Dynamics Flashcards

1
Q

Define space for Newtonian dynamics

A

Space is Euclidean R^3

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2
Q

Define a reference frame for Newtonian dynamics

A

A choice of origin, O, with orthogonal, right - handed 3D axes at O.

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3
Q

Define a point particle

A

An idealised object modelled as being at position r(t) relative to a reference frame, where t is time.

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4
Q

Define velocity

A

The first derivative of position

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5
Q

Define speed

A

The magnitude of velocity

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6
Q

Define acceleration

A

The second derivative of position

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7
Q

Define linear momentum

A

p = mv

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8
Q

Give Newton’s First Law

A

In an inertial reference frame, a point particle moves with constant momentum, unless acted on by a non-zero total external force.

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9
Q

Give Newton’s Second Law

A

In an inertial reference frame, the dynamics of a point particle satisfies F = dp/dt, where F is the total external force.

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10
Q

Give Newton’s Third Law

A

If particle A exerts a force F on particle B, then particle B exerts the force -F on particle A.

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11
Q

Define the Galilean group

A

The group of combinations of the following transformations on a reference frame:
Translations: r’ = r - x, where x is constant
Rotations: r’ = Rr, where R is a rotation matrix
Galilean boosts: r’ = r - ut, where u is a constant velocity

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12
Q

Give the formula for the Gravitational force near the Earth’s surface

A

F = mg towards the Earth

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13
Q

Give the formula for the Gravitational force between two celestial objects at large distance.

A

F = -G(m_1)(m_2)/(r^2) in the direction towards the other body, where m_1 and m_2 are the masses of the two objects

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14
Q

Give the formula for fluid drag in a viscous fluid

A

F = -6πµRv, where µ is the viscosity, R is the radius of the sphere and v is the velocity.

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15
Q

Give the formula for fluid drag on an aerofoil in air

A

F = - D|v|v, where D is the drag coefficient and v is the velocity.

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16
Q

Give the formula for the spring force

A

F = - k(x - L), where k is the spring constant, x is the length of the spring and L is the natural length of the spring, acting in the direction to return the spring to its natural length.

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17
Q

Give the fomula for the force on a charged particle in electric and magnetic fields.

A

F = qE + q(v^B), where q is charge, m is mass, v is velocity, E is the electric field and B is the magnetic field.

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18
Q

Define the kinetic energy of a point particle

A

T = 1/2.m.(dr/dt)^2

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19
Q

Define the potential energy of a point particle

A

V(x) = - the integral of F(s)ds, from an arbtritary point to the particle’s position.

20
Q

Define an equilibrium solution of Newton II

A

A position x = x_e for all time, so F(x_e) = 0 for all t.

21
Q

Define an equilibrium point

A

A position (x, y, z) = (x_e, y_e, z_e) for all time so F(x, y, z) = G(x_e, y_e, z_e) = 0 for all t.

22
Q

Define a stable equilibrium

A

If m*(d^2ξ/dt^2) = ξF’(x_e), where ξ = x - x_e. The equilibrium at x_e is stable if the solutions to the differential equation are complex. Stable equilibriums are local minimums of the potential.

23
Q

Define the work done by a force

A

The work done by a force F in moving a particle from r_1 to r_2 is the integral of F.dr from r_1 to r_2.

24
Q

Define a conservative force.

A

A force F is conservative if there exists V such that F = −∇V

25
Q

Define a central force

A

A force, F, that is proportional to r, where r is the position vector of a particle relative to the origin of an inertial reference frame.

26
Q

Define angular momentum

A

The angular momentum of a particle about a point P is L_p := (r - x)∧m(dr/dt)

27
Q

Define torque

A

The torque of a force F about a point P with position vector x is τ_p = (r-x)^F, where r is the position of the particle.

28
Q

Give the inverse square law

A

V(r) = -κ/r and F = -κ/r^2(e_r)

29
Q

Give Newton’s Law of Universal Gravitation

A

F = -(G_N)(m_1)(m_2)/|(r_1)-(r_2)| in the direction between the particles.

30
Q

Give Kepler’s 1st Law

A

The path of a planet is an ellipse.

31
Q

Give Kepler’s 2nd Law

A

A straight line joining the Sun and a planet sweeps out equal areas in equal time.

32
Q

Give Kepler’s 3rd Law

A

(Period of an orbit)^2/(Semi major axis of the ellipse)^3 is constant for all planets.

33
Q

Define the centre of mass

A

The point with position vector 1/M times the sum of (m_i)(r_i).

34
Q

Define the total momentum

A

The total momentum of a system of particles is P = M(dR/dt), where R is the centre of mass.

35
Q

Define a closed system

A

A system where the net external force is 0.

36
Q

Define a centre of mass reference frame

A

A reference frame with the origin as the centre of mass.

37
Q

Define the total angular momentum about P.

A

Sum of (r-x)^m(dr/dt), where x is the position of P.

38
Q

Give the strong form of Netwon’s Third Law

A

If particle A exerts a force F on particle B, then particle B exerts the force -F on particle A. Additionally, this force acts along the vector (r_A - r_B).

39
Q

Define the angular velocity of a reference frame.

A

If e_i(dot) = ω ^ e_i, then ω is the angular velocity of the reference frame.

40
Q

Define a rigid body

A

An object where the distribution of mass between any two points is fixed.

41
Q

Define the rest frame

A

The reference frame where r_I are at rest, so [d(r_I)/dt]S = 0.

42
Q

Define the inertia tensor

A

I_ij = Sum of: (m_I)[(r_I.r_I)(δ_ij) - (r_Ii)(r_Ij)]

43
Q

Define rotational kinetic energy

A

The rotational kinetic energy about G is (1/2)ω.(L_G)

44
Q

Define the moment of inertia

A

n^T.I.n, where I is the inertia tensor.

45
Q

Define the principle moments of inertia

A

The eigenvalues of the inertia tensor.