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2 Unless otherwise noted, the content of this course material is licensed under a Creative Commons BY 3.0 License. http://creativecommons.org/licenses/by/3.0/ Copyright © 2009, August E. Evrard. You assume all responsibility for use and potential liability associated with any use of the material. Material contains copyrighted content, used in accordance with U.S. law. Copyright holders of content included in this material should contact open.michigan@umich.edu with any questions, corrections, or clarifications regarding the use of content. The Regents of the University of Michigan do not license the use of third party content posted to this site unless such a license is specifically granted in connection with particular content. Users of content are responsible for their compliance with applicable law. Mention of specific products in this material solely represents the opinion of the speaker and does not represent an endorsement by the University of Michigan. For more information about how to cite these materials visit http://open.umich.edu/education/about/terms-of-usehttp://open.umich.edu/education/about/terms-of-use Any medical information in this material is intended to inform and educate and is not a tool for self-diagnosis or a replacement for medical evaluation, advice, diagnosis or treatment by a healthcare professional. You should speak to your physician or make an appointment to be seen if you have questions or concerns about this information or your medical condition. Viewer discretion is advised: Material may contain medical images that may be disturbing to some viewers.

3 Physics 140 – Fall 2007 lecture #24: 29 Nov Exam #3 tonight 6:00-7:30 pm Ch 9-12 Ch 14 topics: ideal fluid dynamics volume flow rate (incompressible fluids) Bernoulli’s equation Source: V.van Gogh, Starry Night

4 An ideal fluid is defined by the following set of characteristics. The flow of the fluid must be steady The velocity at any point in the flow does not change in time. incompressible The density does not change with pressure. non-viscous There are no sources of internal friction that could remove energy from the flow. irrotational An element (small piece) of the flow traces out a straight path aligned with the fluid velocity, not a helical pattern around it. Ideal fluids

5 Ideal fluid flow is a simple, but useful approximation to actual fluid motion. Arrows here represent the flow velocity in a cross-sectional cutout of the pipe. The velocity is constant across the area, there is no rotation, and no drag (viscosity) near the edges of the pipe.

6 Small drag in streamlined position Large drag in unstreamlined position Both Images CC: BY-SA BoH (wimimedia commons) http://creativecommons.org/licenses/by-sa/3.0/

7 Turbulent flow: `vortex shedding’ around an obstacle Steady (also called laminar) flow to the left of an island becomes unsteady (or turbulent ) after passing by it. The grey scale image above shows clouds in the atmosphere. Patches of the flow behind the obstacle are spun up to create a series of vortices that alternately roll off, or ‘shed’, from the top and bottom of the tube. The behavior downstream of the tube is one of many examples of non-ideal fluid flow. Island (from above) ideal fluid flows in Source: NASA

8 For a fluid of density  flowing through a pipe of cross-sectional area A at speed v, the amount of mass  m passing through a joint in the pipe in a time interval  t is given by For regions of flow in which there are no sources or sinks of fluid, the requirement that mass is neither created nor destroyed implies that the product  Av is the same at all parts of the flow Since an incompressible fluid has the same density at all points in the flow (  =constant), then two locations (1 and 2) of a pipe with different cross-sectional area will have the same volume flow rate  m =  A v  t A 1 v 1 = A 2 v 2  1 A 1 v 1 =  2 A 2 v 2 Conservation of mass for incompressible fluids

9 Flow in an ideal fluid conserves total energy. When fluid flows in a gravitational field, the energy (per unit volume of fluid) comes in three forms: gravitational potential energy density:  gy kinetic energy density:  v 2 /2 (ordered particle velocities) internal energy density: P (disordered particle velocities) The requirement that the total energy be conserved implies that the sum of these three forms remains constant throughout the flow. The result is Bernoulli’s equation P +  v 2 /2 +  gy = constant Conservation of energy: Bernoulli’s equation

10 mostly disordered motion – high pressure – low velocity mostly ordered motion – low pressure – high velocity vv ~ 0

11 A blood platelet drifts along with the flow of blood through an artery that is partially blocked. As the platelet moves from the wide region to the narrow region, it experiences 1)an increase in pressure. 2)a decrease in pressure. 3)no change in pressure.

12 An ideal fluid flows in the above arrangement of tubes. Rank the locations according to the flow velocity, greatest to least. 1)3, 2, 1 2)3, 1, 2 3)1, 2, 3 4)1, 2=3 5)1=3, 2

13 A water tank with an open top sits on a table at rest. If it is rapidly punctured with five, vertically aligned holes, what would resulting flow look like?

14 A small water tank with an open top is dropped, preserving its vertical orientation, down an elevator shaft. Just after release, it is rapidly punctured with five, vertically aligned holes. What will resulting flow look like?

15 You sit in a boat on a man-made lake filled with a fixed volume of water. Accompanying you is the pair of large rocks from back in Chapter 10. This time, instead of throwing the rocks sideways, you drop them gently into the water. What happens to the water level in the lake after the rocks have sunk below the surface? 1)It goes up. 2)It goes down. 3)It stays the same.


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