangest-thing-about-neutrinos

If an electron and a positron (or any other pair) come into contact with one another, they’ll completely annihilate, and in the process, the magic of E=mc^2 turns their mass into a huge amount of energy.

Pasted from http://io9.com/5818706/where-did-matter-come-from

Dave Goldberg is the author, with Jeff Blomquist, of ”A User’s Guide to the Universe: Surviving the Perils of Black Holes, Time Paradoxes, and Quantum Uncertainty.” 

(follow us on twitter,facebook, twitter or our blog.) He is an Associate Professor of Physics at Drexel University and is currently working on a new book on symmetry.

Feel free to send email toaskaphysicist@io9.com with any questions about the universe.

Pasted from

Feb 17 2012 11 00 pm est

I just left a comment on his blog to let him know I’ll be showcasing his article in this video.

Dave features an article about Taylor Wilson. He built a nuclear reactor at age 14.. I wonder if he can help with this neutrino UFO engine idea?

Just a thought…

37 17 ci

37 18 ar

37 19 k

37 20 ca