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Bernoulli's principle
Bernoulli's principle
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A flow of air through a Venturi meter. The kinetic energy increases at the expense of the fluid pressure, as shown by the difference in height of the two columns of water.
Video of a Venturi meter used in a lab experiment

Bernoulli's principle is a key concept in fluid dynamics that relates pressure, speed and height. For example, for a fluid flowing horizontally, Bernoulli's principle states that an increase in the speed occurs simultaneously with a decrease in pressure.[1]: Ch.3 [2]: 156–164, § 3.5  The principle is named after the Swiss mathematician and physicist Daniel Bernoulli, who published it in his book Hydrodynamica in 1738.[3] Although Bernoulli deduced that pressure decreases when the flow speed increases, it was Leonhard Euler in 1752 who derived Bernoulli's equation in its usual form.[4][5]

Bernoulli's principle can be derived from the principle of conservation of energy. This states that, in a steady flow, the sum of all forms of energy in a fluid is the same at all points that are free of viscous forces. This requires that the sum of kinetic energy, potential energy and internal energy remains constant.[2]: § 3.5  Thus an increase in the speed of the fluid—implying an increase in its kinetic energy—occurs with a simultaneous decrease in (the sum of) its potential energy (including the static pressure) and internal energy. If the fluid is flowing out of a reservoir, the sum of all forms of energy is the same because in a reservoir the energy per unit volume (the sum of pressure and gravitational potential ρgh) is the same everywhere.[6]: Example 3.5 and p.116 

Bernoulli's principle can also be derived directly from Isaac Newton's second law of motion. When a fluid is flowing horizontally from a region of high pressure to a region of low pressure, there is more pressure from behind than in front. This gives a net force on the volume, accelerating it along the streamline. [a][b][c]

Fluid particles are subject only to pressure and their own weight. If a fluid is flowing horizontally and along a section of a streamline, where the speed increases it can only be because the fluid on that section has moved from a region of higher pressure to a region of lower pressure; and if its speed decreases, it can only be because it has moved from a region of lower pressure to a region of higher pressure. Consequently, within a fluid flowing horizontally, the highest speed occurs where the pressure is lowest, and the lowest speed occurs where the pressure is highest.[10]

The upstream static pressure (1) is higher than in the constriction (2), and the fluid speed at "1" is slower than at "2", because the cross-sectional area at "1" is greater than at "2".

Bernoulli's principle is only applicable for isentropic flows: when the effects of irreversible processes (like turbulence) and non-adiabatic processes (e.g. thermal radiation) are small and can be neglected. However, the principle can be applied to various types of flow within these bounds, resulting in various forms of Bernoulli's equation. The simple form of Bernoulli's equation is valid for incompressible flows (e.g. most liquid flows and gases moving at low Mach number). More advanced forms may be applied to compressible flows at higher Mach numbers.

Incompressible flow equation

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In most flows of liquids, and of gases at low Mach number, the density of a fluid parcel can be considered to be constant, regardless of pressure variations in the flow. Therefore, the fluid can be considered to be incompressible, and these flows are called incompressible flows. Bernoulli performed his experiments on liquids, so his equation in its original form is valid only for incompressible flow.

A common form of Bernoulli's equation is:

where:

  • is the fluid flow speed at a point,
  • is the acceleration due to gravity,
  • is the elevation of the point above a reference plane, with the positive -direction pointing upward—so in the direction opposite to the gravitational acceleration,
  • is the static pressure at the chosen point, and
  • is the density of the fluid at all points in the fluid.

Bernoulli's equation and the Bernoulli constant are applicable throughout any region of flow where the energy per unit mass is uniform. Because the energy per unit mass of liquid in a well-mixed reservoir is uniform throughout, Bernoulli's equation can be used to analyze the fluid flow everywhere in that reservoir (including pipes or flow fields that the reservoir feeds) except where viscous forces dominate and erode the energy per unit mass.[6]: Example 3.5 and p.116 

The following assumptions must be met for this Bernoulli equation to apply:[2]: 265 

  • the flow must be steady, that is, the flow parameters (velocity, density, etc.) at any point cannot change with time,
  • the flow must be incompressible—even though pressure varies, the density must remain constant along a streamline;
  • friction by viscous forces must be negligible.

For conservative force fields (not limited to the gravitational field), Bernoulli's equation can be generalized as:[2]: 265  where Ψ is the force potential at the point considered. For example, for the Earth's gravity Ψ = gz.

By multiplying with the fluid density ρ, equation (A) can be rewritten as: or: where

  • q = 1/2ρv2 is dynamic pressure,
  • h = z + p/ρg is the piezometric head or hydraulic head (the sum of the elevation z and the pressure head)[11][12] and
  • p0 = p + q is the stagnation pressure (the sum of the static pressure p and dynamic pressure q).[13]

The constant in the Bernoulli equation can be normalized. A common approach is in terms of total head or energy head H:

The above equations suggest there is a flow speed at which pressure is zero, and at even higher speeds the pressure is negative. Most often, gases and liquids are not capable of negative absolute pressure, or even zero pressure, so clearly Bernoulli's equation ceases to be valid before zero pressure is reached. In liquids—when the pressure becomes too low—cavitation occurs. The above equations use a linear relationship between flow speed squared and pressure. At higher flow speeds in gases, or for sound waves in liquid, the changes in mass density become significant so that the assumption of constant density is invalid.

Simplified form

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In many applications of Bernoulli's equation, the change in the ρgz term is so small compared with the other terms that it can be ignored. For example, in the case of aircraft in flight, the change in height z is so small the ρgz term can be omitted. This allows the above equation to be presented in the following simplified form: where p0 is called total pressure, and q is dynamic pressure.[14] Many authors refer to the pressure p as static pressure to distinguish it from total pressure p0 and dynamic pressure q. In Aerodynamics, L.J. Clancy writes: "To distinguish it from the total and dynamic pressures, the actual pressure of the fluid, which is associated not with its motion but with its state, is often referred to as the static pressure, but where the term pressure alone is used it refers to this static pressure."[1]: § 3.5 

The simplified form of Bernoulli's equation can be summarized in the following memorable word equation:[1]: § 3.5 

Static pressure + Dynamic pressure = Total pressure.

Every point in a steadily flowing fluid, regardless of the fluid speed at that point, has its own unique static pressure p and dynamic pressure q. Their sum p + q is defined to be the total pressure p0. The significance of Bernoulli's principle can now be summarized as "total pressure is constant in any region free of viscous forces". If the fluid flow is brought to rest at some point, this point is called a stagnation point, and at this point the static pressure is equal to the stagnation pressure.

If the fluid flow is irrotational, the total pressure is uniform and Bernoulli's principle can be summarized as "total pressure is constant everywhere in the fluid flow".[1]: Equation 3.12  It is reasonable to assume that irrotational flow exists in any situation where a large body of fluid is flowing past a solid body. Examples are aircraft in flight and ships moving in open bodies of water. However, Bernoulli's principle importantly does not apply in the boundary layer such as in flow through long pipes.

Unsteady potential flow

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The Bernoulli equation for unsteady potential flow is used in the theory of ocean surface waves and acoustics. For an irrotational flow, the flow velocity can be described as the gradient φ of a velocity potential φ. In that case, and for a constant density ρ, the momentum equations of the Euler equations can be integrated to:[2]: 383 

which is a Bernoulli equation valid also for unsteady—or time dependent—flows. Here φ/t denotes the partial derivative of the velocity potential φ with respect to time t, and v = |φ| is the flow speed. The function f(t) depends only on time and not on position in the fluid. As a result, the Bernoulli equation at some moment t applies in the whole fluid domain. This is also true for the special case of a steady irrotational flow, in which case f and φ/t are constants so equation (A) can be applied in every point of the fluid domain.[2]: 383  Further f(t) can be made equal to zero by incorporating it into the velocity potential using the transformation: resulting in:

Note that the relation of the potential to the flow velocity is unaffected by this transformation: ∇Φ = ∇φ.

The Bernoulli equation for unsteady potential flow also appears to play a central role in Luke's variational principle, a variational description of free-surface flows using the Lagrangian mechanics.

Compressible flow equation

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Bernoulli developed his principle from observations on liquids, and Bernoulli's equation is valid for ideal fluids: those that are inviscid, incompressible and subjected only to conservative forces. It is sometimes valid for the flow of gases as well, provided that there is no transfer of kinetic or potential energy from the gas flow to the compression or expansion of the gas. If both the gas pressure and volume change simultaneously, then work will be done on or by the gas. In this case, Bernoulli's equation in its incompressible flow form cannot be assumed to be valid. However, if the gas process is entirely isobaric, or isochoric, then no work is done on or by the gas (so the simple energy balance is not upset). According to the gas law, an isobaric or isochoric process is ordinarily the only way to ensure constant density in a gas. Also the gas density will be proportional to the ratio of pressure and absolute temperature; however, this ratio will vary upon compression or expansion, no matter what non-zero quantity of heat is added or removed. The only exception is if the net heat transfer is zero, as in a complete thermodynamic cycle or in an individual isentropic (frictionless adiabatic) process, and even then this reversible process must be reversed, to restore the gas to the original pressure and specific volume, and thus density. Only then is the original, unmodified Bernoulli equation applicable. In this case the equation can be used if the flow speed of the gas is sufficiently below the speed of sound, such that the variation in density of the gas (due to this effect) along each streamline can be ignored. Adiabatic flow at less than Mach 0.3 is generally considered to be slow enough.[15]

It is possible to use the fundamental principles of physics to develop similar equations applicable to compressible fluids. There are numerous equations, each tailored for a particular application, but all are analogous to Bernoulli's equation and all rely on nothing more than the fundamental principles of physics such as Newton's laws of motion or the first law of thermodynamics.

Compressible flow in fluid dynamics

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For a compressible fluid, with a barotropic equation of state, and under the action of conservative forces,[16] where:

  • p is the pressure
  • ρ is the density and ρ(p) indicates that it is a function of pressure
  • v is the flow speed
  • Ψ is the potential associated with the conservative force field, often the gravitational potential

In engineering situations, elevations are generally small compared to the size of the Earth, and the time scales of fluid flow are small enough to consider the equation of state as adiabatic. In this case, the above equation for an ideal gas becomes:[1]: § 3.11  where, in addition to the terms listed above:

  • γ is the ratio of the specific heats of the fluid
  • g is the acceleration due to gravity
  • z is the elevation of the point above a reference plane

In many applications of compressible flow, changes in elevation are negligible compared to the other terms, so the term gz can be omitted. A very useful form of the equation is then:

where:

Compressible flow in thermodynamics

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The most general form of the equation, suitable for use in thermodynamics in case of (quasi) steady flow, is:[2]: § 3.5 [17]: § 5 [18]: § 5.9 

Here w is the enthalpy per unit mass (also known as specific enthalpy), which is also often written as h (not to be confused with "head" or "height").

Note that where e is the thermodynamic energy per unit mass, also known as the specific internal energy. So, for constant internal energy the equation reduces to the incompressible-flow form.

The constant on the right-hand side is often called the Bernoulli constant and denoted b. For steady inviscid adiabatic flow with no additional sources or sinks of energy, b is constant along any given streamline. More generally, when b may vary along streamlines, it still proves a useful parameter, related to the "head" of the fluid (see below).

When the change in Ψ can be ignored, a very useful form of this equation is: where w0 is total enthalpy. For a calorically perfect gas such as an ideal gas, the enthalpy is directly proportional to the temperature, and this leads to the concept of the total (or stagnation) temperature.

When shock waves are present, in a reference frame in which the shock is stationary and the flow is steady, many of the parameters in the Bernoulli equation suffer abrupt changes in passing through the shock. The Bernoulli parameter remains unaffected. An exception to this rule is radiative shocks, which violate the assumptions leading to the Bernoulli equation, namely the lack of additional sinks or sources of energy.

Unsteady potential flow

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For a compressible fluid, with a barotropic equation of state, the unsteady momentum conservation equation

With the irrotational assumption, namely, the flow velocity can be described as the gradient φ of a velocity potential φ. The unsteady momentum conservation equation becomes which leads to

In this case, the above equation for isentropic flow becomes:

Derivations

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Bernoulli equation for incompressible fluids

The Bernoulli equation for incompressible fluids can be derived by either integrating Newton's second law of motion or by applying the law of conservation of energy, ignoring viscosity, compressibility, and thermal effects.

Derivation by integrating Newton's second law of motion

The simplest derivation is to first ignore gravity and consider constrictions and expansions in pipes that are otherwise straight, as seen in Venturi effect. Let the x axis be directed down the axis of the pipe.

Define a parcel of fluid moving through a pipe with cross-sectional area A, the length of the parcel is dx, and the volume of the parcel A dx. If mass density is ρ, the mass of the parcel is density multiplied by its volume m = ρA dx. The change in pressure over distance dx is dp and flow velocity v = dx/dt.

Apply Newton's second law of motion (force = mass × acceleration) and recognizing that the effective force on the parcel of fluid is A dp. If the pressure decreases along the length of the pipe, dp is negative but the force resulting in flow is positive along the x axis.

In steady flow the velocity field is constant with respect to time, v = v(x) = v(x(t)), so v itself is not directly a function of time t. It is only when the parcel moves through x that the cross sectional area changes: v depends on t only through the cross-sectional position x(t).

With density ρ constant, the equation of motion can be written as by integrating with respect to x where C is a constant, sometimes referred to as the Bernoulli constant. It is not a universal constant, but rather a constant of a particular fluid system. The deduction is: where the speed is large, pressure is low and vice versa.

In the above derivation, no external work–energy principle is invoked. Rather, Bernoulli's principle was derived by a simple manipulation of Newton's second law.

A streamtube of fluid moving to the right. Indicated are pressure, elevation, flow speed, distance (s), and cross-sectional area. Note that in this figure elevation is denoted as h, contrary to the text where it is given by z.
Derivation by using conservation of energy

Another way to derive Bernoulli's principle for an incompressible flow is by applying conservation of energy.[19] In the form of the work-energy theorem, stating that[20]

the change in the kinetic energy Ekin of the system equals the net work W done on the system;

Therefore,

the work done by the forces in the fluid equals increase in kinetic energy.

The system consists of the volume of fluid, initially between the cross-sections A1 and A2. In the time interval Δt fluid elements initially at the inflow cross-section A1 move over a distance s1 = v1 Δt, while at the outflow cross-section the fluid moves away from cross-section A2 over a distance s2 = v2 Δt. The displaced fluid volumes at the inflow and outflow are respectively A1s1 and A2s2. The associated displaced fluid masses are – when ρ is the fluid's mass density – equal to density times volume, so ρA1s1 and ρA2s2. By mass conservation, these two masses displaced in the time interval Δt have to be equal, and this displaced mass is denoted by Δm:

The work done by the forces consists of two parts:

  • The work done by the pressure acting on the areas A1 and A2
  • The work done by gravity: the gravitational potential energy in the volume A1s1 is lost, and at the outflow in the volume A2s2 is gained. So, the change in gravitational potential energy ΔEpot,gravity in the time interval Δt is

Now, the work by the force of gravity is opposite to the change in potential energy, Wgravity = −ΔEpot,gravity: while the force of gravity is in the negative z-direction, the work—gravity force times change in elevation—will be negative for a positive elevation change Δz = z2z1, while the corresponding potential energy change is positive.[21]: 14–4, §14–3  So: And therefore the total work done in this time interval Δt is The increase in kinetic energy is Putting these together, the work-kinetic energy theorem W = ΔEkin gives:[19] or After dividing by the mass Δm = ρA1v1 Δt = ρA2v2 Δt the result is:[19] or, as stated in the first paragraph:

Further division by g produces the following equation. Note that each term can be described in the length dimension (such as meters). This is the head equation derived from Bernoulli's principle:

The middle term, z, represents the potential energy of the fluid due to its elevation with respect to a reference plane. Now, z is called the elevation head and given the designation zelevation.

A free falling mass from an elevation z > 0 (in a vacuum) will reach a speed when arriving at elevation z = 0. Or when rearranged as head: The term v2/2g is called the velocity head, expressed as a length measurement. It represents the internal energy of the fluid due to its motion.

The hydrostatic pressure p is defined as with p0 some reference pressure, or when rearranged as head: The term p/ρg is also called the pressure head, expressed as a length measurement. It represents the internal energy of the fluid due to the pressure exerted on the container. The head due to the flow speed and the head due to static pressure combined with the elevation above a reference plane, a simple relationship useful for incompressible fluids using the velocity head, elevation head, and pressure head is obtained.

If Eqn. 1 is multiplied by the density of the fluid, an equation with three pressure terms is obtained:

Note that the pressure of the system is constant in this form of the Bernoulli equation. If the static pressure of the system (the third term) increases, and if the pressure due to elevation (the middle term) is constant, then the dynamic pressure (the first term) must have decreased. In other words, if the speed of a fluid decreases and it is not due to an elevation difference, it must be due to an increase in the static pressure that is resisting the flow.

All three equations are merely simplified versions of an energy balance on a system.

Bernoulli equation for compressible fluids

The derivation for compressible fluids is similar. Again, the derivation depends upon (1) conservation of mass, and (2) conservation of energy. Conservation of mass implies that in the above figure, in the interval of time Δt, the amount of mass passing through the boundary defined by the area A1 is equal to the amount of mass passing outwards through the boundary defined by the area A2: Conservation of energy is applied in a similar manner: It is assumed that the change in energy of the volume of the streamtube bounded by A1 and A2 is due entirely to energy entering or leaving through one or the other of these two boundaries. Clearly, in a more complicated situation such as a fluid flow coupled with radiation, such conditions are not met. Nevertheless, assuming this to be the case and assuming the flow is steady so that the net change in the energy is zero, where ΔE1 and ΔE2 are the energy entering through A1 and leaving through A2, respectively. The energy entering through A1 is the sum of the kinetic energy entering, the energy entering in the form of potential gravitational energy of the fluid, the fluid thermodynamic internal energy per unit of mass (ε1) entering, and the energy entering in the form of mechanical p dV work: where Ψ = gz is a force potential due to the Earth's gravity, g is acceleration due to gravity, and z is elevation above a reference plane. A similar expression for ΔE2 may easily be constructed. So now setting 0 = ΔE1 − ΔE2: which can be rewritten as: Now, using the previously-obtained result from conservation of mass, this may be simplified to obtain which is the Bernoulli equation for compressible flow.

An equivalent expression can be written in terms of fluid enthalpy (h):

Applications

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Condensation visible over the upper surface of an Airbus A340 wing caused by the increase in relative humidity accompanying the fall in pressure and temperature

In modern everyday life there are many observations that can be successfully explained by application of Bernoulli's principle, even though no real fluid is entirely inviscid,[22] and a small viscosity often has a large effect on the flow.

  • Bernoulli's principle can be used to calculate the lift force on an airfoil, if the behaviour of the fluid flow in the vicinity of the foil is known. For example, if the air flowing past the top surface of an aircraft wing is moving faster than the air flowing past the bottom surface, then Bernoulli's principle implies that the pressure on the surfaces of the wing will be lower above than below. This pressure difference results in an upwards lifting force.[d][23] Whenever the distribution of speed past the top and bottom surfaces of a wing is known, the lift forces can be calculated (to a good approximation) using Bernoulli's equations,[24] which were established by Bernoulli over a century before the first man-made wings were used for the purpose of flight.
  • The basis of a carburetor used in many reciprocating engines is a throat in the air flow to create a region of low pressure to draw fuel into the carburetor and mix it thoroughly with the incoming air. The low pressure in the throat can be explained by Bernoulli's principle, where air in the throat is moving at its fastest speed and therefore it is at its lowest pressure. The carburetor may or may not use the difference between the two static pressures which result from the Venturi effect on the air flow in order to force the fuel to flow, and as a basis a carburetor may use the difference in pressure between the throat and local air pressure in the float bowl, or between the throat and a Pitot tube at the air entry.
  • An injector on a steam locomotive or a static boiler.
  • The pitot tube and static port on an aircraft are used to determine the airspeed of the aircraft. These two devices are connected to the airspeed indicator, which determines the dynamic pressure of the airflow past the aircraft. Bernoulli's principle is used to calibrate the airspeed indicator so that it displays the indicated airspeed appropriate to the dynamic pressure.[1]: § 3.8 
  • A De Laval nozzle utilizes Bernoulli's principle to create a force by turning pressure energy generated by the combustion of propellants into velocity. This then generates thrust by way of Newton's third law of motion.
  • The flow speed of a fluid can be measured using a device such as a Venturi meter or an orifice plate, which can be placed into a pipeline to reduce the diameter of the flow. For a horizontal device, the continuity equation shows that for an incompressible fluid, the reduction in diameter will cause an increase in the fluid flow speed. Subsequently, Bernoulli's principle then shows that there must be a decrease in the pressure in the reduced diameter region. This phenomenon is known as the Venturi effect.
  • The maximum possible drain rate for a tank with a hole or tap at the base can be calculated directly from Bernoulli's equation and is found to be proportional to the square root of the height of the fluid in the tank. This is Torricelli's law, which is compatible with Bernoulli's principle. Increased viscosity lowers this drain rate; this is reflected in the discharge coefficient, which is a function of the Reynolds number and the shape of the orifice.[25]
  • The Bernoulli grip relies on this principle to create a non-contact adhesive force between a surface and the gripper.
  • During a cricket match, bowlers continually polish one side of the ball. After some time, one side is quite rough and the other is still smooth. Hence, when the ball is bowled and passes through air, the speed on one side of the ball is faster than on the other, and this results in a pressure difference between the sides; this leads to the ball rotating ("swinging") while travelling through the air, giving advantage to the bowlers.

Misconceptions

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Airfoil lift

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An illustration of the incorrect equal transit-time explanation of airfoil lift

One of the most common erroneous explanations of aerodynamic lift asserts that the air must traverse the upper and lower surfaces of a wing in the same amount of time, implying that since the upper surface presents a longer path the air must be moving over the top of the wing faster than over the bottom. Bernoulli's principle is then cited to conclude that the pressure on top of the wing must be lower than on the bottom.[26][27]

Equal transit time applies to the flow around a body generating no lift, but there is no physical principle that requires equal transit time in cases of bodies generating lift. In fact, theory predicts – and experiments confirm – that the air traverses the top surface of a body experiencing lift in a shorter time than it traverses the bottom surface; the explanation based on equal transit time is false.[28][29][30] While the equal-time explanation is false, it is not the Bernoulli principle that is false, because this principle is well established; Bernoulli's equation is used correctly in common mathematical treatments of aerodynamic lift.[31][32]

Common classroom demonstrations

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There are several common classroom demonstrations that are sometimes incorrectly explained using Bernoulli's principle.[33] One involves holding a piece of paper horizontally so that it droops downward and then blowing over the top of it. As the demonstrator blows over the paper, the paper rises. It is then asserted that this is because "faster moving air has lower pressure".[34][35][36]

One problem with this explanation can be seen by blowing along the bottom of the paper: if the deflection was caused by faster moving air, then the paper should deflect downward; but the paper deflects upward regardless of whether the faster moving air is on the top or the bottom.[37] Another problem is that when the air leaves the demonstrator's mouth it has the same pressure as the surrounding air;[38] the air does not have lower pressure just because it is moving; in the demonstration, the static pressure of the air leaving the demonstrator's mouth is equal to the pressure of the surrounding air.[39][40] A third problem is that it is false to make a connection between the flow on the two sides of the paper using Bernoulli's equation since the air above and below are different flow fields and Bernoulli's principle only applies within a flow field.[41][42][43][44]

As the wording of the principle can change its implications, stating the principle correctly is important.[45] What Bernoulli's principle actually says is that within a flow of constant energy, when fluid flows through a region of lower pressure it speeds up and vice versa.[46] Thus, Bernoulli's principle concerns itself with changes in speed and changes in pressure within a flow field. It cannot be used to compare different flow fields.

A correct explanation of why the paper rises would observe that the plume follows the curve of the paper and that a curved streamline will develop a pressure gradient perpendicular to the direction of flow, with the lower pressure on the inside of the curve.[47][48][49][50] Bernoulli's principle predicts that the decrease in pressure is associated with an increase in speed; in other words, as the air passes over the paper, it speeds up and moves faster than it was moving when it left the demonstrator's mouth. But this is not apparent from the demonstration.[51][52][53]

Other common classroom demonstrations, such as blowing between two suspended spheres, inflating a large bag, or suspending a ball in an airstream are sometimes explained in a similarly misleading manner by saying "faster moving air has lower pressure".[54][55][56][57][58][59][60][61]

See also

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Notes

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Bernoulli's principle is a fundamental concept in that describes the relationship between the , , and in a moving , stating that an increase in the speed of a element results in a simultaneous decrease in its or potential energy. Formulated by the Swiss mathematician and physicist Daniel Bernoulli, the principle was first published in his seminal work Hydrodynamica in 1738, where it emerged from studies of motion and energy conservation. This principle applies specifically to steady, inviscid (frictionless), and incompressible flows along a streamline, providing a cornerstone for understanding phenomena in both liquids and gases. The mathematical foundation of Bernoulli's principle is expressed through Bernoulli's equation, which equates the total per unit volume along a streamline: P+12ρv2+ρgh=constantP + \frac{1}{2} \rho v^2 + \rho g h = \text{constant}, where PP is the , ρ\rho is the fluid , vv is the , gg is , and hh is the above a reference level. For horizontal flows where elevation changes are negligible, the equation simplifies to P+12ρv2=constantP + \frac{1}{2} \rho v^2 = \text{constant}, illustrating the inverse relationship between pressure and velocity. These derivations assume ideal conditions—no viscosity, steady flow without , and constant —making the principle an approximation for real-world fluids but invaluable for engineering analyses. Bernoulli's principle has wide-ranging applications in engineering and physics, most notably in , where it explains the generation of lift on wings: air flows faster over the curved upper surface than the flat lower surface, reducing pressure above the wing and producing an upward force. It also underpins devices like the Venturi meter for measuring fluid flow rates through pressure differences in constrictions and pitot-static tubes for determining aircraft airspeed. In , the principle informs the design of carburetors and aspirators, where high-velocity fluid draws in lower-pressure substances, and it extends to natural phenomena such as flow in vessels or patterns around structures. Despite limitations in viscous or compressible flows, Bernoulli's principle remains a key tool for predicting fluid behavior in low-speed, ideal scenarios.

Introduction and History

Statement of the Principle

Bernoulli's principle describes a fundamental relationship in where an increase in the speed of a moving , whether or gas, is accompanied by a corresponding decrease in the within that . This intuitive observation highlights how faster-moving fluids exert lower compared to slower-moving ones, a phenomenon rooted in the as the accelerates and converts potential or energy into . For instance, in airflow over an , the higher on the upper surface results in lower , contributing to lift generation. In its general verbal form, the principle states that along a streamline in a flowing , the total per unit volume—comprising the energy, , and gravitational —remains constant, assuming no energy losses due to or other dissipative effects. This conservation implies that an increase in (from higher velocity) must be balanced by a decrease in energy or (from elevation changes). The principle applies specifically to ideal fluids that are inviscid (lacking ) and either incompressible or compressible under conditions where variations are negligible, and it holds for steady flow where conditions do not change with time along the streamline. The principle was first articulated by in his 1738 book , where he derived it from the conservation of (an early concept of ) applied to fluid motion, treating the fluid as composed of particles whose energy balance governs and relationships. Bernoulli's work emphasized in incompressible, frictionless flows, laying the groundwork for later formalizations in .

Historical Development

Daniel Bernoulli first articulated the core ideas underlying the principle in his 1738 book , where he applied Newtonian mechanics and the concept of (living force) to analyze fluid motion, particularly in , framing it as a balance of energy per unit volume between pressure, , and . This work established the principle's foundations in , emphasizing how variations in fluid speed affect pressure, though Bernoulli's formulation was initially limited to incompressible, steady flows without explicit momentum derivations. Leonhard Euler refined and generalized Bernoulli's insights in his 1757 publication "Principes généraux du mouvement des fluides," extending the principle to arbitrary fluid motions by deriving it rigorously from the momentum equations of inviscid flow, thus providing a more universal framework beyond confined pipe systems. Euler's contributions clarified the principle's applicability to broader hydrodynamic scenarios, marking a shift from empirical hydraulics to theoretical fluid dynamics. In the late 18th and 19th centuries, experimentalists like advanced practical applications through his 1797 investigations into fluid flow through constrictions, demonstrating pressure drops consistent with the principle in hydraulic setups and inspiring devices for . By the 1800s, the principle gained recognition as a manifestation of for ideal fluids, with scholars integrating it into thermodynamic contexts while distinguishing it from the more comprehensive Navier-Stokes equations, which account for and account for the principle's limitations in real, dissipative flows. The 20th century saw the principle's integration into , notably in Ludwig Prandtl's 1904 theory, which relied on Bernoulli's inviscid approximations for outer flow regions while addressing viscous effects near surfaces, enabling accurate predictions of lift and drag in . This evolution underscored the principle's enduring role as a foundational tool in , bridging 18th-century to modern engineering analyses.

Mathematical Formulations

Incompressible Flow

Bernoulli's principle in the context of incompressible flow applies to fluids that do not change density, such as liquids or low-speed gases, under specific conditions. The key assumptions are that the flow is steady (no time variation), inviscid (no viscosity or friction), incompressible (constant density ρ\rho), and analyzed along a single streamline. These conditions simplify the analysis to conservation of energy without dissipative losses or density variations. The Bernoulli equation for such flow states that along a streamline, the sum of , per unit volume, and energy per unit volume remains constant: P+12ρv2+ρgh=constantP + \frac{1}{2} \rho v^2 + \rho g h = \text{constant} where PP is the , vv is the , hh is the above a reference level, and gg is the acceleration due to gravity. This form, originally conceptualized by in his 1738 work , expresses the conservation of for the element. Each term in the equation represents : PP is the energy per unit volume, 12ρv2\frac{1}{2} \rho v^2 is the or per unit volume, and ρgh\rho g h is the per unit volume. The units are consistent in pascals (Pa) or N/m², confirming the equation's balance as total per unit volume. For horizontal flows where elevation changes are negligible (h1=h2h_1 = h_2), the equation simplifies to: P+12ρv2=constantP + \frac{1}{2} \rho v^2 = \text{constant} This form highlights the inverse relationship between pressure and velocity, central to many engineering applications. A representative example is the pressure drop in a narrowing pipe carrying water (ρ=1000\rho = 1000 kg/m³). Consider steady horizontal flow where the cross-sectional area decreases, causing velocity to increase from v1=1v_1 = 1 m/s to v2=2v_2 = 2 m/s by continuity. Assuming constant total pressure, the pressure decreases by ΔP=12ρ(v22v12)=12×1000×(41)=1500\Delta P = \frac{1}{2} \rho (v_2^2 - v_1^2) = \frac{1}{2} \times 1000 \times (4 - 1) = 1500 Pa, illustrating the Venturi effect.

Compressible Flow

Bernoulli's principle extends to compressible flows under specific assumptions, including inviscid conditions, steady flow, and isentropic processes, where the flow is reversible and adiabatic with constant . These assumptions allow variations with and , which are negligible in incompressible cases but critical at high speeds. For such flows, the principle takes the form v22+dPρ+gz=constant,\frac{v^2}{2} + \int \frac{dP}{\rho} + g z = \text{constant}, where vv is the flow speed, ρ\rho is , PP is , gg is , and zz is ; the integral term accounts for compressible effects by relating pressure changes to density variations. Under isentropic conditions, the thermodynamic relation dh=dP/ρdh = dP / \rho (from Tds=dhdP/ρT ds = dh - dP / \rho with ds=0ds = 0) simplifies this to the enthalpy-based equation h+v22+gz=constant,h + \frac{v^2}{2} + g z = \text{constant}, where hh is the specific , representing the total energy per unit mass along a streamline. For ideal gases undergoing isentropic compression or expansion, these equations connect directly to the Mach number M=v/aM = v / a, where aa is the speed of sound. The stagnation pressure P0P_0 (pressure at zero velocity) relates to the local pressure PP by PP0=(1+γ12M2)γ/(γ1),\frac{P}{P_0} = \left(1 + \frac{\gamma - 1}{2} M^2 \right)^{-\gamma / (\gamma - 1)}, with γ\gamma as the specific heat ratio (e.g., γ=1.4\gamma = 1.4 for air); this formula quantifies how pressure drops with increasing speed in compressible regimes, unlike the linear 12ρv2\frac{1}{2} \rho v^2 term in incompressible flow. Similar relations hold for temperature and density ratios, emphasizing the role of thermal effects in high-Mach flows. This formulation breaks down in the presence of shock waves or other non-isentropic processes, such as those involving irreversibilities like or , where increases and the constant total no longer holds uniformly.

Unsteady Potential Flow

In unsteady , the assumptions are that the fluid is inviscid and irrotational, allowing the velocity field v\mathbf{v} to be expressed as the of a ϕ\phi, such that v=ϕ\mathbf{v} = \nabla \phi and ×v=0\nabla \times \mathbf{v} = 0. These conditions apply to both compressible and incompressible flows, with as a conservative . The unsteady Bernoulli equation for such flows is derived from the Euler equations by integrating the momentum balance, yielding ϕt+12ϕ2+dPρ+gz=f(t)\frac{\partial \phi}{\partial t} + \frac{1}{2} |\nabla \phi|^2 + \int \frac{dP}{\rho} + g z = f(t), where ϕt\frac{\partial \phi}{\partial t} represents the temporal , dPρ\int \frac{dP}{\rho} accounts for pressure work, gzg z is the , and f(t)f(t) is an arbitrary function of time uniform throughout the domain. This form holds everywhere in the flow field, not just along streamlines, due to the irrotational nature. For incompressible flows, where density ρ\rho is constant, the equation simplifies to ϕt+12v2+Pρ+gz=f(t)\frac{\partial \phi}{\partial t} + \frac{1}{2} v^2 + \frac{P}{\rho} + g z = f(t), with v=vv = |\mathbf{v}|. This version is particularly useful for analyzing time-varying phenomena without density variations. Physically, the ϕt\frac{\partial \phi}{\partial t} term captures the local rate of change of the velocity potential, reflecting unsteadiness such as accelerating fluid particles in dynamic environments, which modifies the balance between kinetic energy, pressure, and potential energy compared to steady flows. A representative application is in the analysis of small-amplitude water waves under theory, where the linearized unsteady Bernoulli equation at the relates to wave elevation: pd=ρϕt=ρgηp_d = -\rho \frac{\partial \phi}{\partial t} = \rho g \eta, with η\eta as the surface displacement, enabling computation of wave-induced pressures and forces on structures.

Derivations

From Euler's Equations

The Euler equations describe the motion of an inviscid fluid, given by vt+(v)v=1ρP(gh),\frac{\partial \mathbf{v}}{\partial t} + (\mathbf{v} \cdot \nabla) \mathbf{v} = -\frac{1}{\rho} \nabla P - \nabla (g h), where v\mathbf{v} is the velocity vector, ρ\rho is the fluid density, PP is the , gg is the , and hh is the above a reference level. This form incorporates the material acceleration on the left and the and gravitational on the right. To derive Bernoulli's principle, apply the vector identity (v)v=(v22)v×(×v),(\mathbf{v} \cdot \nabla) \mathbf{v} = \nabla \left( \frac{v^2}{2} \right) - \mathbf{v} \times (\nabla \times \mathbf{v}), where v=vv = |\mathbf{v}| and ×v=ω\nabla \times \mathbf{v} = \boldsymbol{\omega} is the . Substituting this into the Euler equations yields vt+(v22)v×ω=1ρP(gh).\frac{\partial \mathbf{v}}{\partial t} + \nabla \left( \frac{v^2}{2} \right) - \mathbf{v} \times \boldsymbol{\omega} = -\frac{1}{\rho} \nabla P - \nabla (g h). For steady flow (v/t=0\partial \mathbf{v}/\partial t = 0), take the of this equation with the differential displacement vector dld\mathbf{l} along a streamline, where dld\mathbf{l} is parallel to v\mathbf{v}. The term v×ωdl=0\mathbf{v} \times \boldsymbol{\omega} \cdot d\mathbf{l} = 0 because it is to the streamline direction. Integrating along the streamline from to point 2 gives 12(v22)dl+121ρPdl+12(gh)dl=0,\int_1^2 \nabla \left( \frac{v^2}{2} \right) \cdot d\mathbf{l} + \int_1^2 \frac{1}{\rho} \nabla P \cdot d\mathbf{l} + \int_1^2 \nabla (g h) \cdot d\mathbf{l} = 0, which simplifies to v222v122+12dPρ+g(h2h1)=0.\frac{v_2^2}{2} - \frac{v_1^2}{2} + \int_1^2 \frac{dP}{\rho} + g (h_2 - h_1) = 0. Thus, v22+dPρ+gh=constant along the streamline,\frac{v^2}{2} + \int \frac{dP}{\rho} + g h = \text{constant along the streamline}, assuming barotropic flow where ρ=ρ(P)\rho = \rho(P), allowing the pressure integral to depend only on the endpoints. For irrotational flow (ω=0\boldsymbol{\omega} = 0), the equation holds not just along a single streamline but between any two points in the flow field, as the term vanishes everywhere and the constant is uniform. In the unsteady case with irrotational flow, where v=ϕ\mathbf{v} = \nabla \phi and ϕ\phi is the , the derivation includes the local term as v/t=(ϕ/t)\partial \mathbf{v}/\partial t = \nabla (\partial \phi / \partial t). Integrating similarly along a path yields the unsteady Bernoulli : ϕt+v22+dPρ+gh=constant (may vary with time).\frac{\partial \phi}{\partial t} + \frac{v^2}{2} + \int \frac{dP}{\rho} + g h = \text{constant (may vary with time)}. This extends the steady form by accounting for temporal changes in the potential.

From Energy Considerations

Bernoulli's principle can be derived from the conservation of mechanical energy applied to a fluid particle or a control volume in steady flow, where the work done by pressure forces balances the changes in kinetic and potential energy of the fluid. In this approach, consider a fluid element moving along a path; the net work performed by surrounding pressure forces on the element equals the increase in its kinetic energy plus the change in gravitational potential energy, assuming no dissipative losses. This energy balance reflects the first law of thermodynamics for a system without heat transfer or shaft work. For incompressible, steady flow of an inviscid fluid, the pressure work term arises from the integral of pressure over the volume displacement, PdVρ\int \frac{P \, dV}{\rho}, which simplifies under constant density ρ\rho to Pρ\frac{P}{\rho} when evaluated between two points. Combining this with the kinetic energy change 12v2\frac{1}{2} v^2 and potential energy ρgh\rho g h, the resulting equation is: P+12ρv2+ρgh=constant,P + \frac{1}{2} \rho v^2 + \rho g h = \text{constant}, where PP is pressure, vv is velocity, gg is gravitational acceleration, and hh is elevation, all evaluated along a streamline. This form holds for fluids like liquids where density variations are negligible. The derivation assumes steady flow (no time-varying properties), inviscid conditions (no or effects), (constant ), and no or external work. These conditions ensure that mechanical energy is conserved without conversion to . For compressible flows, such as in gases, the energy balance incorporates changes in due to density variations. Under adiabatic and reversible (isentropic) conditions, leads to conservation of total , yielding: h+v22+gh=constant,h + \frac{v^2}{2} + g h = \text{constant}, where hh is the specific , which for an is cpTc_p T with constant specific heat cpc_p and TT. This form accounts for thermodynamic work in compressing or expanding the fluid. This energy-based derivation requires the flow to be reversible, meaning no entropy generation from shocks, friction, or heat transfer; it does not apply to dissipative or irreversible processes where energy is lost to heat. In such cases, additional terms for losses must be included, modifying the constant to account for non-conservative effects.

Applications

In Aerodynamics

Bernoulli's principle plays a central role in generating lift on by establishing differences arising from variations in over the wing's curved surfaces. In subsonic flight, air flowing over the upper surface of a cambered travels faster than over the lower surface due to the of the , which accelerates the flow over the curved upper surface through the effects of circulation and the Coanda effect, resulting in lower above the wing and higher below, as dictated by the principle that an increase in fluid corresponds to a decrease in . This net upward force, known as lift, is a direct consequence of these differentials. Within the framework of potential flow theory, the lift generated by an airfoil is quantitatively linked to circulation through the Kutta-Joukowski theorem, which states that the lift per unit span is given by L=ρVΓL' = \rho V_\infty \Gamma, where ρ\rho is the fluid density, VV_\infty is the freestream velocity, and Γ\Gamma is the circulation around the . The ensures smooth flow off the trailing edge, fixing the circulation value and enabling velocity fields that satisfy irrotational flow assumptions. Bernoulli's equation then relates these velocities to pressure distributions along streamlines, with higher velocities on the upper surface producing the requisite low-pressure region for lift. This integration of circulation theory with Bernoulli's principle provides a foundational for airfoil performance in inviscid, incompressible approximations. High-lift devices, such as trailing-edge flaps, enhance aerodynamic performance during takeoff and landing by altering the airfoil geometry to increase effective camber and circulation. When deployed, flaps deflect downward, accelerating airflow over the upper surface and creating steeper velocity gradients, which, per Bernoulli's principle, amplify the pressure differential across the wing and boost lift coefficients by up to 80-100% compared to clean configurations. This increase in circulation, as predicted by the Kutta-Joukowski , allows to operate at lower speeds without stalling, though it also elevates drag. In supersonic , Bernoulli's principle is adapted through its compressible form for isentropic flow regions, such as Prandtl-Meyer expansion fans that occur at convex corners on airfoils or nozzles, where flow accelerates and decreases continuously across the fan without entropy increase. For shock waves, which are non-isentropic and involve abrupt deceleration and rise, the principle does not apply directly across the discontinuity due to total losses, but it informs the upstream and downstream conditions in conjunction with Rankine-Hugoniot relations. These adaptations enable of -velocity trades in high-speed flows around supersonic wings, where expansion fans on the upper surface contribute to lift by lowering . The historical application of these concepts is evident in the ' 1903 glider designs, which implicitly incorporated pressure-velocity trade-offs akin to Bernoulli's principle through empirical testing of curved wing surfaces to achieve sufficient lift for controlled flight. Their iterative experiments with shapes demonstrated faster flow over the upper surface yielding lower and upward , enabling the first sustained powered flight later that year without explicit reference to the principle but aligning with its physical basis.

In Hydrodynamics and Devices

In hydrodynamics, Bernoulli's principle finds extensive application in devices that exploit the relationship between velocity and in incompressible liquid flows. The , a direct consequence of the principle, occurs when a fluid accelerates through a in a pipe, leading to a decrease in at the narrow section while velocity increases to conserve mass flow. This phenomenon is utilized in Venturi meters to measure liquid flow rates by detecting the pressure differential across the , which correlates with velocity via the and Bernoulli's relation. Similarly, in carburetors for systems, the Venturi creates low to draw into the airstream, facilitating atomization and mixing, though primarily in hybrid air-liquid contexts. Pitot tubes provide a practical means to measure in liquids, such as in or channels, by capturing the difference between (where flow is brought to rest) and . The device consists of a tube aligned with the flow to sense total pressure P0P_0 and a port for PP, yielding v=2(P0P)/ρv = \sqrt{2 (P_0 - P)/\rho}
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