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Riemann sums and integrals

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    We've done several
    videos already
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    where we're approximating
    the area under a curve
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    by breaking up that
    area into rectangles
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    and then finding the sum of
    the areas of those rectangles
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    as an approximation.
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    And this was actually
    the first example
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    that we looked at where
    each of the rectangles
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    had an equal width.
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    So we equally
    partitioned the interval
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    between our two boundaries
    between a and b.
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    And the height of the
    rectangle was the function
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    evaluated at the left
    endpoint of each rectangle.
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    And we wanted to generalize it
    and write it in sigma notation.
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    It looked something like this.
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    And this was one case.
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    Later on, we looked
    at a situation
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    where you define the
    height by the function
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    value at the right endpoint
    or at the midpoint.
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    And then we even
    constructed trapezoids.
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    And these are all particular
    instances of Riemann sums.
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    So this right over
    here is a Riemann sum.
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    And when people talk
    about Riemann sums,
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    they're talking about
    the more general notion.
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    You don't have to
    just do it this way.
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    You could use trapezoids.
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    You don't even have to have
    equally-spaced partitions.
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    I used equally-spaced partitions
    because it made things
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    a little bit
    conceptually simpler.
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    And this right here is
    a picture of the person
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    that Riemann sums
    was named after.
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    This is Bernhard Riemann.
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    And he made many
    contributions to mathematics.
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    But what he is most
    known for, at least
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    if you're taking a
    first-year calculus course,
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    is the Riemann sum.
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    And how this is used to
    define the Riemann integral.
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    Both Newton and
    Leibniz had come up
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    with the idea of
    the integral when
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    they had formulated calculus,
    but the Riemann integral
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    is kind of the most
    mainstream formal,
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    or I would say
    rigorous, definition
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    of what an integral is.
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    So as you could imagine, this is
    one instance of a Riemann sum.
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    We have n right over here.
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    The larger n is, the better an
    approximation it's going to be.
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    So his definition of
    an integral, which
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    is the actual area
    under the curve,
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    or his definition of a
    definite integral, which
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    is the actual area under
    a curve between a and b
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    is to take this Riemann sum,
    it doesn't have to be this one,
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    take any Riemann sum, and
    take the limit as n approaches
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    infinity.
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    So just to be clear,
    what's happening
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    when n approaches infinity?
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    Let me draw another
    diagram here.
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    So let's say that's my y-axis.
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    This is my x-axis.
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    This is my function.
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    As n approaches
    infinity-- so this is a,
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    this is b-- you're just going
    to have a ton of rectangles.
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    You're just going to get a
    ton of rectangles over there.
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    And there are going to
    become better and better
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    approximations for
    the actual area.
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    And the actual area
    under the curve
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    is denoted by the integral
    from a to b of f of x times dx.
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    And you see where
    this is coming from
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    or how these
    notations are close.
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    Or at least in my brain,
    how they're connected.
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    Delta x was the width for
    each of these sections.
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    This right here is delta x.
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    So that is a delta x.
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    This is another delta x.
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    This is another delta x.
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    A reasonable way to
    conceptualize what dx is,
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    or what a differential
    is, is what delta x
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    approaches, if it
    becomes infinitely small.
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    So you can conceptualize
    this, and it's not
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    a very rigorous way
    of thinking about it,
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    is an infinitely small-- but
    not 0-- infinitely small delta
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    x, is one way that you
    can conceptualize this.
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    So once again, as you
    have your function
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    times a little small
    change in delta x.
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    And you are summing,
    although you're
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    summing an infinite number
    of these things, from a to b.
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    So I'm going to
    leave you there just
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    so that you see the connection.
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    You know the name
    for these things.
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    And once again, this
    one over here, this
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    isn't the only Riemann sum.
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    In fact, this is often
    called the left Riemann sum
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    if you're using it
    with rectangles.
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    You can do a right Riemann sum.
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    You could use the midpoint.
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    You could use a trapezoid.
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    But if you take the limit of
    any of those Riemann sums,
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    as n approaches
    infinity, then that you
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    get as a Riemann
    definition of the integral.
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    Now so far, we haven't
    talked about how
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    to actually evaluate this thing.
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    This is just a
    definition right now.
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    And for that we will
    do in future videos.
Title:
Riemann sums and integrals
Description:

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Video Language:
English
Team:
Khan Academy
Duration:
04:26

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