Calc06_1day2

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    6.1 day 2

    Euler’s Method

    Leonhard Euler 1707 - 1783

    Leonhard Euler made a

    huge number of

    contributions to

    mathematics, almost half

    after he was totally blind.

    (When this ortrait was

    made he had already lost

    most of the sight in his right

    eye.!

    "reg #elly, $anford $igh %chool, &ichland, Washington

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      Leonhard Euler 1707 - 1783

    't was Euler who originated

    the following notations

    e (base of natural log!

    ( ) f x (function notation!

    π   (i!

    i   ( )1−

    (summation!∑

     y∆

    (finite change! →

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    )here are many differential e*uations that can not be sol+ed.

    We can still find an aroimate solution.

    We will ractice with an easy one that can be sol+ed.

    2dy

     xdx

    = 'nitial +alue0 1 y   =

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    2dy

     xdx

    =0 1 y   =

    n   n x n y dydx   dy   1n y +

    0.5dx  =

    0   0 1   0 0 1

    1 .5 1 1   .5 1.52   1 1.5 2   1   2.5

    dydx dy

    dx

    ⋅ =1n n y dy y ++ =

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    3 1.5   2.5 3 1.5   4.0

    4 2.0   4.0

    dydx dy

    dx

    ⋅ =1n n y dy y ++ =

    2dy

     xdx

    =

    n   n x n y dydx   dy   1n y +

    0.5dx  =

    0   0 1   0 0 1

    1 .5 1 1   .5 1.52   1 1.5 2   1   2.5

    0 1 y   =

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    2dy

     xdx

    =   ( )0,1 0.5dx  =

    2dy x dx=

    2 y x C = +

    1 0   C = +

    21 y x= +

    Eact %olution

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    't is more accurate if a smaller

    +alue is used for dx.

    )his is called Euler’s Method.

    't gets less accurate as you

    mo+e away from the initial

    +alue.

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    )he )'-/ has Euler’s Method built in.

    Eamle   ( ).001 100dy

     y ydx = −0 10 y   =

    We will do the sloefield first

    6 0' E34)'5%"rah7..

    89   ( )1 .001 1 100 1 y y y′ = ∗ ∗ −We use

     y1 for  y

    t  for  x

    MODE

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    6 0' E34)'5%"rah7..

    ( )1 .001 1 100 1 y y y′ = ∗ ∗ −

    W'05W t:9:

    tma91;:tste9.2

    tlot9:

    min9:

    ma9

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    t:9:

    tma91;:

    tste9.2

    tlot9:min9:

    ma9

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    While the calculator is still dislaying the grah

    yi1=10

    tstep = .2

    'f tste is larger the grah

    is faster.'f tste is smaller the

    grah is more accurate.

     ' >ress and change %olution Method to EULER.

    W'05W

    "&4>$

    89

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    )o lot another cur+e with a different initial +alue

    Either mo+e the curser or enter the initial conditions

    when romted.

    F8

    8ou can also in+estigate the cur+e by using .F3

    )race

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    y1 2t ′ =

    t:9:

    tma91:tste9.;

    tlot9:

    min9:

    ma91:

    scl91

    ymin9:

    yma9;yscl91

    ncur+es9:

    Este91

    fldres91=

    "&4>$

    ow let’s use the calculator to reroduce our first grah

    2dy

     x

    dx

    = 0 1 y   =

    yi1 1=

    We use

     y1 for  y

    t  for  x

     '  ?hange ields to FLDOFF.→

    W'05W

    89

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      →

    3se to confirm that the oints are the same as

    the ones we found by hand.

    F3 )race

    )able>ress

    )bl%et>ress and set tblstart... 0 tbl.... .5∆

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    )his gi+es us a table of the oints that we found in our

    first eamle.

    )able>ress

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    )he boo@ refers to an A'mro+ed Euler’s MethodB. We will

    not be using it, and you do not need to @now it.

    )he calculator also contains a similar but more comlicated

    (and more accurate! formula called the &unge-#utta

    method.

    8ou don’t need to @now anything about it other than the fact

    that it is used more often in real life.

    )his is the solution method on your calculator.

    π