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Nalanda

Curriculum

Physics

48 entries across 5 tiers. Each tier builds on the tiers before it, so read top to bottom and every idea arrives after its prerequisites. Where an entry has entries to read first, they are listed under it.

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T0 Primitives and observation

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T1 Core relationships and structures

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  • Action-reaction pairs

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    • Force as interaction Defining force as something that always involves two bodies is what makes the pairing of forces on those two bodies almost automatic.
  • Force as interaction

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    • Inertia and the persistence of motion Naming force as whatever changes an object's motion away from its inertial state requires first establishing that unforced motion persists rather than needing continuous cause.
  • Mass as resistance to acceleration
  • The relation between force, mass, and acceleration

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    • Force as interaction You need a clean, interaction-based notion of force before you can ask how much acceleration a given force produces in a given object.
    • Mass as resistance to acceleration Mass is the proportionality constant that links force and acceleration, so it must be defined before that relation can be derived rather than merely stated.
  • Universal gravitation

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  • Weight and gravitational interaction
  • Conservation of mechanical energy

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    • Kinetic energy Mechanical energy conservation is the claim that kinetic energy plus potential energy stays constant, which requires kinetic energy to be defined first.
    • Potential energy and configuration You cannot track the exchange between motion and configuration until configuration itself has a quantity attached to it.
  • Kinetic energy

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    • Work as force through distance Kinetic energy is defined as the work required to accelerate a mass from rest to a given speed, so work must be defined first.
  • Potential energy and configuration
  • Work as force through distance

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  • Kinetic friction and energy loss

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    • Static friction Once the required force exceeds the static maximum, the same contact begins to slide and the kinetic friction regime takes over.
    • Work as force through distance Energy lost to friction is calculated as negative work done by the friction force over the sliding distance.
  • Normal force and contact constraints
  • Static friction

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    • Normal force and contact constraints The maximum available static friction is set as a fraction of the normal force, so sticking cannot be analyzed without first solving for the normal force.
  • Tension in strings and cables

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  • Acceleration

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    • Speed and velocity Acceleration is defined as the rate of change of velocity, so velocity must be a settled, directed quantity before a rate of change of it means anything.
  • Inertia and the persistence of motion

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    • Physical models and idealization Inertia is only visible once friction and air resistance are idealized away, so grasping idealization is what makes the frictionless case worth imagining at all.
  • Motion graphs

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    • Acceleration Reading acceleration as the slope of a velocity time graph, and displacement as area under it, requires the definition of acceleration to already be in hand.
    • Speed and velocity Reading a velocity value off the slope of a position time graph requires already knowing that velocity is a rate, not a raw distance covered.
  • Position, distance, and displacement

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  • Speed and velocity

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  • Two-dimensional motion and projectiles

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    • Acceleration Projectile motion is built from a constant downward acceleration acting alongside an unaccelerated horizontal velocity, so the concept of acceleration must precede combining the two.
    • Motion graphs Predicting a projectile path by combining independent horizontal and vertical motions is easiest to check by reasoning about each motion's own position and velocity time graph first.
    • Position, distance, and displacement Decomposing a curved path into independent horizontal and vertical parts requires treating displacement as a vector with components in the first place.
    • Vectors as directed quantities Position, velocity, and acceleration in more than one dimension are vector quantities, and projectile motion is the standard first place they are combined.
  • Elastic and inelastic collisions

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    • Impulse and force over time The impulse each body exerts on the other during contact is what changes their individual momenta in a collision.
    • Kinetic energy Collisions are classified by how much kinetic energy survives the impact, so comparing kinetic energy before and after is the basic diagnostic tool.
    • Momentum as quantity of motion Every collision analysis starts from the conserved total momentum of the colliding bodies.
  • Impulse and force over time

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  • Momentum as quantity of motion

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  • Circular motion and inward acceleration

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    • Angles, rotation, and radians Angular speed and linear speed around a circular path are related through the radian definition of angle established here.
    • Circles, radius, and pi Describing motion around a circular path requires the radius and circumference relationships established here to connect rotational and linear quantities.
    • Two-dimensional motion and projectiles Circular motion is understood by the same trick of splitting motion into components under a known acceleration, here applied to a constantly redirected rather than constantly downward acceleration.
  • Angular momentum

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  • Center of mass and balance

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    • Rotational inertia How mass is distributed around a pivot, the same fact that sets rotational inertia, also determines where a body's effective balance point sits.
  • Rotational inertia

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    • Torque and rotational effect Rotational inertia is defined as the constant relating torque to angular acceleration, so torque must be established first.
  • Static equilibrium

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    • Angular momentum A body with zero net torque and no changing angular momentum is the rotational half of the equilibrium condition.
    • Center of mass and balance Whether a supported body stays at rest depends on whether the center of mass sits over the base of support, making it a direct input to equilibrium reasoning.
    • Tension in strings and cables Suspended loads and cable systems are among the standard worked cases of bodies held motionless by balanced forces, including tension.
    • Torque and rotational effect True rest requires zero net torque as well as zero net force, so equilibrium reasoning depends on torque being defined.
  • Torque and rotational effect

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T2 Mechanisms and transformations

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  • Conduction, convection, and radiation

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    • The second law and irreversibility All three heat transfer mechanisms move energy spontaneously from hot to cold and never reverse on their own, which is the second law playing out in a concrete setting.
  • Heat as energy transfer

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  • Internal energy

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    • Heat as energy transfer To write a correct energy account for a system you must first be able to separate heat, energy crossing a boundary, from the energy already stored inside.
  • Phase transitions
  • Pressure from microscopic collisions
  • Temperature as microscopic energy distribution
  • The first law of thermodynamics

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    • Heat as energy transfer The first law is a bookkeeping statement about heat and work, so heat must first be defined as a process quantity rather than a stored one.
    • Internal energy The first law states how internal energy changes in terms of heat and work, so internal energy must first be defined as the thing being tracked.
  • The ideal gas model

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    • Dimensional analysis in physics Confirming that a proposed relation among pressure, volume, and temperature is dimensionally consistent is the first filter a physical model must pass before its predictions are trusted.
    • Physical models and idealization Treating gas molecules as point particles with no volume and no attraction between them is an explicit idealization whose stated scope this entry teaches how to evaluate.
    • Pressure from microscopic collisions This derivation of pressure from molecular collisions is the exact mechanism combined with temperature to produce the ideal gas law.
    • Temperature as microscopic energy distribution The ideal gas law ties pressure, volume, and temperature together, and that link only makes sense once temperature is understood as molecular kinetic energy.
  • The second law and irreversibility

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    • Kinetic friction and energy loss Friction converting organized kinetic energy into disorganized heat is the clearest mechanical example of the one-way arrow the second law generalizes.
    • The first law of thermodynamics The first law establishes that energy is conserved in every process; the second law then adds the further constraint on which conserving processes can actually occur.

T3 Systems and interaction

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  • Damping, driving, and resonance

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    • Oscillation and restoring forces Resonance is what happens when a periodic push meets a system's own restoring behavior, so the undamped oscillator's natural frequency has to exist as a concept before energy loss and driving can be layered onto it.
  • Oscillation and restoring forces

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    • Conservation of mechanical energy The back-and-forth exchange between kinetic and potential energy is the energy account of every oscillator.
    • Second-order dynamics The spring and pendulum equations derived here are the mathematical skeleton underneath the physical account of restoring forces and oscillation.
    • Springs, dampers, and suspension The spring's linear restoring force introduced here is the mechanism a later treatment of oscillation generalizes into periodic motion.
  • Waves as travelling disturbances

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    • Oscillation and restoring forces A travelling wave is a chain of oscillators handing motion to their neighbors, so the behavior of one oscillator in isolation is the unit a wave is assembled from.

T5 Advanced synthesis and limits

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  • Orbit as continuous free fall

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    • Angular momentum Orbital motion under a central force conserves angular momentum, which is why orbiting bodies speed up near closest approach and slow down far away.
    • Universal gravitation Orbital motion is the case of continuous free fall under exactly the inverse-square gravitational force this entry derives.
Physics curriculum · Nalanda