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UVAS DVM Admission Test Physics Syllabus

The Physics syllabus for UVAS DVM Admission Test in full: 13 chapters and 43 topics, every one listed below, plus 50 Physics flashcards with answers.

13Chapters
43Topics
50Flashcards

Physics syllabus: all 13 chapters

Expand any chapter to see its topics and sub-topics.

  1. Vectors and Equilibrium

    3 topics
    • Scalars and vectors
    • Addition of vectors
    • Torque and equilibrium
  2. Force and Motion

    4 topics
    • Newton's laws of motion
    • Equations of motion
    • Projectile motion
    • Momentum and impulse
  3. Work, Energy and Power

    4 topics
    • Work and energy
    • Conservation of energy
    • Absolute potential energy
    • Power and efficiency
  4. Rotational and Circular Motion

    3 topics
    • Angular displacement and velocity
    • Centripetal force
    • Moment of inertia
  5. Fluid Dynamics

    3 topics
    • Viscosity and terminal velocity
    • Bernoulli's equation
    • Applications of fluid flow
  6. Waves

    4 topics
    • Progressive waves
    • Stationary waves
    • Sound and the Doppler effect
    • Superposition and interference
  7. Thermodynamics

    4 topics
    • Kinetic theory of gases
    • First law of thermodynamics
    • Second law and entropy
    • Heat engines
  8. Electrostatics

    3 topics
    • Coulomb's law
    • Electric field and potential
    • Capacitors
  9. Current Electricity

    3 topics
    • Ohm's law and resistance
    • Electrical circuits and Kirchhoff's laws
    • Electrical power
  10. Electromagnetism

    3 topics
    • Magnetic field and force on a conductor
    • Motion of charged particles in fields
    • Electromagnetic devices
  11. Electromagnetic Induction and AC

    3 topics
    • Faraday's law of induction
    • Lenz's law
    • Alternating current
  12. Electronics

    3 topics
    • Semiconductors and diodes
    • Rectification
    • Transistors and logic gates
  13. Modern and Nuclear Physics

    3 topics
    • Quantum theory and photoelectric effect
    • Atomic spectra
    • Nuclear physics and radioactivity

UVAS DVM Admission Test Physics flashcards — 50 questions with answers

  1. What is the difference between a scalar and a vector quantity?

    A scalar has only magnitude (e.g. mass, speed, energy), while a vector has both magnitude and direction (e.g. displacement, velocity, force).

  2. Give three examples each of scalar and vector quantities.

    Scalars: mass, temperature, energy, speed, time. Vectors: displacement, velocity, acceleration, force, momentum.

  3. How is a vector resolved into rectangular components?

    For a vector F at angle θ to the x-axis: Fx = F cosθ and Fy = F sinθ. The vector is split into perpendicular x and y components.

  4. How do you find the magnitude and direction of a vector from its components Fx and Fy?

    Magnitude F = √(Fx² + Fy²); direction θ = tan⁻¹(Fy/Fx) measured from the x-axis.

  5. State the head-to-tail (triangle) rule for vector addition.

    Place the tail of the second vector at the head of the first; the resultant is the vector drawn from the tail of the first to the head of the last vector.

  6. How is the resultant of two vectors A and B at angle θ found (parallelogram law)?

    R = √(A² + B² + 2AB cosθ), with direction tan α = (B sinθ)/(A + B cosθ) relative to A.

  7. What is the resultant of two perpendicular vectors of magnitudes 3 and 4?

    R = √(3² + 4²) = √25 = 5 units.

  8. Define torque (moment of a force) and give its formula.

    Torque is the turning effect of a force about an axis: τ = r F sinθ = Force × perpendicular distance (moment arm). SI unit: N·m.

  9. State the two conditions for complete equilibrium of a body.

    1st condition: net force is zero (ΣF = 0). 2nd condition: net torque is zero (Στ = 0).

  10. What are the three states/types of equilibrium?

    Stable (returns to original position), unstable (moves further away when disturbed), and neutral (stays in new position).

  11. State Newton's first law of motion.

    A body remains at rest or in uniform motion in a straight line unless acted upon by a net external force (law of inertia).

  12. State Newton's second law of motion and its equation.

    The rate of change of momentum is proportional to the applied force and in its direction: F = ma (or F = Δp/Δt).

  13. State Newton's third law of motion.

    For every action there is an equal and opposite reaction; the two forces act on different bodies.

  14. Define inertia.

    Inertia is the property of a body to resist any change in its state of rest or uniform motion; it is measured by the body's mass.

  15. Write the three equations of motion for uniform acceleration.

    vf = vi + at; S = vi t + ½ a t²; vf² = vi² + 2aS.

  16. What is the acceleration and velocity-time relationship for a freely falling body?

    Acceleration = g (≈ 9.8 m/s² downward). v = gt, h = ½gt², and v² = 2gh, taking initial velocity zero.

  17. Define projectile motion.

    Two-dimensional motion of a body under gravity alone, having a constant horizontal velocity and a uniformly accelerated vertical motion.

  18. For a projectile launched at velocity v and angle θ, what are the horizontal and vertical velocity components?

    Horizontal: vx = v cosθ (constant). Vertical: vy = v sinθ − gt (changes with time).

  19. Write the formula for the time of flight of a projectile launched at angle θ with speed v.

    T = (2v sinθ)/g.

  20. Write the formula for the maximum height of a projectile.

    H = (v² sin²θ)/(2g).

Show the other 30 Physics flashcards
  1. Write the formula for the horizontal range of a projectile.

    R = (v² sin2θ)/g.

  2. At what launch angle is the horizontal range of a projectile maximum, and what is that range?

    At θ = 45°, range is maximum and equals v²/g (since sin90° = 1).

  3. What is the shape of a projectile's trajectory and the velocity direction at maximum height?

    The trajectory is a parabola; at maximum height the vertical velocity is zero, so velocity is purely horizontal (v cosθ).

  4. Define linear momentum and give its formula and unit.

    Momentum is the product of mass and velocity: p = mv. It is a vector; SI unit is kg·m/s (or N·s).

  5. Define impulse and state its relationship with momentum.

    Impulse = Force × time (F·Δt) and equals the change in momentum: F·Δt = Δp = m(vf − vi). Unit: N·s.

  6. State the law of conservation of momentum.

    In the absence of an external force, the total momentum of an isolated system remains constant before and after a collision/interaction.

  7. What is the difference between elastic and inelastic collisions?

    In an elastic collision both momentum and kinetic energy are conserved; in an inelastic collision momentum is conserved but kinetic energy is not.

  8. Define work and give its formula.

    Work is done when a force moves a body through a displacement: W = F·S·cosθ, where θ is the angle between force and displacement. SI unit: joule (J).

  9. When is the work done by a force zero, maximum, and negative?

    Zero when θ = 90°; maximum (positive) when θ = 0°; negative when θ = 180° (force opposes motion).

  10. Write the formulas for kinetic energy and gravitational potential energy.

    Kinetic energy KE = ½mv²; gravitational potential energy PE = mgh.

  11. State the work-energy theorem.

    The net work done on a body equals the change in its kinetic energy: W = ½mvf² − ½mvi².

  12. State the law of conservation of energy.

    Energy can neither be created nor destroyed; it only changes from one form to another, and the total energy of an isolated system remains constant.

  13. For a body falling freely, how do KE and PE change while total energy stays constant?

    As the body falls, PE decreases and KE increases by an equal amount, keeping total mechanical energy (KE + PE) constant.

  14. What is meant by absolute (gravitational) potential energy?

    It is the work done in bringing a body from infinity to a point in a gravitational field. U = −GMm/r, taken as zero at infinity (hence negative for a bound body).

  15. Write the formula for escape velocity and its approximate value from Earth.

    vesc = √(2GM/R) = √(2gR) ≈ 11.2 km/s for Earth.

  16. Define power and give its formula and SI unit.

    Power is the rate of doing work: P = W/t = F·v. SI unit: watt (W), where 1 W = 1 J/s.

  17. Define efficiency and how it is calculated.

    Efficiency = (useful output energy or power / total input energy or power) × 100%. It is always less than 100% due to energy losses.

  18. Define angular displacement and its SI unit.

    Angular displacement is the angle swept by a rotating body about its axis. SI unit: radian (rad). One revolution = 2π rad.

  19. Define angular velocity and give the relation between linear and angular velocity.

    Angular velocity ω = Δθ/Δt (rad/s). Linear velocity v = rω, where r is the radius.

  20. Write the relation between linear acceleration and angular acceleration.

    a = rα, where α is angular acceleration (rad/s²) and r is the radius of the circular path.

  21. Define centripetal force and give its formula.

    Centripetal force is the net inward force keeping a body in circular motion, directed toward the centre: Fc = mv²/r = mrω².

  22. Define centripetal acceleration and give its formula.

    Centripetal acceleration is directed toward the centre of the circle: ac = v²/r = rω².

  23. Define moment of inertia and its SI unit.

    Moment of inertia is the rotational analogue of mass, the resistance to angular acceleration: I = Σmr². SI unit: kg·m².

  24. Give the moment of inertia of a solid sphere, a thin hoop/ring, and a solid disc about their central axes.

    Solid sphere: I = (2/5)MR². Hoop/ring: I = MR². Solid disc/cylinder: I = ½MR².

  25. Write the formula for rotational kinetic energy and angular momentum.

    Rotational KE = ½Iω²; angular momentum L = Iω. Unit of L: kg·m²/s.

  26. Define viscosity and name the coefficient that measures it.

    Viscosity is the internal friction or resistance to flow between layers of a fluid. It is measured by the coefficient of viscosity η (unit: Pa·s or N·s/m²).

  27. State Stokes' law for the drag force on a sphere moving through a fluid.

    F = 6πηrv, where η is viscosity, r the radius of the sphere, and v its velocity.

  28. Define terminal velocity and write its formula for a sphere falling in a fluid.

    Terminal velocity is the constant maximum velocity attained when drag plus buoyancy balance weight: vt = (2r²(ρ − σ)g)/(9η), where ρ is sphere density and σ fluid density.

  29. State Bernoulli's equation and the principle it expresses.

    P + ½ρv² + ρgh = constant. It states that for an ideal fluid, the sum of pressure energy, kinetic energy, and potential energy per unit volume stays constant; where speed is high, pressure is low.

  30. Define a progressive (travelling) wave and write the wave speed relation.

    A progressive wave transfers energy through a medium without transporting the medium itself. Wave speed v = fλ, where f is frequency and λ is wavelength.

UVAS DVM Admission Test Physics FAQ

What is in the UVAS DVM Admission Test Physics syllabus?

UVAS DVM Admission Test Physics is split into 13 chapters: Vectors and Equilibrium, Force and Motion, Work, Energy and Power, Rotational and Circular Motion, Fluid Dynamics, Waves, Thermodynamics, Electrostatics, Current Electricity, Electromagnetism, Electromagnetic Induction and AC, Electronics and Modern and Nuclear Physics. Together they contain 43 topics.

How many chapters are in UVAS DVM Admission Test Physics?

13 chapters, containing 43 topics. The largest chapter is Force and Motion, with 4 topics.

Are there flashcards for UVAS DVM Admission Test Physics?

Yes — a 50-card Physics deck, printed in full in the flashcards section of this page and available in the Examius app with spaced repetition. The free plan covers one exam of your choice, including its flashcards; Examius Pro, a one-time purchase, unlocks every other exam and deck.