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UndergraduateClassical mechanics


Fluid mechanics


Fluid mechanics is a branch of classical mechanics that deals with the behavior of fluids (liquids, gases, and plasmas) and the forces acting on them. It is the basis of many disciplines such as engineering, atmospheric science, oceanography, and biology. At the undergraduate level, it is essential to develop a strong understanding of fluid mechanics to apply these principles to real-world scenarios.

Liquids

Unlike solids, fluids do not have a fixed shape but take the shape of their container. This is due to their ability to flow. In simple terms, a fluid is a substance that continuously deforms under applied shear stress. Fluids are generally classified into two types:

  • Liquids: Definite volume but no definite shape. For example, water.
  • Gases: Neither definite volume nor definite shape. For example, air.

Fundamentals of Fluid Mechanics

Density and specific gravity

Density is defined as the mass per unit volume of a fluid. It is represented by the symbol ρ (rho). The formula for density is:

ρ = frac{m}{V}

Where:

  • m is the mass of the liquid
  • V is the volume of the liquid

Specific gravity is the ratio of the density of a fluid to the density of a standard reference fluid, usually water for liquids. It is a dimensionless quantity and is often used to compare the densities of substances.

Pressure in liquids

Pressure is the force applied per unit area within a fluid and is measured in pascals (Pa). The formula for pressure is:

P = frac{F}{A}

Where:

  • P is the pressure
  • F is the applied force
  • A is the area over which the force is distributed

In a fluid at rest, pressure increases with depth due to the weight of the fluid above it. It is described by the hydrostatic pressure equation:

P = P_0 + rho gh

Where:

  • P_0 is the atmospheric pressure at the surface
  • ρ is the density of the fluid
  • g is the acceleration due to gravity
  • h is the height (depth) of the fluid

A practical example of this principle is the pressure experienced by a diver underwater, which increases with depth.

Buoyancy and Archimedes' principle

Buoyancy is the upward force applied to an object immersed in a fluid, which counteracts the object's weight. Archimedes' principle states:

The buoyancy force acting on an object is equal to the weight of the fluid displaced by that object.
F_b = rho_f g V_d

Where:

  • F_b is the buoyancy force
  • &rho_f is the fluid density
  • V_d is the volume of the displaced fluid
buoyant force

For example, a ship floats because the buoyancy force acting on it is equal to the force of gravity pulling it down.

Fluid flow

Laminar and turbulent flow

Fluid flow may be classified as either laminar or turbulent depending on the flow behaviour:

  • Laminar Flow: Smooth, orderly flow with parallel layers. Occurs at low velocities.
  • Turbulent flow: Disordered, irregular flow with eddies. Occurs at high velocities.

The Reynolds number (Re) helps predict whether the flow will be laminar or turbulent:

Re = frac{rho v L}{mu}

Where:

  • rho is the density of the liquid
  • v is the velocity of the fluid
  • L is the characteristic length (for example, pipe diameter)
  • mu is the dynamic viscosity of the fluid

If Re is less than 2000, the flow is probably laminar; if greater than 4000, the flow is turbulent.

laminar flow turbulent flow

Continuity equation

The continuity equation expresses the principle of mass conservation in fluid dynamics. It states that for an incompressible fluid, the mass flow rate must remain constant from one cross-section of a tube to another.

A_1 v_1 = A_2 v_2

Where:

  • A_1 and A_2 are the cross section areas
  • v_1 and v_2 are the velocities of the fluid at points 1 and 2

This equation implies that if the cross-sectional area of the pipe decreases, the velocity must increase to conserve the mass flow rate, and vice versa.

Bernoulli's equation

Bernoulli's equation relates pressure, velocity, and height in a flowing fluid, assuming it is incompressible and has no friction. It is expressed as:

P + frac{1}{2}rho v^2 + rho gh = text{constant}

This equation implies that an increase in fluid velocity leads to a decrease in pressure or potential energy, and vice versa. It is often used to explain phenomena such as lift on an airplane wing.

high pressure Low Pressure Air Flow

Viscosity and surface tension

Stickiness

Viscosity is a measure of a fluid's resistance to deformation or flow. It tells how "thick" or "thin" the fluid is. For example, honey has a higher viscosity than water. The viscous force experienced by the fluid layer is given by:

F = mu A frac{dv}{dy}

Where:

  • F is the force due to viscosity
  • mu is the dynamic viscosity of the fluid
  • A is the area of the fluid layer
  • frac{dv}{dy} is the velocity gradient perpendicular to the flow direction

Surface tension

Surface tension is the elastic tendency of the surface of a liquid, which enables it to have the minimum possible surface area. It is due to the cohesive forces between the liquid molecules on the surface.

This property is responsible for phenomena like small insects walking on water and the formation of droplets.

Applications of Fluid Mechanics

  • Hydraulics: Uses the principles of fluid mechanics to design systems such as brakes and elevators.
  • Aerodynamics: This involves the study of air flow, which is important to the design of vehicles and aircraft.
  • Blood Flow in Biology: Understanding blood flow in the cardio-vascular system relies heavily on fluid mechanics.

Overall, the study of fluid mechanics provides important insights into natural systems and technological applications, helping us to design systems efficiently and better understand natural phenomena.


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