Plasma Fusion MAIN3 Final

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    Plasma

    FusionThe energy source of thefuture.

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    What is Fusion?Fusion is a nuclear reaction (a reaction

    involving nucleons). Like chemical reactions,these reactions involve a netrelease/absorption of energy.

    Fusion is the process where 2 small nuclei aremerged to form a lighter particle, and aheavier nucleus.

    A common example, which takes place in the

    sun, is deuterium and tritium forming heliumand a single neutron.

    [1]

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    When this occurs the total mass decreases

    slightly, with connection to nuclear bindingenergy.(1) This is implied by Einsteinsfamous equation, the mass lost must bechanged into energy.

    Typically the atoms to the left ofthe curve release energy from

    fusion, those on the right release

    energy from fission. Iron is the most stable element at

    the top of the curve and is

    effectively inert.[1]

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    What is plasma?A plasma is an ionised gas, known as the

    fourth state of matter.

    This is when the electrons have beendissociated from their nuclei.

    As plasma consists of separated chargedparticles, electric fields are present.

    As the charged particles move, current flows,inducing magnetic fields.

    [2]

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    As a result of these properties, fusion can

    occur within plasmaIf a strong enough magnetic field is applied,

    the nuclei in the plasma can fuse, if this forceis sustained for a long enough time.

    [2]

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    Graph Of Potential

    Energy Between 2Protons

    [3]

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    Why Nuclear Fusion?

    Nuclear fusion could meet the increasing worldenergy demand.

    Fusion produces almost no carbon dioxideemission which is one of the major green housegases

    Fusion is safe.

    Fusion is a sustainable energy source.

    [4,5,6]

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    Fusion & Plasma The

    Perfect MatchThe equation used to calculate the

    temperature for fusion to occur is:

    The ideal fuel for a material at thistemperature is a plasma.

    As fusion will only occur at plasma

    temperatures, its logical for any realisticplasma generators to allow fusion to occur ina controlled, confined plasma. Wherein liesthe main issue.

    kTE

    =2

    3

    [7,8,9,10]

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    Confinement Issues

    Extreme temperatures and the nature of theplasma mean it will try to occupy all availablespace. In this event it will reach the walls

    which is not exactly helpful.If the plasma is moving at any significant

    velocity its momentum and any turbulencethat occurs will increase the chances of the

    plasma reaching the walls.

    [11,12]

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    Fusion Chamber

    [11]

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    Plasma In A Toroidal

    SystemLinear systems were designed but failed

    because they could not effectively contain theplasma.

    This led to the development of the toroidalsystem.

    A toroidal system effectively confines theplasma.

    [12]

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    Spherical Tokamak

    Commercial toroidal shapedfusion chamber in whichplasma is confined

    Plasma is heated to 100million degrees

    Large current required tomaintain the field containingplasma

    Plasma DOES NOT touch wallsof chamber.

    [13]

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    Heating the Plasma

    Currently insufficient energy is produced tomaintain the plasma temperature.

    Device operates in pulses.

    Three ways to heat plasma :

    - Ohmic heating

    - Neutral Beam Injection

    - Radio Frequency Heating

    [14]

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    JET- EFDA

    Joint European Torus European FusionDevelopment Agreement

    Nuclear fusion research organisation

    Aims to realise the use of fusion technology tocreate sustainable energy at economicallycompetitive costs.

    Currently in the development of ...

    [15]

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    ITER

    [13]

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    ITER

    International Thermonuclear ExperimentalReactor

    Latest fusion device that aims to demonstratescientific and technical feasibility of fusionpower.

    To be implemented in a power plant.

    Based on the spherical tokamak concept.The design of device finished in 2006.

    Construction is due to be complete in 2018.

    [13]

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    How IT(ER) works

    Plasma used to fuse hydrogen isotopes

    Torus is covered by a lithium blanket

    Fusion releases high energy neutronsNeutrons are stopped by the lithium blanket

    absorbing energy of the neutrons in theprocess

    This creates heatThis then used to turn a turbine

    [13]

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    History of Fusion

    The inspiration that led to discovering fusioncame from the question Why does the sunshine?

    One of the first major steps in understandingthis was Einstein's E=mc2

    It was first properly formulated in Hans

    Bethes paper Energy production in stars,which led to him winning the Nobel prize.

    [17,18]

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    Experimental

    Development of FusionThe first experiments were carried out in the

    Cavendish laboratory, but it wasnt until afterthe Manhattan project that there was major

    interest in fusion.In the UK many projects were carried out

    including ventures at Imperial College.

    These culminated in the ZETA (Zero EnergyToroidal Assembly) that gave many

    promising results in the period from 1954-1958.

    [17,18]

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    Tokamaks

    After the atoms for peace conference in1958 there was co-operation between theRussians and British, leading to the

    verification and development of tokamaks.The name tokamak comes from (toroidal'nayakamera s magnitnymi katushkami)

    Tokamaks are the basis of the JET and the

    ITER projects.

    [16]

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    Future of FusionWhen the ITER project comes online it is

    expected to run for 1000 seconds with amaximum output of 500MW.

    Beyond ITER a project called DEMO isplanned, which will go 25 times beyondbreakeven point, whereas ITER is only 10times beyond.

    Although progress is encouraging it is likelythat a commercially viable reactor will not berunning before 2050.

    [19,20,21,22,

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    Disadvantages of Fusion

    The release of neutrons will activatematerials, making them radioactive.

    There is also a risk of tritium leaking into

    water systems or the atmosphereWhen plants are deactivated there will be an

    abundance of radioactive waste.

    Due to the high capital costs and necessaryskills it is not a viable option for manydeveloping countries

    [25,26]

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    Energy for the Future?

    Still a technology in the development stages

    It is a long term solution, commercial plantsare not going to be readily available for many

    years.In the mans everlasting quest for more

    energy, is fusion the best solution?

    Looking at these incredulities, it can only be

    realised by the power of the fusion. Thequestion stands :

    Do we need fusion? And the answer will beyes if not now then in the future.

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    Fusion as an energy source. Prepared for IOP by W. J. Nuttall 09.2008. p1

    introduction to plasma physics by R.J. Goldston and Paul Harding Rutherford

    http://www.opencourse.info/astronomy/introduction/12.sun_interior/

    BP Review of World Energy 2008

    http://www.solarenergy.org/resources/energyfacts.html

    Fusion as an Energy Source A guide from the Institute of Physics

    Heisenberg Uncertainty Principle-http://zebu.uoregon.edu/~imamura/208/jan27/hup.html

    Quantum Tunnelling-http://hyperphysics.phy-astr.gsu.edu/Hbase/quantum/barr.html#c1

    Wave Function-http://hyperphysics.phy-astr.gsu.edu/Hbase /hframe.html

    Young and Freedman, University Physics

    Basic Magnetic Confinement (+pic)-http://www-fusion-magnetique.cea.fr/gb/fusion/principes/principes02.htm

    Confinement and Heating info-http://www.fusion-eur.org/fusion_cd/magnetic.htm

    http://www.iter.org/ http://www.scienceworld.physics.co.uk

    www.jet.efda.org/

    http://en.wikipedia.org/wiki/Timeline_of_nuclear_fusion

    http://www.efda.org/fusion_energy/short_history_of_fusion_research.htm

    http://ec.europa.eu/research/energy/fu/fu_int/article_1247_en.htm

    http://www.newscientist.com/article/mg19025543.300-editorial-nuclear-fusion-must-be-worth-the-gamble.html NewScientist, last update 7th June 2006

    http://www.iter.org/cost.htm ITER Official Site, last accessed 18th January 2009 http://www.iter.org/a/index_nav_4.htm ITER Official Site, last accessed 18th January 2009

    http://fusionforenergy.europa.eu/3_4_demo_en.htm, last accessed 18th January

    Gleick, Peter, The Worlds Water 2002 2003. Island Press, Washington DC, 1998

    Martin, James, The Meaning of the 21st Century, Eden Project Books, 2006

    www.world-nulcear.org

    www.parliament.uk

    http://www.opencourse.info/astronomy/introduction/12.sun_interior/http://www.solarenergy.org/resources/energyfacts.htmlhttp://zebu.uoregon.edu/~imamura/208/jan27/hup.htmlhttp://hyperphysics.phy-astr.gsu.edu/Hbase/quantum/barr.html#c1http://hyperphysics.phy-astr.gsu.edu/Hbase/hframe.htmlhttp://hyperphysics.phy-astr.gsu.edu/Hbase/hframe.htmlhttp://www-fusion-magnetique.cea.fr/gb/fusion/principes/principes02.htmhttp://www.fusion-eur.org/fusion_cd/magnetic.htmhttp://www.iter.org/http://www.scienceworld.physics.co.uk/http://www.jet.efda.org/http://en.wikipedia.org/wiki/Timeline_of_nuclear_fusionhttp://www.efda.org/fusion_energy/short_history_of_fusion_research.htmhttp://ec.europa.eu/research/energy/fu/fu_int/article_1247_en.htmhttp://www.newscientist.com/article/mg19025543.300-editorial-nuclear-fusion-must-be-worth-the-gamble.htmlhttp://www.iter.org/cost.htmhttp://fusionforenergy.europa.eu/3_4_demo_en.htmhttp://www.world-nulcear.org/http://www.parliament.uk/http://www.parliament.uk/http://www.world-nulcear.org/http://fusionforenergy.europa.eu/3_4_demo_en.htmhttp://www.iter.org/cost.htmhttp://www.newscientist.com/article/mg19025543.300-editorial-nuclear-fusion-must-be-worth-the-gamble.htmlhttp://ec.europa.eu/research/energy/fu/fu_int/article_1247_en.htmhttp://www.efda.org/fusion_energy/short_history_of_fusion_research.htmhttp://en.wikipedia.org/wiki/Timeline_of_nuclear_fusionhttp://www.jet.efda.org/http://www.scienceworld.physics.co.uk/http://www.iter.org/http://www.fusion-eur.org/fusion_cd/magnetic.htmhttp://www-fusion-magnetique.cea.fr/gb/fusion/principes/principes02.htmhttp://hyperphysics.phy-astr.gsu.edu/Hbase/hframe.htmlhttp://hyperphysics.phy-astr.gsu.edu/Hbase/hframe.htmlhttp://hyperphysics.phy-astr.gsu.edu/Hbase/hframe.htmlhttp://hyperphysics.phy-astr.gsu.edu/Hbase/quantum/barr.html#c1http://hyperphysics.phy-astr.gsu.edu/Hbase/quantum/barr.html#c1http://hyperphysics.phy-astr.gsu.edu/Hbase/quantum/barr.html#c1http://zebu.uoregon.edu/~imamura/208/jan27/hup.htmlhttp://zebu.uoregon.edu/~imamura/208/jan27/hup.htmlhttp://zebu.uoregon.edu/~imamura/208/jan27/hup.htmlhttp://www.solarenergy.org/resources/energyfacts.htmlhttp://www.opencourse.info/astronomy/introduction/12.sun_interior/