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Introduction[redigera | redigera wikitext]

This article is an effort in describing some basic considerations with regard to fusion power and its creation. The focus is however not only on fusion power alone but on understanding related physical phenomena such as for instance pressure.

Plasmas in nature[redigera | redigera wikitext]

The Saha equation states

,

where ni is the ion density and nn is the neutral atoms density and Ui is the ionization energy of the gas.

Putting for ordinary air

gives

which is ridiculously low.[förklaring behövs]

The ionization remains low until Ui is only a few times kT.

So there exist no plasmas naturally here on earth, only in astronomical bodies with temperatures of millions of degrees.

Basic considerations[redigera | redigera wikitext]

When there is a moving particle of charge in a magnetic field, the following equation applies:

A simple way of solving this equation is to put

The equation then becomes

While only considering the magnitude we get

and while v=wr we get

where wc is called the cyclotron frequency and rL is called the Larmor radius.

This means that a particle will gyrate around the lines of force with the cyclotron frequency and the Larmor radius.

This is the most fundamental reason why a plasma can be confined by a magnetic field.

Energy and temperature of a plasma[redigera | redigera wikitext]

It will later on be shown that the average energy may be written

where there is an additional kT/2 for each degree of freedom (whatever that means).

The speed is then

The above energy equation can be derived while using the Maxwellian velocity distribution function

where the volume particle density can be calculated using

which gives us

What this means is that while the most probable speed is when

there are particles with both lower and higher speeds that has the same temperature (my[vem?] guess).

Some ITER calculations[redigera | redigera wikitext]

According to Francis F. Chen, physicists use

to avoid confusion.

Let's state some constants:

With the thankful aid of the_wolfman I also have some actual data for the ITER tokamak

The temperature of the plasma is then

or some 100MK.

Using EAV which is repeated here for convenience

and the fact that Deuterium consists of one proton and one neutron while the neutron mass is almost the same as that of a proton we may use

We then have

or some 1000 km/s

And B=5T gives

or 2mm(?)

and

or 480Mrad/s

If the fusion products are protons and of some 10MeV of energy then

and

Where rL still is quite small...

The magnetic flux density of a short solenoid is

which using R=2m and B=5T gives

Considering some ten turns per coil for minimum resistive losses gives some 2 MA which verifies the above.

Deriving the magnetic flux density of a current loop[redigera | redigera wikitext]

This picture describes the derivation of magnetic flux density due to a current loop

From Maxwell's equations we have

which may be rewritten as

where A might be an arbitrary vector.

Using the vector magnetic potential

and realising that

we have from Biot-Savat law

Defining

and

and

and realising that the r-part cancel out we get

or

Drifts in a plasma[redigera | redigera wikitext]

Using

and putting the left side to zero while taking the cross product with B we obtain

The transverse components of this equation are

and the magnitude of this guiding center drift is

Realising that

one could set

where F might be

due to an E-field or

due to gravity or

due to the centrifugal force while a particle is moving along the lines of force.

Then the drift due to E will be

This picture shows how an E-field would interact with a B-field to change the particle orbit.

This picture describes what happens to a particle when the magnetic field is non uniform.

and the drift due to gravity will be

This graph describes the centrifugal drift in a plasma.

and the drift due to a curved B-field will be

It is interestingMall:According to whom to note that

It is harder to derive and explain the drift in a nonuniform B-field where the force may be written

where vp denotes speed perpendicular to B.

Which put into the force-formula above gives the guiding center drift

which can be generalized to

which is the grad-B drift or the drift caused by inhomogeneities in B.

It can therefore be shown that the total drift in a curved vacuum field is

Here I quote Francis F. Chen:

"It is unfortunate that these drifts add. This means that if one bends a magnetic field into a torus for the purpose of confining a thermonuclear plasma, the particles will drift out of the torous no matter how one juggles the temperature and magnetic fields"

The plasma as a fluid[redigera | redigera wikitext]

If we consider a plasma as a fluid we have

where it can be shown that the two terms to the left may be omitted.

If we then take the cross product with B we have

or

where one term has been deliberatelly omitted.

Rearranging the above yields the total perpendicular drift in a plasma considered as a fluid

where the so-called diamagnetic drift is

where the force is

meaning the gradient of the pressure

to volume particle density.

For an isoterm plasma we have

Inductance Calculation[redigera | redigera wikitext]

The definition of inductance, L, is:

Using

for a long solenoid

or

for a short solenoid it is clear that the adequate formula depends upon diameter versus length. But in many cases the reality is somewhere in between.

Anyway, the inductance of our short solenoid is:

Estimating A to be circular then

And with N=10 and R=2m this yields

Visualising some ten coils around the tokamak which may be connected in series yields some

and to make things complete

This inductance does however only affect power-on. With a smoot onset of voltage (read Amps) the inductance does not matter so much as the resistive losses. But it is interesting to keep this in mind anyway. After all, we are talking MAs here...

I will get back to this later on.

Drift considerations in a plasma[redigera | redigera wikitext]

Getting back to our general B-formula for a short solenoid which is repeated here for convenience

we can see that the magnetic flux density diminishes as

along the

which in our case is "almost" equal to the

This however creates a gradient in B but this gradient is mostly along the B-field.

So even though B lessens with distance to the next coil the grad-B drift might be negligible due to the curl of grad-B with B.

The tokamak current[redigera | redigera wikitext]

This picture is mainly for fun i.e. it reflects the initial condition of a differential equation.

It is preliminary considered that SW1 and SW2 are closed at different times and in such a way that they never are closed at the same time. The voltage source E is preliminary considered stable as a battery.

For the tokamak current, It, we may write

[where the charge q stored by C has been converted to an equivalent voltage because of C=Coulomb/Volt=As/Volt]

Putting

(The sign of this one is a bit hard for me[vem?] to understand but maybe one can view it like the current coming out of the capacitor is leaving the capacitor, therefore the minus sign.)

and deriving once more gives

or

Putting

and

gives the characteristic equation

where

And if

the solution may be written

Using the initial values

and

[This initial value is however a bit hard to understand. But it must come from

where E is the capacitor voltage at t=0 and not the induction of the current derivate. In short, E/L forces the current derivate at t=0 in this case and the valid sign comes from the schematic above.]

then

yielding

so now we have

Deriving this while putting t=0 yields

thus

and finally

This graph is just a fictuous solution to a differential equation

If we derive this and put it equal to zero in search of maximum, one gets:

or

or

The strange thing here is that while r1 needs to be greater than r2 for making the current above positive, my[vem?] result actually indicates that only if r1 is less than 2,71 times r2, tmax is positive.

Here we[vem?] could put tmax into i(t) to calculate maximum current. We won't however do that because that is just plain algebra. It is however interesting to view i(t) in another way referring to the definition of r1 and r2 above

To make things complete regarding solutions for second order differential equations we[vem?] have two more conditions to regard. If

then

If

then

and this makes

which gives the solution

Here we can see that the current is attenuated sinusoidally by the frequency and the "amplitude"

To summarize, all the above solutions are based on the critical condition that

where b should be equal or greater than w to yield a stable response.

Finally, let's do calculate Imax just for fun :)

Using

we get

Supply current[redigera | redigera wikitext]

This basic part doesn't really need a mathematical derivation because one could easily write

It is known that

.

The differential equation of first order may be written

Now we know the solution but we could pretend that we doesn't and guess

Then

Boundary values say that

and

this one is however somewhat tricky but comes from

where

While there are three unknowns, we[vem?] need a third condition which is

Using these boundary conditions, one first gets

and

Then we have

Differentiating this yields

and

which gives

thus

Finally, deriving this and using the capacitor formula for the current gives

Standard model[redigera | redigera wikitext]

  1. electron and positron ("anti-electron")
  2. muon and anti-muon
  3. tau and anti-tau

Along with these comes their neutrino and anti-neutrino which gives six distinct types of particles or:

  1. electron
  2. electron-neutrino
  3. muon
  4. muon-neutrino
  5. tau
  6. tau-neutrino

The neutrinos are preliminary massless and thus very hard to detect.

The dominant three of these are fundamentals and consist of quarks. For our purposes it is enough to recognize two types of quarks namely the up-quark and the down-quark. This is due to the fact that a neutron consists of two down-quarks and one up-quark while a proton consists of two up-quarks and one down-quark.

As mentors at PF have explained, a neutron can undergo weak interaction (transmutation) and be converted to a proton releasing an electron and an anti-neutrino. This has to do with the fact that a quark can change its type/flavor. In this case one down-quark "only" has to change to one up-quark to make the change of the particle.

It has also been explained how a proton can be changed to a neutron in a similar manner.

This is the basic reason for all those protons at the birth of a star like our Sun can generate neutrons and thus Deuterium to actually start the fusion process to Helium.

Radiation particles[redigera | redigera wikitext]

1) Beta-particle (electron)

2) Alpha-particle (ordinary Helium_4 nuclei)

3) Gamma-rays (high energetic photons emitted from the nuclei)

4) X-rays (slightly lower energetic photons emitted when electrons are decelerated or accelerated)

Bohr model[redigera | redigera wikitext]

The other day I came to the conclusion that in the solar plasma, there are both protons (ionized hydrogen atoms), neutrons and excited as well as neutral hydrogen atoms.

The different kinds of hydrogen are being hit all the time by high energetic particles such as the protons and probably, by collision, even the neutrons.

This in turn excites the hydrogen to different levels, as well as being ionized to a proton.

Omitting that the proton itself also may recombine with an electron to form hydrogen again, it is fair to say that the different levels of excitation (i.e. different orbits) gives rise to several possibilities for quantum leaps.

If for instance one has three orbits (n=1–3), the leaps could be made from 3→2, 2→1 and 3→1.

And while the orbital energy for hydrogen may be written:

and

this means that the first leap has the smallest energy difference, the second the next smallest and the third the highest.

This also means that several kinds of color/photons is sent out from the Sun.

I don't know how many excitation levels hydrogen has, but the above leads to two conclusions:

  • n is large, giving several orbital energy states and lots of "recombination possibilities" and thus emitted colors all over the spectra making the Sun "yellow".
  • Excited hydrogen atoms as well as neutral Hydrogen atoms is abundant in the Sun. Because if they were not, no light would appear.

The above is however not true (but the mechanism is). A colleague of mine told me[vem?] that the visible light from the Sun is due to heat only. I[vem?] asked him why and he said that heat itself emits light in a totally different manner.

I recognize a formula like this:

which I think is a derivate of the Stefan-Boltzmann radiation law.

I[vem?] actually used this relationship when I did a rough but rather accurate estimation of the Sun's temperature.

Anyway, I[vem?] asked my colleague what made the radiation then. He answered that it was due to the electrons being decelerated due to collisions while being heated up. Which may be compared to how X-rays above are generated.

Copied from Wikipedia:

"Thermal radiation is electromagnetic radiation generated by the thermal motion of charged particles in matter. All matter with a temperature greater than absolute zero emits thermal radiation. When the temperature of the body is greater than absolute zero, interatomic collisions cause the kinetic energy of the atoms or molecules to change. This results in charge-acceleration and/or dipole oscillation which produces electromagnetic radiation, and the wide spectrum of radiation reflects the wide spectrum of energies and accelerations that occur even at a single temperature."

The question now is however how charge-accelerations or dipole oscillations actually makes light.

Here I'm simply stating Planck's Law:

Where B is the spectral radiance.

Viewing the beautiful picture at Wikipedia of this function it is amazing, to say the least, that it fits so perfectly with the temperature of the Sun.

And to make things complete, the Wien Displacement law:

where b˜3*10−3 [mK]

Being the amateur that I am I would say that this equation is used to determine the temperature of stellar objects.

Thermal radiation[redigera | redigera wikitext]

I have understood that there are more ways to generate light. The mechanism I am thinking of is thermal radiation and reading about this in Wikipedia took me so far as to charge-acceleration and dipole oscillation.

While surfing around in Wikipedia I[vem?] got to remember that light is a TEM-wave.

Being an electrical engineer, I began to think:

where

which both means that jw is a derivation operator for any stationary signal and that the current and the voltage is 90 degrees out of phase in an inductor.

If one considers the Bohr model and the Bohr radius rB we have an orbiting moving charge (at a constant speed) which by definition is equal to current.

Now, the magnetic flux through a coil of area S may be simplified to

Where N=1 for our orbiting electron and lm is the length of the magnetic path.

Faraday law[redigera | redigera wikitext]

states the emf-induction due to magnetic flux change.

And the relationship

leads back to my first formulas.

Viewing these equations, one has both B and E 90 degrees out of phase.

Considering the differential version of Faraday's law we have

which also states the direction of it all.

But we all know that for induction to happen the moving conductor has to cut the lines of force.

So this is by definition a TEM-wave.

The speed of the (circulating) charge need however to be non-constant (otherwise no induction can be made) which means that we have to accelerate the charge by for instance heat.

Considering

from below we note that v is constant within the Bohr radius.

So the only way of increasing the speed of the electron is to move it up to another shell.

In other words, linear thermal radiation cannot be achieved by heating.

Planck's law of radiation must be due to another phenomena which probably is vibration of the nuclei and/or electron.

Or perhaps the Bohr model is just too simple?

Apart from the Bohr restriction, the conclusion must be that every accelerated charge like above give rise to TEM.

A free accelerated or decelerated charge might suit even better for this reasoning. In this case it is more obvious that there are no spectral lines when it comes to thermal radiation and this is because of the "linear" speed states while adding kT.

Bohr model derivation[redigera | redigera wikitext]

While I love to simplify things as much as possible the Bohr model suits my way of trying to understand.

It has been proven that

which means that the length of the electron orbit has to be an integer number of times the wavelength.

With the use of the de Broglie wavelength

and

the above equation may be rewritten as

Referring to the basic force relationship where the centrifugal force is equal to the electromagnetic force we may write

where

Solving for v yields

Integrating the electromagnetic force gives the potential energy as

The kinetic energy may as usual be written

Adding Ep with Ek with the use of the expression for v above then yields

Now,

Solving for r yields

For n=1 this is called the Bohr Radius and for Hydrogen it can be shown that this is some 0,5Å.

Using this equation and the above expression for speed gives

which shows how speed is descretely depended on shell number (n).

For optional atom you may view k as kA where A is the atom number (this is however not true in real life).

Proton-proton fusion[redigera | redigera wikitext]

1) Protons fuse

2) One proton is transmuted into one neutron forming Deuterium (releasing one positron and an electron-neutrino).

3) Deuterium fuses with another proton (which also releases gamma-rays)

4) Two of the resulting Helium_3 neclei fuse

5) An Alpha particle (Helium_4) forms with the energetic release of two protons to complete the process.

A fun quote by Arthur Eddington:

"I am aware that many critics consider the stars are not hot enough. The critics lay themselves open to an obvious retort; we tell them to go and find a hotter place."

Pressure[redigera | redigera wikitext]

I have come to know two types of pressure

1) Gravitational pressure (GP)

2) Plasma pressure (PP)

Gravitational pressure may be written

and plasma pressure

There is actually no difference in units here but I like to keep them separated.

is the density with regard to weight per cubic meter, n is the density with regard to number of particles per cubic meter.

It is important to state that difference because density will be used for both cases.

Pressure in practice[redigera | redigera wikitext]

Normal air pressure (1atm) is

This only means that we humans have adapted to 1 kg/cm2 and nothing else (except that it all implies an actual atmosphere).

This fact was very strange to me but if you think about it, there are fishes that live and survive deep down in our seas.

And while pressure increases with 1atm for every 10m of water depth, it is amazing that they can survive down there.

But it is equally strange for the fish.

Neither of us can survive in our disrespectively pressurized environment.

And what we actually feel is not this ambient pressure but the difference.

Water depth aside we may also create a pressure difference by moving an object in a fluid:

This equation says that as soon as we have a fluid we will create a pressure on it simply by moving it.

While we do not feel one whole kg/cm2 we feel as little increase as 1 meter under water (+1hg/cm2).

And we only have to dive a couple of 10 m below the water surface before we get drunk due to nitrogen "poisoning" which is the reason why scuba divers breath Helium instead of Oxygen at these depths.

The pressure at the deepest part of our sea is about 1000 atm but this is only felt if we as humans (needing 1 atm) would want to visit that place (which some have done in spite of all). The interesting part is that the vessel hull will have to withstand the above pressure equal to an elephant standing on a dime.

The barometric formula

reflects the air pressure at different heights (p0 being 1 atm)

This formula is approximately accurate up to some 10 km (where it actually equals 0).

Anyway, is not linear above some 5 km where

should be used instead (m simply is the molecular weight).

The atmosphere is not uniform. There are four districtive layers or spheres (defined by temperature):

4) Thermosphere (80 km-Karman Line)

3) Mesosphere (50–80 km)

2) Stratosphere (10–50 km)

1) Toposphere (<10 km)

Where the Karman line is 100 km, specified as the height at which a vessel needs to fly as fast as orbital speed to keep height.

Orbital speed means the speed where the centrifugal force equals the gravitational force.

The atmosphere is thus as high as 100 km. I have always thought some 10 km.

Tokamak pressure[redigera | redigera wikitext]

Below follows an attempt in calculating the ITER Tokamak pressure based on data so thankfully given to me by the_wolfman.

using this imaginary part

and the area is thus

where C is some 10m(?) which would give

And the magnitude of F above is

Using protons only with a B of 5T and a kT of 10keV

we have

and thus

Now,

Which also is independent of T :)

I wonder what I do wrong.

Plasma pressure[redigera | redigera wikitext]

From the Ideal Gas law we have

where n is the (particle) density.

Listening to the skilled guys in PF forum I would however like to rearrange this law somewhat

While we all know that P has the magic unit J/m3 multiplication with V gives Joule and thus energy.

Work to the gas may be defined as the increasement of the PV-product because then temperature and thus Ek increases.

Work done by the gas may be defined as the decreasement of the PV-product because then temperature decreases.

It is also interesting to note that the work divided by N gives the work done to, or made by, one single molecule. Which in turn gives the temperature and thus speed of that single molecule.

The first law of thermodynamics seems to be

Where Q is the total energy, U the internal energy and W is the work which is positive if work is done by the gas or negative if work is done on the gas.

The internal energy is defined by

Where KE is the kinetic energy and PE is the potential energy.

Now, we know that the kinetic energy is closely related to temperature but what I didn't know is that potential energy is inversely related to pressure.

I got this latter knowledge from Andrew Mason. Simply stated it comes from the fact that low pressure means that the molecules are furher apart and as they are furher apart they do have higher potential energy.

To me this sounded crazy because the (gravitational or electromagnetic) force is stronger the closer molecules are and this would mean a higher potential energy.

But using the simple relationship

made me understand that work actually has to be done to move an object a certain distance against f.i gravity and this in turn tells me that that object then must have a higher potential energy (like mgh or Fx).

It is actually the same when it comes to the Bohr Model but then the potential energy of that certain electron is negative close to the nuclei and zero at infinity. Which only is a definition of coordinates.

Plasma heating[redigera | redigera wikitext]

Quoting the_wolfman:

There are five ways we commonly heat a plasma relevant to fusion:

1) Ohmic heating. You run a current through a plasma and this creates heat due to electrical resistance.

2) Wave heating. We use antennas to inject electromagnetic waves into a plasma. The plasma absorbs these waves and converts their energy into heat. Similar to a how a microwave heats leftovers.

3) Neutral beam heating. We inject beams of high energy neutral particles into the plasma. As the particles collide with the plasma they slow down and their kinetic energy is converted into heat.

4) Compressive heating. When you compress a plasma you do pdv work on it just like any other fluid. This work in turn heats the plasma.

5) Alpha particle heating. If you get fusion to occur, high energy alpha particles are produced. They then heat the plasma as they slow down.

See also[redigera | redigera wikitext]

References[redigera | redigera wikitext]

Sources[redigera | redigera wikitext]

1) David K. Cheng, Field and Wave Electromagnetics

2) Francis F. Chen, Plasma Physics and Controlled Fusion

3) Jan Petersson, Matematisk Analys, Del 2

4) http://hyperphysics.phy-astr.gsu.edu/hbase/hframe.html

[[Category:Plasma physics]]