All Flashcards
What are the differences between conservative and dissipative forces?
Conservative Forces: Path independent, total work in a closed path is zero. Dissipative Forces: Path dependent, energy is lost from the system (usually as heat).
What are the differences between gravitational potential energy near Earth and at large distances?
Near Earth: Uniform field, (Delta U = mgDelta h). Large Distances: Non-uniform field, (U = -frac{Gm_1m_2}{r}).
What is the definition of Hooke's Law?
The force exerted by an ideal spring is proportional to the displacement from its equilibrium position: (F_s = -k Delta x)
What is the definition of spring constant (k)?
A measure of a spring's stiffness; a larger k means the spring is harder to stretch.
What is the definition of elastic potential energy?
The energy stored in a spring due to its deformation: (U_s = frac{1}{2}k(Delta x)^2)
What is a conservative force?
A force where the work done is independent of the path taken; it only depends on the initial and final positions.
What is the definition of gravitational potential energy near Earth?
The change in potential energy due to a change in height in a uniform gravitational field: (Delta U = mgDelta h)
What is the general formula for gravitational potential energy?
The gravitational potential energy between two masses at a distance r: (U = -frac{Gm_1m_2}{r})
What are the steps to calculate the work done by a conservative force?
- Identify the conservative force. 2. Determine the initial and final positions. 3. Use the formula (W = -Delta U) or (W = int_{a}^{b} F cdot dr).
What are the steps to determine the potential energy stored in a spring?
- Determine the spring constant, k. 2. Measure the displacement from equilibrium, Δx. 3. Use the formula (U_s = frac{1}{2}k(Delta x)^2).
What are the steps to find force from a potential energy graph?
- Determine the potential energy function, U(x). 2. Find the slope of the graph at the point of interest. 3. Take the negative of the slope to find the force: (F = -frac{dU}{dr}).
What are the steps to derive the general formula for gravitational potential energy?
- Start with the definition of work: (W = int_{r_i}^{r_f} F(r) dr). 2. Substitute Newton's Law of Universal Gravitation: (F(r) = frac{Gm_1m_2}{r^2}). 3. Integrate to find the change in potential energy. 4. Set initial potential energy to 0 at infinity.