Body force Created 2026-09-24 Updated 2026-10-13
A body force acts throughout a body's or fluid's volume, rather than only through its surface. Gravity is the example used in hydrostatic pressure: a gravitational field gives force per unit volume , where is the mass density. More generally, a body force per unit mass contributes to momentum conservation. Forces from electromagnetism are another example. Surface pressure forces produce buoyancy on an immersed body, while its body force from gravity acts downward.
Buoyancy Created 2026-09-28 Updated 2026-10-13
Buoyancy is the resultant upward force exerted by a resting fluid on an immersed body in a downward gravitational field. The fluid pushes inward, perpendicular to each part of the body's surface. Because hydrostatic pressure increases with depth, the upward push from below exceeds the downward push from above. Opposite horizontal forces cancel; buoyancy is the remaining vertical force. A sinking body still receives this upward support. [ref]
More precisely, pressure on a small surface of area with outward unit normal vector exerts
The minus sign says the force points into the body. On a cube, the top force points down, the bottom force points up, and the side forces cancel in pairs because opposite sides have the same pressure at each depth. This is a surface traction; gravity on the body itself is a separate body force. [ref]
For a computed example, stipulate resting water with constant mass density and uniform gravitational acceleration . A fully immersed cube has side , top depth and bottom depth . Each horizontal face has area , and its volume is . Its top and bottom gauge pressures are
The corresponding forces relative to the common surface pressure are downward and upward. Therefore the net buoyancy is
Using absolute pressures adds the same to both face forces, leaving their difference unchanged. Zero gauge pressure at the surface does not mean zero absolute pressure. Increasing both depths by the same amount also leaves buoyancy unchanged in this constant-mass density model.
Figure 1.
How a hydrostatic pressure difference supports an immersed cube
. Left: a fully immersed cube of side has its top at depth and bottom at . The inward pressure forces on its sides cancel; its horizontal faces have area . The displayed face forces use gauge pressure, whose common surface offset cancels in the net upward buoyancy. Right: gauge pressure increases linearly with depth, marking at the top and at the bottom. Details.
Archimedes' principle turns this calculation into a rule for bodies of any shape. It explains floating equilibrium and lets us infer an immersed body's volume from the difference between its force from gravity and the force needed to support it. In particular, buoyancy depends on the displaced volume and the surrounding mass density, whereas the body's own mass density decides how its force from gravity compares with that support.
Equivalence principle Created 2026-09-28 Updated 2026-10-13
The equivalence principle states that gravity couples universally to energy-momentum and that a freely falling local frame removes uniform gravitational acceleration at a point. Tidal curvature remains measurable over a finite region.
Imagine releasing a ball inside a small falling elevator. Relative to the cabin it initially floats, because cabin and ball share the same free fall. The weak equivalence principle says this trajectory is independent of the test particle's composition for identical initial conditions. The Einstein equivalence principle further identifies local nongravitational experiments with those of special relativity. It is a statement about experiments in a local inertial frame, not just equality of two masses.
The word local is essential. Coordinates can make the metric tensor equal to the Minkowski metric and its first derivatives vanish at one event. They generally cannot erase the Riemann curvature tensor, which involves second derivatives. Two separated balls can therefore approach or recede even inside the falling cabin. A sufficiently extended experiment detects these tidal forces; a long observation can accumulate them even when the cabin is small. The equivalence principle does not identify an entire planetary gravitational field with acceleration in flat spacetime. See Tong's discussion of normal coordinates and local equivalence.
Gravity 2026-10-13
Gravity governs falling bodies and orbits. Newtonian gravity describes it through a gravitational field acting on masses; general relativity instead relates matter and radiation to the geometry of spacetime through the Einstein field equations.
Hydrostatic pressure Created 2026-09-24 Updated 2026-10-13
Hydrostatic pressure is the pressure distribution in a resting fluid, balancing its body force from gravity. Take upward and a uniform downward gravitational field , where . The vertical pressure gradient satisfies
A short derivation balances the vertical forces on a thin horizontal layer of area and thickness : . Dividing by and taking the derivative gives the equation above. For constant mass density , integration from the surface at gives
Thus pressure increases with depth . For the stipulated water with mass density and gravitational acceleration , depths and give gauge pressures and . Their difference produces the buoyancy of the example cube. [ref]
For an ordinary stationary laboratory sample, a useful convention is
The bulk kinetic energy includes organized whole-body motion; for pure translation it is , with total mass and center of mass speed . The external potential energy includes elevation in an imposed gravitational field, approximately in a uniform field. Accelerating a sealed bottle or lifting it without otherwise changing its state changes these mechanical terms, rather than its internal energy. Molecular kinetic energy is measured relative to the chosen bulk motion.[ref]
State the convention rather than applying this separation blindly. If an experiment separately tracks a rotating apparatus or an organized flow, its mechanical kinetic energy must not also be counted in . In Joule's paddle-wheel experiment, waiting for the apparatus and fluid to come to rest removes such an endpoint ambiguity. Including the vessel and paddle changes whose internal energy is measured; including the falling weights additionally puts their changing gravitational potential energy inside the enlarged system's total energy balance.
Neutral buoyancy 2026-10-14
Neutral buoyancy means a fully immersed body's upward buoyancy equals its downward force from gravity. For a body of fixed volume in a constant-mass density fluid under a uniform gravitational field, this occurs when its mean mass density equals the surrounding mass density. A cube of mass density in the stipulated water has mass , so both forces are .
Ideally it can remain at rest at any depth for which it stays fully immersed and clear of boundaries. Raising or lowering it changes the absolute pressure, but neither its displaced volume nor the difference between the vertical pressure forces. There is therefore no vertical restoring force toward a preferred depth in this model. Neutral buoyancy is a vertical force balance, not a claim about resistance to tilting or about a compressible body whose volume changes with pressure.
Model the assembly as a heavy symmetric top with a fixed frictionless support, a uniform gravitational field, and centre of mass on its symmetry axis. Assume constant spin, negligible damping, and initial conditions prepared for uniform precession of a heavy symmetric top. Large spin means the transverse angular momentum from precession is small: . Also require . A large spin rate alone does not select steady motion after an arbitrary release.
For an original illustrative calculation, stipulate
The transverse principal moments of inertia are about the pivot, including the parallel axis theorem contribution. These inputs give
The ratio is small; the more direct angular momentum ratio is small too. These are model calculations, not experimental results.
Check the approximation against the existing exact uniform precession of a heavy symmetric top condition. Its total angular momentum is
At constant , differentiating this expression and equating it to the gravitational torque gives
For the slow solution can be evaluated without subtracting two nearly equal numbers:
It exceeds by about . The other solution is about and violates the assumed slow precession; the quadratic's two roots must not be conflated. Its discriminant must be nonnegative for these steady solutions to exist.
Figure 1.
Synthetic steady-precession calculations: larger spin slows the drift and larger transverse torque speeds it up
. Details.
The original curves hold fixed and vary spin and the imposed torque coefficient in . For gravity alone, ; the other curves are hypothetical changes in the transverse torque, not observations of this wheel. Solid curves use the slow quadratic root; dashed curves use . The second panel displays their relative difference. Increasing spin improves this approximation for the parameters shown. It does not remove nutation caused by inappropriate initial conditions.