Fusion Celestial to Earthbound. A Comparison 1 gallon of seawater=300 gallons of gasoline 1 gallon...
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Transcript of Fusion Celestial to Earthbound. A Comparison 1 gallon of seawater=300 gallons of gasoline 1 gallon...
FusionFusionCelestial to EarthboundCelestial to Earthbound
A ComparisonA Comparison
1 gallon of seawater=300 gallons of gasoline1 gallon of seawater=300 gallons of gasoline 82,459,000 barrels per day in 2005 -> 82,459,000 barrels per day in 2005 ->
1,583,212,800 gallons of gasoline1,583,212,800 gallons of gasoline 5,277,376 gallons of ocean water burned in a 5,277,376 gallons of ocean water burned in a
fusion reactor= 1,583,212,800 gallons of fusion reactor= 1,583,212,800 gallons of gasolinegasoline
5,277,376 gallons of ocean water=1.5E-12% 5,277,376 gallons of ocean water=1.5E-12% of the total volume of the oceanof the total volume of the ocean
Only .015% of naturally occurring hydrogen Only .015% of naturally occurring hydrogen is deuteriumis deuterium
How Does Fusion How Does Fusion Occur?Occur? Two lighter nuclei combine to Two lighter nuclei combine to
form a heavier nucleus coupled form a heavier nucleus coupled with a release of energywith a release of energy
Coulomb BarrierCoulomb Barrier– HeatHeat
Fuel ConfinementFuel Confinement Self Sustaining?Self Sustaining?
– Lawson CriteriaLawson Criteria
The SunThe Sun
Proton-Proton chainProton-Proton chain– BeginningsBeginnings
11H + H + 11H → H → 22H + H + ee++ + + ννee 22H + H + 11H → H → 33He + He + γγ
– pp1pp1 33He +He +33He → He → 44He + He + 11H + H + 11HH
– pp2pp2 33He + 4He→He + 4He→77BeBe + + γγ 77Be + e−→Be + e−→77LiLi + + νeνe 77Li + Li + 11H→H→44He + He + 44HeHe
– pp3pp3 33He + He + 44He→He→77Be + Be + γγ 77Be + Be + 11H→H→88BB + γ + γ 88B→B→88Be + eBe + e++ + + νeνe 88Be↔Be↔44He + He + 44HeHe
The Sun (cont’d)The Sun (cont’d)
Carbon-Nitrogen-Carbon-Nitrogen-Oxygen chainOxygen chain– 1212C + C + 11H→H→1313N + γN + γ– 1313N→N→1313C + e+ + νeC + e+ + νe– 1313C + C + 11H→H→1414N + γN + γ– 1414N + N + 11H→H→1515O O – 1515O→O→1515N + e+ + νeN + e+ + νe– 1515N + N + 11H→H→1212C + C + 44HeHe
Earthbound?Earthbound?
Can’t use gravitational forceCan’t use gravitational force– Must use electromagnetic forceMust use electromagnetic force
Magnetic confinementMagnetic confinement Limited in reaction choiceLimited in reaction choice
– ExothermicExothermic– Low Z nucleiLow Z nuclei
Ignition EnergyIgnition Energy– D-T reaction=100 million degrees D-T reaction=100 million degrees
Celsius Celsius
The ReactionsThe Reactions
(1)D+T→ (1)D+T→ 44He(3.5 MeV)+ n(14.1 MeV) He(3.5 MeV)+ n(14.1 MeV) (2i)D+D→ T(1.01 MeV)+ p(3.02 MeV) (2i)D+D→ T(1.01 MeV)+ p(3.02 MeV) 50%50% (2ii) → (2ii) → 33He(0.82 MeV)+ n(2.45 MeV) He(0.82 MeV)+ n(2.45 MeV) 50%50% (3)D+(3)D+33He→ He→ 44He(3.6 MeV)+ p(14.7 MeV)He(3.6 MeV)+ p(14.7 MeV) (4)T+T→ (4)T+T→ 44He +2 n+ 11.3 MeVHe +2 n+ 11.3 MeV (5)(5)33He+He+33He→ He→ 44He +2 p+ 12.9 MeVHe +2 p+ 12.9 MeV (6i)(6i)33He+T→ He+T→ 44He + p +n+ 12.1 MeV He + p +n+ 12.1 MeV 51%51% (6ii) → (6ii) → 44He(4.8 MeV)+ D(9.5 MeV) He(4.8 MeV)+ D(9.5 MeV) 43%43% (6iii) → (6iii) → 44He(0.5 MeV)+ n(1.9 MeV)+p(11.9 MeV) He(0.5 MeV)+ n(1.9 MeV)+p(11.9 MeV) 6%6% (7)D+(7)D+66Li→2 Li→2 44He+ 22.4 MeVHe+ 22.4 MeV (8)p+(8)p+66Li→ Li→ 44He(1.7 MeV)+ 3He(2.3 MeV)He(1.7 MeV)+ 3He(2.3 MeV) (9)3He+(9)3He+66Li→2 Li→2 44He + p+ 16.9 MeVHe + p+ 16.9 MeV
First StepsFirst Steps
Hydrogen BombHydrogen Bomb Radio-frequency heatingRadio-frequency heating Linear ConfinementLinear Confinement
– Pinch effectPinch effect Magnetic MirrorsMagnetic Mirrors ToroidToroid
– StellaratorStellarator
StellaratorStellarator
ProblemsProblems
Plasma InstabilityPlasma Instability Heat LossHeat Loss
TokamakTokamak
Large toroid that produces a Large toroid that produces a toroidal magnetic fieldtoroidal magnetic field
Charged plasma also creates Charged plasma also creates magnetic fieldmagnetic field
Large external shaping magnetsLarge external shaping magnets Name derived from Russian: Name derived from Russian:
toroidalnaya kamera magnitnaya toroidalnaya kamera magnitnaya katushka katushka
Tokamak (cont’d)Tokamak (cont’d)
Tokamak (cont’d)Tokamak (cont’d)
Tokamak (cont’d)Tokamak (cont’d)
The Big ThreeThe Big Three
TFTR (tokamak fusion test reactor TFTR (tokamak fusion test reactor located at Princeton University) located at Princeton University)
JET (joint European torus, located JET (joint European torus, located in Culham, UK as part of a in Culham, UK as part of a European collaboration)European collaboration)
JT-60 (located in Japan)JT-60 (located in Japan)
ResultsResults
JET reactor produces 16MW of JET reactor produces 16MW of fusion energyfusion energy
TFTR and JT-60 produce around TFTR and JT-60 produce around 10.7 MW of fusion energy10.7 MW of fusion energy
Q values of 0.6-0.9Q values of 0.6-0.9
The FutureThe Future
ITER (international thermonuclear ITER (international thermonuclear experiment reactor)experiment reactor)
GoalsGoals– 400MW fusion energy400MW fusion energy– Q value of around 10Q value of around 10
ConsiderationsConsiderations
SafetySafety– Amount of fuel in reactorAmount of fuel in reactor– Reaction sustainabilityReaction sustainability
WasteWaste FuelFuel
SourcesSources
1)http://www.bp.com1)http://www.bp.com 2)Fowler, T. K. 2)Fowler, T. K. The Fusion Quest, The Fusion Quest, The Johns Hopkins The Johns Hopkins
University Press: Baltimore and London, 1997University Press: Baltimore and London, 1997 3)Braams, C.M.; Stott, P.E. 3)Braams, C.M.; Stott, P.E. Nuclear Fusion: Half a Nuclear Fusion: Half a
Century of Magnetic Confinement Fusion ResearchCentury of Magnetic Confinement Fusion Research; ; Institute of Physics Publishing: Bristol and Institute of Physics Publishing: Bristol and Philadelphia, 2002Philadelphia, 2002
4)http://www.jet.efda.org/pages/focus/006heating/7c-4)http://www.jet.efda.org/pages/focus/006heating/7c-t.jpgt.jpg
5)http://en.wikipedia.org/wiki/ITER5)http://en.wikipedia.org/wiki/ITER 6)http://www.lateralscience.co.uk/latscipics/6)http://www.lateralscience.co.uk/latscipics/
stellarator.jpgstellarator.jpg