Line 18 a3w Thermal Equilibrium Neutrons Maxwell–Boltzmann Distribution UFO 5g WOW SETI

Maxwell–Boltzmann distribution gases colliding diagram

Line 18 a3w Thermal Equilibrium Neutrons Maxwell–Boltzmann Distribution UFO 5g WOW SETI

5g force ufo engine acceleration plasma formulas

part 134 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 17 2012 11 40 am est

My Thoughts

Key words “kinetic energy” “temperature” “
“moderation” “neutron” are in this section.

They appear in lots of other wow seti lines as well.

Same with the word inelastic and excited state.

Again were looking at ways to cool the Neutrinos and then convert them into energy so we can use that formula to travel faster than the speed of light and reach the goal of 5g force for the UFO Engine acceleration speed.

Another thing now that I know it takes so much FUEL for them to rocket up INTO outerspace. I”m going to look at ways to conserve that energy requirement and find test results that can be used to lengthen the duration of burning time of the said fuels or create new “green” energy that burns cleaner, slower and lasts much longer…

Kinetic energy is transferred between particles.

Feb 17 2012 12 20 pm est

My thoughts

This phrase is standing out here.

If we can create kinetic energy with the neutrinos then we can transfer that “faster than the speed of light energy field” into another particle?

So what particle does the neutrino like? A muon?

Let me see if possible.

Yes it is and it also mentions “leptons”

Another main key word in the wow seti lines of data.

I’ve split this module into part two because I found out that we can do things with the Neutrinos + Muon + Split + Energy = Acceleration Plasma for a UFO ENGINE. Watch this next video to see what i’ve come up with for another formula idea to get 5g force acceleration speed…

Line 18 a3w2

Deuterium – I remember this key word and It’s found on:

Line 18 a3w Thermal equilibrium Neutrons Maxwell–Boltzmann distribution Leptogenesis WOW SETI

Line 18 a3z2 (to be titled)

Deuterium means something with Uranium 238 so I’ve split that module into it’s own because I have another formula idea coming up. See:

Line 18a3w3

My thoughts

Feb 17 2012 12 52 pm est

I’m searching the key words Thermal + Neutron

A set of key words I’ve come across in the wow seti data.

Thermal + Neutron shows up in

Go to the light (not yet filmed or numbered)

Line 15a, 22, 18u, 18fy, 18j, 18m, 18a3m, 18a3r, 18a3w, 18a3x,18a3y

When i do a cross reference i’ll look to see if there’s formulas in these videos.

It will probably mean to Mix them together if there is…
Decay of heavy Majorana neutrinos using the full Boltzmann equation including its implications for leptogenesis
by Anders Basboll, Steen Hannestad
Physics › Miscellaneous Papers
Save PDF to library
Share
• Overview
• Related research
Journal of Cosmology and Astroparticle Physics (2006)
Volume: 01, Pages: 11
• DOI: 10.1088/1475-7516/2007/01/003
• arXiv: hep-ph/0609025

Available from arxiv.org

Such a collision is inelastic, since some of the kinetic energy is transformed to potential energy by exciting some of the internal degrees of freedom of the nucleus to form an excited state.

As the energy of the neutron is lowered, the collisions become predominantly elastic,

Given the mathematics of elastic collisions, as neutrons are very light compared to most nuclei, the most efficient way of removing kinetic energy from the neutron is by choosing a moderating nucleus that has near identical mass.

Neutrons
Atomic Nucleus
Binding energy
Isotopes
Nuclear reactions
Nuclear fission
Nuclear fusion
MeV
Kinetic Energy
Temperature
Inelastic
Scattering cross section
Collissions
Moderator
High energy
Excite nucleus
Potential energy
Internal degrees of freedom
Excited state
Elastic
Kinetic energy
Mass
Neutron
Nucleus
Thermal equilibrium
Hydrogen nuclei
Motion
Particles
Protons
Velocity
Maxwell–Boltzmann distribution
Fission energy
Light water
Heavy water
Low mass
High scattering cross section
Low absorption cross section
Kernels
Energy decrement
Number of crushes
Hydrogen
Deuterium
Beryllium
Carbon
Oxygen
Uranium
The speed of the neutron
Thermal motion
Thermal neutron
Thermalization
Equilibrium
Reactor moderators
Heavy fuel element
Slow moving free neutron
Fission products
Splits fissions
Atoms
Speed of light
CANDU reactor
pressurized water reactor (PWR)
supercritical water reactor (SCWR)
uranium-238
plutonium-beryllium
spallation sources

Decay of heavy Majorana neutrinos using the full Boltzmann equation including its implications for leptogenesis
by Anders Basboll, Steen Hannestad

Gases
Velocity
Thermal + Neutron shows up in

Go to the light (not yet filmed or numbered)

Line 15a, 22, 18u, 18fy, 18j, 18m, 18a3m, 18a3r, 18a3w, 18a3x,18a3y

quote

Moderation
Neutrons are normally bound into an atomic nucleus, and do not exist free for long in nature.

 kinetic energy, E, can be related to temperature 

Moderation is the process of the reduction of the initial high kinetic energy of the free neutron. Since energy is conserved, this reduction of the neutron kinetic energy takes place by transfer of energy to a material known as a moderator.

It is also known as neutron slowing down, since along with the reduction of energy comes a reduction in speed.

Such a collision is inelastic, since some of the kinetic energy is transformed to potential energy by exciting some of the internal degrees of freedom of the nucleus to form an excited state.

As the energy of the neutron is lowered, the collisions become predominantly elastic,

Given the mathematics of elastic collisions, as neutrons are very light compared to most nuclei, the most efficient way of removing kinetic energy from the neutron is by choosing a moderating nucleus that has near identical mass.

Pasted from

Feb 17 2012 11 40 am est

My Thoughts

Key words “kinetic energy” “temperature” “
“moderation” “neutron” are in this section.

They appear in lots of other wow seti lines as well.

Same with the word inelastic and excited state.

Again were looking at ways to cool the Neutrinos and then convert them into energy so we can use that formula to travel faster than the speed of light and reach the goal of 5g force for the UFO Engine acceleration speed.

Another thing now that I know it takes so much FUEL for them to rocket up INTO outerspace. I”m going to look at ways to conserve that energy requirement and find test results that can be used to lengthen the duration of burning time of the said fuels or create new “green” energy that burns cleaner, slower and lasts much longer…

system at thermal equilibrium, neutrons (red) are elastically scattered by a hypothetical moderator of free hydrogen nuclei (blue), undergoing thermally activated motion.

In a system at thermal equilibrium, neutrons (red) are elastically scattered by a hypothetical moderator of free hydrogen nuclei (blue), undergoing thermally activated motion.

Kinetic energy is transferred between particles.

As the neutrons have essentially the same mass as protons and there is no absorption, the velocity distributions of both particles types would be well-described by a single Maxwell–Boltzmann distribution.

Pasted from

Kinetic energy is transferred between particles.

Feb 17 2012 12 20 pm est

My thoughts

This phrase is standing out here.

If we can create kinetic energy with the neutrinos then we can transfer that “faster than the speed of light energy field” into another particle?

So what particle does the neutrino like? A muon?

Let me see if possible.

Yes it is and it also mentions “leptons”

Another main key word in the wow seti lines of data.

I’ve split this module into part two because I found out that we can do things with the Neutrinos + Muon + Split + Energy = Acceleration Plasma for a UFO ENGINE. Watch this next video to see what i’ve come up with for another formula idea to get 5g force acceleration speed…

Line 18 a3w2

Deuterium – I remember this key word and It’s found on:

Line 18 a3w Thermal equilibrium Neutrons Maxwell–Boltzmann distribution Leptogenesis WOW SETI

Line 18 a3z2 (to be titled)

Deuterium means something with Uranium 238 so I’ve split that module into it’s own because I have another formula idea coming up. See:

Line 18a3w3

Quote:

Distribution of neutron velocities once moderated
After sufficient impacts, the speed of the neutron will be comparable to the speed of the nuclei given by thermal motion; this neutron is then called a thermal neutron, and the process may also be termed thermalization.

Once at equilibrium at a given temperature the distribution of speeds (energies) expected of rigid spheres scattering elastically is given by the Maxwell–Boltzmann distribution.

This is only slightly modified in a real moderator due to the speed (energy) dependence of the absorption cross-section of most materials, so that low-speed neutrons are preferentially absorbed,[3][4] so that the true neutron velocity distribution in the core would be slightly hotter than predicted.

Pasted from

My thoughts

Feb 17 2012 12 52 pm est

I’m searching the key words Thermal + Neutron

A set of key words I’ve come across in the wow seti data.

Thermal + Neutron shows up in

Go to the light (not yet filmed or numbered)

Line 15a, 22, 18u, 18fy, 18j, 18m, 18a3m, 18a3r, 18a3w, 18a3x,18a3y

When i do a cross reference i’ll look to see if there’s formulas in these videos.

It will probably mean to Mix them together if there is…

Google
 Maxwell–Boltzmann distribution
The Maxwell–Boltzmann distribution describes particle speeds in gases, where the particles do not constantly interact with each other but move freely between short collisions.

It describes the probability of a particle’s speed (the magnitude of its velocity vector) being near a given value as a function of the temperature of the system, the mass of the particle, and that speed value. This probability distribution is named afterJames Clerk Maxwell and Ludwig Boltzmann.

The Maxwell–Boltzmann distribution is usually thought of as the distribution for molecular speeds, but it can also refer to the distribution for velocities, momenta, and magnitude of the momenta of the molecules, each of which will have a different probability distribution function, all of which are related.

Unless otherwise stated, this article will use “Maxwell–Boltzmann distribution” to refer to the distribution of speed

Pasted from

James Clerk Maxwell

Ludwig Boltzmann

Decay of heavy Majorana neutrinos using the full Boltzmann equation including its implications for leptogenesis
by Anders Basboll, Steen Hannestad
Physics › Miscellaneous Papers
Save PDF to library 
Share
• Overview
• Related research
Journal of Cosmology and Astroparticle Physics (2006)
Volume: 01, Pages: 11
• DOI: 10.1088/1475-7516/2007/01/003
• arXiv: hep-ph/0609025

Available from arxiv.org
or Find this paper at:

Abstract
We have studied the two-body production and decay of a heavy, right-handed neutrino to two light states using the full Boltzmann equation instead of the usual integrated Boltzmann equation which assumes kinetic equilibrium of all species.

Decays and inverse decays are inefficient for thermalising the distribution function of the heavy neutrino and in some parameter ranges there can be very large deviations from kinetic equilibrium.

This leads to substantial numerical differences between the two approaches. Furthermore we study the impact of this difference on the lepton asymmetry production during leptogenesis and find that in the strong washout regime the final asymmetry is changed by 15-30% when the full Boltzmann equation is used.

Pasted from
Google Leptogenesis
In physical cosmology, leptogenesis is the generic term for hypothetical physical processes that produced an asymmetry between leptons and antileptons in the very early universe, resulting in the dominance of leptons over antileptons. The analogous mechanism for baryons is called baryogenesis.

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