Original Message 

From:   John Hoaglund [mailto:hoaglund@essc.psu.edu]

Sent:  Tuesday, September 07, 2004 5:24 PM

Subject:  Energy: a physics primer for a beginning student

 

Eric,

I found some time over the Labor Day weekend to write up some answers to Ryan's questions (we had lousy weather).  This primer is in words only (mostly)!  I wrote a physics and chemistry review for my freshman science classes at the University of Michigan that has more details:

 

http://www.emsei.psu.edu/~hoaglund/physchem/egeocrsp2.html

 

but he can get as much and more from a decent physics or chemistry textbook.  I wrote it though to provide some examples of science in more day to day stuff, often lacking in books that need to be condensed. 

 

Here's my outline for my discussion.

 

I. Intro comments: My advice and opinionated comments on science ed.

II. Where to start.  The four forces, mass, and charge.

III. Thermodynamics: Energy and available energy

IV. Energy supplies

V. Ryan's questions

            1.  How is electricity generated?

            2.  How do solar cells work? (More on electromagnetism and some modern physics)

            3.  What atoms are fused in fusion? How?

 

I.  Intro comments: My advice and opinionated comments on science education.

 

            To answer Ryan’s questions, I need to lay a little ground work.  Before that, some advice (you asked).  Definitely get him involved in the extra curricular (university) stuff for kids, or science camps.  As a parent, obviously support him, but also brace him for the "scientist = nerd" assault he'll endure from our society.  It'll start with his friends teasing him when he tells them he's going to physics camp rather than basketball camp, or because he likes his physics class and asks questions.  Also, when he gets to high school and college, or even before, have him STUDY PHYSICS BEFORE CHEMISTRY, and STUDY CHEMISTRY BEFORE BIOLOGY and STUDY ALL OF THE ABOVE BEFORE GEOLOGY.  You are going to find stubborn resistance to this because it is the complete inverse of the usual progression taught in U.S. high schools.  This idea was championed by Leon Lederman, the previous (or still current?) director of Fermi Lab, in an editorial in the New York Times.  Though one might argue that as a physicist [and a brilliant one] he's presenting a physics bias in the teaching debate, as a geologist, I couldn't agree with him more.  How can you understand the energy and forces involved in chemical bonds if you don't know what energy is (other than in fluffy non-technical terms) because you haven't studied physics yet?  The argument against doing this is that the kids don't have the math background early in their high school career to study physics.  That depends upon how it is presented and whether or not the teacher is willing to teach the needed math as she/he goes.  Also, you're going against the tide and may encounter a few problems.  For example, the physics teacher may assume the kids have a full understanding of what atoms and elements are (from the assumption they had chemistry first) when she/he launches into a discussion of heat energy as atoms vibrating in their chemical bonds.  These problems are surmountable.

 

            Sounds like Ryan has the usual, "yeah, but where does that come from?" questions, and wants to know where to start.  Kids ask the most challenging questions, and it's hard to give easy, yet satisfying, answers to these [so don't conclude that you are "science challenged" for not answering clearly because you're not].  I can't remember who, but some famous scientist (it may have been Einstein) said that if you can't explain what you're doing in science to a 6 year old, you're a charlatan.  Ryan's a little older than that, so I'll try to target his age rather than expose myself as a charlatan.

 

            Following Lederman's advice, I suggest he start with physics.  At the end of the 19th century, it was thought that everything could be explained in terms of Newton's laws (forces in general), thermodynamics, and electromagnetism, what is known as "classical physics."  That may seem quaint, but in actual fact, I dare say 75% of working scientist's research is on, or within topics that can be explained by classical physics, with perhaps some instruments that use modern physics for measurement purposes.  One last piece of advice is that a science student should become very comfortable and fluid in being able to convert measurement units.  So often, a concept may be understood, but a calculation may be off, adding frustration to the study, when in fact the student has the "right" answer in the "wrong" units.  Practice converting "furlongs per fortnight" to "miles per hour" to "meters per second" for velocity, or "cubic furlongs" to "cubic feet" to "gallons" to "liters" for volume.  We lost the Mars Rover to unit screw ups.

 

II.  Where to start.  The four forces, mass, and charge.

 

            My advice on where to start, especially for someone interested in physics, is to start where ALL science starts:  the 4 basic forces.  I wish someone had outlined these for me before I started my science training.  I kept asking myself the, "yeah, but where did that come from?" questions.  It took my college level physics course before I learned that everything is derivable (at least with a hell of a lot of math) from the 4 fundamental forces of the universe and their interactions with matter:  gravity, electro-magnetism, strong nuclear force, and weak nuclear force.  Also remember the measurement unit, Newtons, which is a kilogram of mass multiplied by an acceleration in meters per square seconds.  Currently there are 4 forces in the universe and they just ARE with no reason.  Oh sure, you'll come across a paper now and then with someone claiming they found a 5th force (anti gravity comes to mind), but the forces are where you start.  If you're still asking, "yeah, but why the fundamental 4?" you're getting into philosophy (metaphysics to be exact).  There is a branch of physics trying to relate (i.e. derive) all the 4 forces from some general principles (a "unified field theory"), but where to start there gets into philosophy too:  you have to assume certain things to get started (like particles have fields of energy and momentum that interact, etc.).  Take the 4 forces for granted, start there, and move on.

 

99% of what he'll study in science is derivable from gravity and/or electro-magnetism and their interactions with matter, so let's start there.  There is a beautiful symmetry in these forces, a "makes you wonder." In fact it makes many a cosmologist wonder about the unity (hence unified field theory) of the forces. 

 

Gravity:

F = ( G m1 m2  ) / R2 that is, force = gravity constant (the universal one, NOT Earth's value of constant acceleration due to its gravity) times the mass of the first object times the mass of the second object divided by the square of the distance between them [this is known as Newton's law of gravity].  As for the gravity constant, it's another "just is" that doesn't vary but is now measured and known to the 20th decimal place [originally measured by Cavendish in a really cool experiment].  Any two objects with mass have a force of attraction between them governed by that law.  People are attracted to each other in more ways than one! There is a gravitational force between two people, but it is SO weak compared to their attraction to the Earth (due to the Earth's relatively HUGE mass) that the inter-person force isn't noticed.  This underscores that gravity is the weakest of the 4 forces, and yet gravity is what keeps the planets in their orbits [in fact Newton proved his theory of gravity by showing he could explain Kepler's planetary laws with it].

 

 Electro-magnetism:

 F = ( k q1 q2) / R2 that is, force = Coulomb constant times the charge of the first object times the charge of the second object divided by the square of the distance between them [this is known as Coulomb's law].  As for the Coulomb constant, it's another "just is" that doesn't vary but is now measured and known to the 20th decimal place.  Any two objects with charge have a force between them governed by that law, attractive if the charges are opposite, repulsive if the same.

 

OK, I lied.  That's just the electrostatic force.  The other half, magnetism, is different, but thanks to pioneering work in the late 1800's by James Clerk Maxwell, it is known to be related to the first half, electrostatic [some say Maxwell was the first to "unify" two forces].  Faraday discovered that a moving charge (electric current) induces a magnetic field, and/or a changing magnetic field induces a moving charge (see your electricity generating question below).  But magnetism also has an "inverse square law" like these other forces, called the Biot Savart law, where the magnetic field, B, induced (created) by a moving current (i.e. stream of "moving charges" called electrons) is equal to the magnetic constant times the current divided by the square of the distance from the wire (i.e. the current).  As for the magnetic constant, it's another "just is" that doesn't vary but is now measured and known to the 20th decimal place (all zeros once written in scientific notation because the value is exactly 107 Newtons per square Amps for the purpose of defining Amps).  The magnetic field then induces a force proportional to the magnetic field (so that force decays with the inverse square law along with the decay of the field) on any other magnets or charges.  The magnetic field exerts a 1) force on a magnet according to F = q'B where q' is the "pole strength" of the magnet (a property of the magnet itself), aligning the magnet with its north pole in the direction of the applied magnetic field.  Magnetic field lines come out of the north pole and into the south pole of a magnet, so if the applied magnetic field comes from another magnet, this force wants to align the north pole of the original magnet toward the south pole of the other magnet, which is in the direction of the magnetic field lines.  The "pole strength" property of a material, and why certain materials are magnetic (or magnetizable), is a long topic.  Suffice it to say that magnetism of materials comes from the quantum electron configuations around the atoms in the magnet, specifically unpaired electron "spins" which induce magnetic fields.  That is something that is covered a little more thoroughly in introductory chemistry than in introductory physics.  The magnetic field exerts a 2) force on a charged particle according to F=qv x B ( a charge times its velocity times the magnetic field; the "x" is a special type of multiplication you do with vectors that will be explained in his math / physics courses).

 

Strong nuclear force:

The strong nuclear force holds all those positively charge protons together in the nucleus (against that charge force that wants to repel them) and glues some neutrons in there as well.  These forces are not readily described by single formulas.  The sub atomic experiments haven't yielded a unique or simple formula.  Descriptions of the strong force include that it decays even faster than an "inverse square law" with distance, and that it changes from attractive (come closer) to repulsive (but not too close) as that distance closes.  It is really important though because it is basically the glue of matter.  When two bodies interact (a rock falls and hits another rock), the gravitational force pulling the two bodies together meets the electrostatic force bonding the nuclei together, and the strong nuclear glue force holding each nucleus together.  The solid bodies may smash into pieces (broken chemical bonds), but generally the atoms don't...except subatomic interactions like when a neutron hits a uranium atom causing it to break up and release more neutrons.

 

Weak nuclear force:

The weak nuclear force is responsible for certain instabilities in the nucleus.  Again, there are not simple formulations on it, but it determines why some nuclear configuations are stable (stable isotopes) and others are not (radioactive isotopes), and it's responsible for one of the three types of radioactivity: beta radiation, which is essentially a high energy electron that emanates from the nucleus (as opposed to the orbiting electron shells) turning one of the nucleus' neutrons into a proton [beta radiation is one of two radiations that transmutes (i.e.  changes) one element into another (the transmutation of the elements), the other being alpha decay, which is essentially the loss of a charged helium atom from the nucleus].

 

Mass and charge:

 Now when you get into these definitions of force, you're left with, "yeah, but what is mass, and what is charge?"  If you look up mass, you get, "a quantity of matter measured in relation to its inertia, the ratio of it's weight (a force) to the acceleration of gravity," and when you look up inertia, you get, "the property of matter to stay at rest if at rest or to stay in motion if in motion, unless objected upon by a force."  You're left with, "wait, you just used force to define mass, and you used mass to define one of the 4 forces (gravity).  What gives?"  And with charge, you get, "the departure from electrical neutrality at a point (or region) as by the accumulation or deficit of electrical particles."  So you want to ask, "what are these electrical particles?" and in response you're probably going to get something like, "matter that moves in response to the electrical force." Again, you're left with, "wait, you just used force to define charge, and you used charge to define the force."  It gets worse.  A little pea brain named Albert Einstein showed us that electromagnetic radiation (energy from electromagnetic waves, including radio, heat, light, uv, x-rays, gamma rays, etc.; see energy below) is quantized (in steps), for which he won the Nobel prize in 1905, and that matter and energy are interchangeable, for which he is most famous.  He and other pea brains have shown that matter and energy have particle-like and wave-like properties, and at the atomic level the energy is "quantized" (i.e.  released or absorbed in steps).  Hey, you're there baby!  First principles from basic observations.  Matter stays moving if it's moving or stopped if it's stopped, unless acted upon by a force, and it's only going to get acted upon by gravity if it has mass, and the electromagnetic force if it has charge (and whatever for the strong and weak forces).  And those come from the very root of what we can observe in this material world, stuff moving or not moving, and changing its "moving".  If it's changing its relative motion, it is being acted upon by a force.  If it's not attributable to the 4 known, congratulations, you just discovered another force and will probably win a Nobel prize.  Suffice it to say that whenever a physicist discovers a new particle, the two fundamental questions they want answered are, "does it have mass?" and "does it have charge?"

 

III Energy and available energy

 

            Energy follows from force.  "Work" is a force acting through a distance.  You apply a force to a rock and lift it through a distance (against gravity), performing "work" equal to the force (minimally the rock's weight) times the distance, hence the measurement unit is a Newton meter, also known as a Joule.  Energy is the capacity to do work and overcome resistance, and it has many forms:  heat, kinetic (the energy of motion), gravitational potential, chemical potential, electrical (i.e charge related energy), electromagnetic waves, mechanical (e.g.  sound, water, earthquake...) waves, nuclear, to name a few.  They all have the same measure as work, the Joule.  The rock may have been moved by you (chemical potential energy in your food converted to electrical energy in your muscles, converted to kinetic energy in your arm, transferred to kinetic energy in the rock), or another rock (gravitational potential energy of the other rock converted to kinetic energy of the other rock transferred, upon collision, to kinetic energy in the first rock), etc.  The neat thing about energy is that it is conserved (the first law of thermodynamics), but the not so neat thing is that you gotta get it from somewhere (the second law of thermodynamics).  Remember all that jazz about entropy in Rifkin's book Hydrogen Economy?  Entropy is a measure of the amount of energy UNavailable for doing work in a changing system.  Another way of saying that is that energy is expended from "available" to "unavailable."  The sad news is that (universal) entropy, the amount of energy NOT available, is always either zero or increasing, and is zero only for completely reversible processes (in which case you put as much energy back into it as you got out).  [I say "universal" entropy because between two systems, one system's entropy may be negative and the other positive, but the net (universal) is always 0 or greater.]

 

            If the energy is conserved (1st law), where is it expended (2nd law)?  Whenever energy changes form, there are "losses" which means some is unavailable.  Where does the unavailable energy go?  The "losses" you usually hear about are heat losses that are "dissipated."  See, heat is one of those forms of energy that is useless to us unless we can move it from one system (hot) to another (cold) and extract work in the process.  You can transform all of heat energy into work, but not cyclically.  For example, you can blow off a bomb converting all of the chemical energy into heat energy, and all of the heat energy into gas expansion, but that's it, all over, you're done, it's not cyclic.  In something cyclic, like an engine, you can use the heat to expand a piston, but to get the piston "unexpanded" so you can do it again (i.e. cycle it), you either have to cool it (contracting the gas), phase change the gas into liquid), or put some of the work you got out back in to compress it.  What actually happens is a little of both, you put some of the work you got out with expansion back in with compression (an expanding piston rotates a crank shaft that is helping to re-compress expanded pistons, but the crank shaft is also moving the drive train, for a net gain of work out), and you cool it (with the radiator/cooling system and by "liberating" the heat in exhaust gases), passing the "waste heat" somewhere else.  That heat is dissipated, not useful for the original process.  You may be able to use it in some other process (like heating the car), but again, only if some of it is ultimately dissipated. 

 

[For example, I've always thought that "waste heat" from a power plant, a major pollutant in the environment, should be used to heat homes.  The "waste heat" is hot water at 100 °C left over from when steam at 100 °C transforms into water at 100 °C and releases the latent heat of the phase change.  After steam expansion to turn the turbine, the turbine “exhaust” is still steam.  Steam heating is very common, but this steam has to be condensed to liquid and piped back to complete the power-cycle.  Water is used to cool the condenser and take the heat away.  Still, hot water is hot water, right?  And there's a lot of it near power plants, which is a problem environmentally.  But it takes a lot more work to pump water around than it does steam, and it's amazing how quickly the water loses its heat when piped.  Steam "stores" heat energy as latent heat that is only released with the phase change to water.  That is why the university's heating system uses steam for cross-campus heating.  Piping hot water to homes right near the power plant might work for heating, but the loss of energy pumping it around and from heat dissipation generally makes this uneconomical (i.e.  no net energy).  Not many people choose to live near power plants, but if so, a home, rather than a cold river, is receiving the dissipated heat of the original power generating process, it's just that the "cold" system that you're moving the heat to is your home.]

 

 Rifkin sums it up best with these quotes:

 

 "While energy cannot be created or destroyed, it is continually changing in form, but always in one direction, from available to unavailable."

(page 44), and:

 

"energy is always transformed in one direction:  from hot to cold, concentrated to dispersed, or ordered to disordered." (page 45).

 

IV Energy supplies

Right now, roughly 85% of our "available" energy comes from chemical potential energy, i.e. something is burned: wood, animal dung, coal, oil, and natural gas.  Basically a little energy called ignition [often kinetic energy converted into frictional heat (the striking of a match), or an electric spark (from a battery or car generator) ], is added to some relatively "unstable" chemical compounds (a substance made of two or more elements), breaking the chemical bonds (overcoming the electrical forces of attraction) between them and forming more "stable" chemical compounds and releasing a lot of energy (more than enough to make up for the initial ignition "investment").  The "unstable" compounds require more energy to hold themselves together than the "stable" compounds do, so when the "stable" compounds form from the "unstable" ones, some energy is left over and is released.  Or if you'd rather (and I prefer to think of it this way), the more "stable" compounds require more energy to bust them apart than the "unstable" ones do.  The "unstable" compounds are wood, animal dung, coal, oil, and natural gas, and the "stable" compounds are CO2 and water (both are greenhouse gases).  About 5% of our energy comes from nuclear, and another 5% from hydro, with less than 5% coming from renewables (solar, wind, tidal, etc.).  Kerry's pushing for 20% renewables, but you can see, even that does not solve the problem, and demand is increasing.

 

V.  Ryan's questions:

 

These are a little outside my discipline, but I'll try to give my best shot:

 

“Ryan is really interested in science, chemistry and physics in particular.  He asks me questions like the following:”

 

1.  How is electricity generated? [His dad tells him generally how turbines work, but he wants to know how the electrons move down the wire.]

 

            The rotating turbine is kinetic energy (the energy of motion).  The kinetic energy comes from either falling water, or pressurized stream (from a heat source which is itself either chemical potential energy from burning something, or heat from nuclear fission, or solar, and hopefully someday controlled fusion).  Falling water transfers gravitational potential energy into the kinetic energy of the rotating turbine in a fairly intuitive process.  Alternatively, converting pressurized steam to kinetic energy is not so straightforward.  It is done usually with water/steam in closed loop, in what is known as a Rankine cycle.  The pressurized steam is allowed to expand in the turbine without adding or removing heat.  The expansion of the gas performs what is known as pressure-volume work on the turbine blades.  That work is the conversion to kinetic energy.  Now you've got expanded gas that you need to recompress, and this is the interesting part.  The gas is allowed to convert from gas to liquid in the condensor, which liberates the latent heat of a phase change into heat energy.  This is the heat release part that is needed in any cyclic engine, and at least some of it is dissipated (lost).  In fact, power plants cycle coolant water to take this heat away, and it is the coolant water (not the water in the Rankine cycle) that is cooled in those familiar cooling towers and/or liberated to the environment.  The Rankine cycle water is then brought back to the boiler and re-converted to pressurized steam, completing the cycle.

 

            Now the kinetic energy is converted into electrical energy by rotating a magnet inside a coil of wire.  The rotation is constantly changing the magnetic field through the coil (called a solenoid), which induces a current to flow in the coil wires by Faraday's law (see above).  Moving charges (in the magnetic field) relative to other charges (outside of the magnetic field) causes a change in voltage, a.k.a.  electric potential, between the two sets of charges.  You can think of electric "potential" as the potential energy of a charge to move toward (or away) from another.  It is a change in the electric potential from one point to another point that causes a charge to move (by the electric force) from the point of high potential to the point of low potential.  Because your turbine (rotating magnet inducing charges to move) is moving a hell of a lot of charges, it is making a hell of a lot of potential difference between the outgoing wire and the incoming wire in a circuit.  [The current is always moving in a circuit.  When the circuit is cut, so is the flow of electric current.]

 

            Of course another source of potential difference other than a power plant and rotating magnets is the chemical battery.  In one cell is an anode made of a metal dissolved in a solution of the metal (i.e. has the same metal in it, except it is dissolved).  The solid metal of the anode loses electrons (i.e. is oxidized) and therefore dissolves into its solution.  The anode is thus a source (donor) of electrons, the negative of a battery.  In another cell is a different metal, also dissolved in a solution of itself.  The metal transmits the electrons into the solution of itself where the dissolved metal gains electrons (i.e. is reduced) and deposits on the solid metal.  This acceptor of electrons is called the cathode, the positive of a battery.  There is a "salt bridge" that, in the anode, accepts the excess metal being dissolved, and contributes a salt, to charge balance the anode cell, and in the cathode, exchanges salts with the cathode cell to keep it charged balanced as well.  The result is that if you hook a wire between the anode and the cathode, electrons will flow from the anode to the cathode because of a change in electrical potential between the chemicals.  Eventually too much salt is exchanged for metal and the battery "dies."  Sometimes a little more life can be added to the battery by removing the cathode and scraping off the metal deposits, but even that doesn't work for long.

 

            Now Ryan is asking a great question about what causes the electrons to move down the wire.  The change in electric potential, which is the work needed to move charge toward (or away from) other charge, is like the change in gravitational potential, which is the work needed to move mass away from (or toward) other mass.  The electric force moves the charge from high electric potential to low, just like the gravitational force moves the mass from high gravitational potential to low.  A change in the electric potential can also be thought of as the sum of all the charges accumulated at some distance from a given charge, making the charge want to move because of the electric force.

 

            Now, how easily that charge moves down the wire is the topic of conductivity.  Actually physicists and engineers express it in terms of the resistance to the charge moving down the wire.  There is always some resistance, except for superconductors.  How well something conducts or resists is a long topic.  It mostly has to do with how satisfied the electrons are in the material.  If they are ALL tightly bonded in a nice low energy arrangement, they're not going to want to move, and you are left with a highly resistant material.  In fact it is such a struggle that there is a lot of interaction between the electrons that want to move through and the electrons that make up the material, causing bounces and wiggles (a.k.a.  heat; resistors get really hot).  Metals make good conductors because in addition to the electrons bonding the metal together, there are a whole bunch of "delocalized" electrons, kinda like electrons without a home, that are ready to move on.  Superconducting materials are rare, but they move electrons through them with no resistance.  So far the ones we know of only superconduct at really low temperatures, and it takes a lot of energy to cool them to the point where the superconductivity (with no "heat" losses like in resistors) can pay off against the energy invested to cool them.  Another holy grail in science is to find a "room temperature" superconductor, one that will superconduct at room temperature, and that can be shaped into a wire, or something that can be readily engineered to transmit electric current.  Superconductors are getting "warmer," i.e. better and better materials are being found that superconduct at higher and higher temperatures.  A breakthrough here happened not too long ago when a superconductor was found that could superconduct above the boiling point of liquid nitrogen, making it really cheap to cool.  The search (lab search that is) goes on.

 

 

 2.  How do solar cells work? Again, he wants the specifics.

 

            The term solar cell usually implies photovoltaic (PV) cells.  Before discussing that, I should say that there are three ways to harvest solar energy:  photochemically, photovoltaically, and thermally (and combinations).  I'm not familiar with any commercial photochemical methods, but will just say that plants harvest solar energy photochemically, specifically with chlorophyll in photosynthesis.  I will focus the discussion on photovoltaic and thermal methods.

 

Photovoltaic Solar

            Photovoltaic (PV) cells produce power by photoconduction, producing I, electric current (in amps), a stream of moving electrons, and photovoltage, producing V, voltage (in volts), an electric force per unit charge, or in other words the electric potential.  Power in Watts (energy delivered in a unit time, i.e.  Joule / second) is the combination (product) of the two, P = IV.  Many people mistakenly say that the current is produced photoelectrically (that is electrons are emitted off the surface of the cell), alluding to the photoelectric effect where electrons are known to be ejected off the surface of metals in the presence of light.  While the concept of the photoelectric effect is extremely important in understanding PV cells, the current produced is not from "emitted" or "ejected" electrons, but rather electrons that are "excited" from what is known as the "valence band" to the "conductance band" in a semi conductor solid.  The electrons are "excited" by gaining energy from electromagnetic photons, a concept first proposed by Albert Einstein in 1905 in his study of the photoelectric effect.

 

            Before 1905, electromagnetic (EM) radiation (e.g.  light) was thought to have only wave properties, and those properties were completely described by Maxwell's electromagnetic theory of light.  As a wave of vibrating electric and magnetic fields, the intensity (brightness), which is the energy delivered per unit time per unit area, is just a constant times the square of the electric field, with NO dependence on the frequency (or wavelength) of the light.  This is intuitive: if you want to make a brighter light, add more electricity to increase the E field.  We still use the EM concept of intensity to describe the energy delivered by light (particularly to describe lighting, etc.), but the EM energy absorbed or emitted by matter is a different story.  A phenomenon called the photoelectric effect was discovered by Hertz:  light incident on certain metal surfaces in a vacuum emits electrons.  Lenard observed that the intensity of the light does increase the number of electrons emitted, but not their energies.  Einstein proposed a radical idea to explain the observations of Hertz and Lenard.  Everyone assumed that the energy of those electrons (measured by the voltage needed to repel them) would be related to the intensity.  Einstein proposed that the energies of the electrons were equal to the energy of electromagnetic photons, an energy bearing particle, and that the energy absorbed by the metal and emitted by the electrons was related to the frequency (inversely related to the wavelength) of the light.  This idea, the fact that light has both particle and wave properties, and that the energy received by EM radiation is related to frequency, turned the physics world on its head.  In 1911, Millikan set up an experiment to disprove Einstein, and instead confirmed his hypothesis!

 

            What the result means to solar cells and other phenomena is that the energies absorbed by atomic particles from EM radiation depend on the frequency of the radiation.  You may have heard of ionizing radiation.  Ionizing radiation delivers enough energy to strip electrons from a substance, literally pulling an electron out of an atom's electron orbitals where they are used in bonding compounds.  The first ionizing radiation is ultra violet (uv), the component of the sun's rays that gives you a sunburn.  Ultra violet lamps are used in a lot of chemical detection equipment, like that used by the gas man who checks for gas leaks in a house.  The uv-stripped electrons from the gas are "countable," and the electron count is related to how much gas is there.  In a solar cell, we do not need as much energy as it takes to ionize electrons, just enough to excite them from one part of the solid (the valence band) to another (the conductance band).  In a solid, bonding electrons shared between sets of atoms are in what is known as the valence band.  In a conductor (such as a metal) or in a semi conductor, there is a conductance band where any electrons in the band can move because they are not involved in bonding the solid.  In a conductor, some of the valence band electrons are also in the conductance band.  These electrons are "delocalized" and free to travel.  In a semi conductor, the valence and conductance band are separated by an energy barrier.  If an electron gets enough energy (the "energy gap") it can jump from the valence to the conductance band.  Once an electron is in the conductance band, it is free to travel (conduct on through).  [In an insulator, there is also a conductance band, but the energy required to get there is too extreme, so no electrons conduct.  Under extreme conditions (like extreme heating), electrons may get enough energy, and the insulator may become a semi conductor or conductor.]

 

            It is not enough to just excite electrons into the conductance band.  You also have to provide a voltage to move them.  The way this is done is to "dope" semi conductors with "impurities" [elements that can sub for the dominant "cation" (positively charge element) in the semi conductor crystal] that leave charge imbalances in the structure.  In a solar cell, a positively (p) charged semi conductor is placed in contact with a negatively (n) charged semi conductor along what is known as a p-n junction.  What p-n junctions do is allow charge to move one way across the junction, but not the other way back again.  Photons of light, then, excite electrons across the junction, building up negative charge in the n-semi-conductor and positive charge in the p-semi-conductor (building up voltage).  For a given frequency of dominant electromagnetic radiation (in this case from the sun), there's a certain "energy gap" that balances the right amount of voltage build up (photovoltage) with available electrons (photocurrent).  It turns out the dominant wavelength (inverse of frequency) of our Sun is around 500 nanometers [calculated with Wein's displacement law for a Sun surface temperature of 5800K], green light, with an average wavelength of yellow light (575 nanometers).  The electromagnetic power (energy per time) distribution of the Sun has about 47% in the visible spectrum, 45% in the infrared (heat), and 8% uv [these power distributions are given by the integral (summation) of Planck's law, with the total power output of the Sun given by the Stefan Boltzman law].  The ideal photovoltage/photocurrent balance for this distribution corresponds to an ideal "energy gap" of 1.1 electron volts (another unit of energy used at the atomic scale), with a theoretical efficiency of converting the Sun's power to electrical power of 44%.  The 1.1 electron volt energy gap corresponds to silicon semi conductors, with a practical efficiency of about 30%.  So crystalline silicon semi conductors are the best, but they're expensive to make (you have to grow crystals while doping them).  Some of the solar cell "breakthroughs" lately are in finding cheaper (or cheaper to build) materials to make cells that have efficiencies close to the silicon champions.  The efficiency is critical: the Sun's power output, even at the Earth's surface after going through the atmosphere, is generous [1340 W/m2 total is cut to about 1000 W/m2 on the Earth's surface], but the translation to electric power is cut to 2/3 by the efficiencies.  On my table on my energy page:

 
http://www.emsei.psu.edu/~hoaglund/energyslaves.html

 

I got the day night world averaged solar output of 238 W/m^2, which for an 80 square meter rooftop (a double wide trailer) corresponds to 460 kW-hrs of energy.  Multiply by ~ 1/3 (say 28%), you get 128 kW hrs compared to an average home electric usage of 16 kW-hr.  Clouds screw that up of course, but that's why you store the energy in hydrogen.  Unfortunately 80 square meters of silicon would cost a mint, so now you see the economics driving the race for cheaper-and-as-efficient solar cells.

 

 Thermal Solar

            As the name implies, you can convert a lot of the Sun's output power into heat.  Most of the Sun's spectrum is above (more energy intense) than infrared (heat), and as the higher energy uv waves are absorbed, they re-emit at lower energy infrared (heat) waves.  This is the greenhouse effect: high energy light and uv passes the glass, gets absorbed by the walls and plants, and re-radiates as heat which gets trapped, hence the heat builds up.  Your car is an oven on a summer (or even winter) day, another example.  Thermal collectors are cheap to build (something like glass to transmit light but trap heat), backed with something "black" (as in "Stefan Boltzman black body absorber"), and filled with a heat carrier like water.  The efficiencies of the collectors are great, as high as 75% or more, but once you heat something above the ambient (surrounding) temperature, it starts to radiate heat.  You're also left with a medium you have to pump around (water pumps and plumbing etc.), and to generate electricity, you have all the losses associated with the "cyclic engine" (see power plant discussion above).  Bottom line: great for heating water for a house (and lots and lots of people do just that), but unless collected from reflectors at a large scale to flash steam, not so efficient for producing electric power.

 

Photovoltaic/Thermal Solar (PVT cells).

Remember the ideal "energy gap" for the solar cell is around 1.1 eV?  Well, the sun's average photon energy is around 1.9 eV (in the red part of the spectrum, it's a typical "yellow" sun but the atmosphere plays tricks).  That leaves some extra energy in the cell, which is absorbed as heat.  A PVT is a combo cell, taking the PV out in current, and circulating a medium through it to take the heat.  I'm not sure what their efficiencies are.

 

 3.  What atoms are fused in fusion? How?

 

Fusion versus Fission:  We should start by defining each term and show the energies that are released.  Fusion is the fusing of atoms producing heavier atoms while fission is the breaking up of heavy atoms into smaller ones.  Both processes are radioactive, the difference is that fission leaves radioactive by products, things that continue to release radioactivity, whereas the fusion radioactivity ceases with the cessation of the reaction.  The byproduct wastes remind me of Charles Schultz's Pig Pen from the Peanuts cartoon:  it keeps having this annoying stuff coming off of it.  The radioactivity has 3 forms:  alpha (a helium atom without its electrons), beta (a high energy electron emitted from the nucleus, as opposed to an orbital), and gamma (a high energy electromagnetic wave).  Gammas are the most lethal and require 6 feet of concrete / lead to stop them.  Of the particulate radiation, alphas are the most lethal, but a piece of paper stops them.  Betas can be stopped by a piece of wood.

 

When comparing fission and fusion, you should look at the curve of binding energy.

 

 http://hyperphysics.phy astr.gsu.edu/hbase/nucene/nucbin.html#c2

 

The mass number is the total number of neutrons and protons in the nucleus, leftmost on the graph is light elements like hydrogen and rightmost are the heavy elements like uranium.  Fission works from right to left (towards iron at the peak).  The binding energy is the energy required to break an atom up into its constituents.  If you form an element of a higher binding energy from one with a lower, you release excess energy (that sounds backwards until you think about it).  Compare the fission (right to left) gradual slope versus the fusion (left to right) steep slope.  You can see there is a huge "bang for the buck" with fusion.

 

            The ideal atoms fused in fusion are hydrogen, specifically two isotopes of hydrogen.  Hydrogen has 1 proton.  If it has one neutron as well, it is called deuterium, a "stable" (i.e.  not radioactive) isotope.  If it has two neutrons, it is called tritium, which is a radioactive isotope (but the radioactivity goes away quickly).  Deuterium-tritium fusion results in stable helium (2 protons, 2 neutrons) plus an extra neutron.  The extra neutron goes into breeding tritium from deuterium and/or deuterium from hydrogen.  These things only fuse at really high temperatures and pressures because you need tremendous energy (heat) to overcome the charge repulsion (two plus charges repel) and get the two positively charged hydrogen atoms close enough to become helium.  The Sun does this with gravity, but that's because it is so huge, there's enough mass to compress the hydrogen.  Remember, the repulsion force is related to the inverse of the square of the distance separating them, and as that distance gets smaller and smaller, that force approaches infinity (almost division by zero).  Heating is done with lasers, and pressure is produced with confinement (either magnetic or inertial).  It also takes energy to strip electrons to create a plasma in the first place.  A plasma is all the hydrogen matter stripped of its electrons.  It is basically a 4th state of matter and has its own properties, but being charged, it can be manipulated by magnets for containment and confinement.  Containment is critical because at the temperatures of fusion, no vessel can hold the plasma.  Right now, the technical issue is getting more energy out than what goes in.  The energies for containment, confinement, plasma generation, and heating require more energy than the limited fractions of a second the reaction can be sustained.  When you hear about the occasional "breakthrough," it usually means some lab somewhere has increased (set a new record for) the sustained reaction time (and got more energy out).  I think the record is at the Joint European Torus ( JET);

 

http://www.jet.efda.org/index.html

 

lab in the UK.

 

The helium has slightly less mass than the deuterium and tritium used to make it.  Where did that mass go? It is converted into energy by Einstein's famous E = mc2, which is energy (out) = mass (lost) times the speed of light squared.  That's a hell of a lot of energy out. 

 

One end note: it takes less input energy to fuse slightly heavier elements, and I read a few years back that they were having some success with lithium-lithium or lithium-hydrogen fusion, but it results in some radioactive byproducts which, in my opinion, defeats the purpose.

 

Another end note: the temperatures for fusion in a hydrogen bomb are created by a fission bomb.  It is the fission bomb that results in most of the radioactive by products, not the hydrogen, although fusion itself does release a considerable amount of gamma (electromagnetic wave) radiation and neutrons.  I've heard that one of the technical problems is that the neutrons make reactor equipment brittle over time. 

 

I found this summary of the radioactivity associated with DT fusion:

 

http://www.lanl.gov/p/projects/pds_in15.shtml

 

"The 16.75 MeV gamma rays that accompany DT fusion provide a high bandwidth alternative to 14 MeV fusion neutrons for DT burn history measurements.  Fusion of deuterium with tritium produces an excited 5He nucleus, which then has several possible de-excitation modes.  The most common mode emits a 14 MeV neutron and a 3.5 MeV alpha particle.  Much less frequent gamma ray modes emit gamma rays at 16.75 MeV to the ground state and possibly at ~ 12 MeV to a broad level near 4 MeV.  Recent values for the DT branching ratio (16.75MeV gamma rays per 14 MeV neutron) vary from 5x105 to 1x104."

 

 

John Hoaglund, Research Associate

The Pennsylvania State University

Earth and Environmental Systems Institute

2217 Earth Engineering Sciences

University Park, PA 16802 6813

(814) 865 4792

hoaglund@essc.psu.edu

http://www.emsei.psu.edu/~hoaglund/