2P1 Mechanics Flashcards
(39 cards)
How can you simplify a 2DoF mass-spring-mass system, which is not connected to a reference position?
By defining a new coordinate system in terms of the centre of mass, xG, and then rearranging. You can then see the acceleration of xG is 0. d/dt(p1)=0, because the lagranian does not depend on the q1, so there is no generalised force. This is the derivation of the conservation of total momentum.
Under what situation will total energy (E=T+V), be conserved in a Lagrangian system?
When the lagranian does not depend explicitly on time.
How do you find the motion of a 1DoF system?
Use the first integral of the equation of motion.
Multiply the eq of motion by qdot, then integrate with respect to time. This should look like the eq for total energy, which is a constant.
When are you likely to be able to find a conservation law within Lagrangian mechanics?
When there is invarianve under a coordinate. i.e. you can define a new reference coordinate and everything is unchanged.
How do you find equilibrium states in a Lagranian system for a 1DoF system?
Set either the acceleration to 0 or the V’(q) to 0. (same thing in essence)
What is the concept of a phase portrait?
For a system with constant total energy, then you can plot a graph of velocity against position for difference energies. Each line represents 1 value of total energy.
What are characteristic phase portraits from maxima and minima of effective potentials?
Minima, forms close circles (eyes). This is indicative of oscillation)
Maxima, they appear to diverge from, hyperbolic (or parabolic) looking curves).
Higher energy lines go over the top.
What is the generalised form for oscillation in a 1DoF system, with an equilibria q0?
mdqddot = - v’‘(q0) dq = -V’(q0 +dq)
What is the second integral of the equation of motion?
Integrate qdot with respact to time.
qdot = dq/dt = sqrt(2/m(E-V(q))
then seperate variables and integrate
How can the concept of effective potential be applied in a central potential?
Central potential V(r), independent of θ
therefore define h as the pθ, since this is constant.
eq of motion =
mrddot = mr θdot^2 - V’(r) = pθ / (mr^3) - V’(r)
Veff’(r) = V’(r) - pθ/(mr^3)
integrate to find effective potential.
the pθ/2mr^2 is known as the centrifugal potential.
What is the first integral for a single DoF system in terms of effective potential?
0.5 m rdot^2 + Veff(r) = E
How do you find the frequency of oscillation for an effective potential system?
Veff(rmin+dr) = Veff(rmin) + 0.5 V’‘eff(rmin) dr^2
=> V’eff(rmin + dr) = V’‘eff(rmin) dr^2
What is the consequence of oscillation for satellite mechanics?
Circular orbits => elliptical, frequency of vibration is the same as the orbital freuqncy.
What is the conseuqnce of oscillation in the motion around a code?
the angular frequency of radial vibration is dependent on the angle of the cone. If this matches the spinning round the cone, then the motion closes, but if it doesn’t then the motion processes around the cone.
What is the eq for total energy?
E = KE + Veff(q)
What is noted about a bead on a freely rotating hoop?
There is infinite effective potential at θ =0, so no matter how much energy the ball has it cannot cross to the other side of the hoop.
How can you simplify a 2-body problem in 3D space?
Write the lagranian in terms of vectors r1, and r2.
Establish new vectors, rG (centre of mass), and rS (seperation vector).
Seperate these Lagranians into two sub Lagrangians, and then solve these seperately.
What is the general form of the kinetic energy in terms of the mass matrix.
T = 0.5 * qdot ^T *M *qdot
What is the general form of the potential energy in terms of the stiffness matricies?
V(q0) - 0.5 * dq^T K dq
What is the general form of each term of the mass and stiffness matrix?
Evaluated at q=q0
Mij = ∂2T/∂qidot∂qjdot
Kij = ∂2V/∂qi∂qj
In the expanded Lagrangian, why are there no linear terms?
Because we are expanding around a stationary point.
What is the generalised form for normal mode vibration with n degree of freedoms?
dq = sum to n [ Ci Ai cos (ωt + φ) ]
where Ai is the mode shapes
What does ω=0 indicate?
Rigid body mode,
dq = (C1 + C2t)A
where A is the mode shape
Conditions for orthogonal mode shapes?
K and M are both symmetric and one is the multiple of the identity matrix.