Ch 36: Special Relativity

Knight Calc - Physics for Scientists and Engineers 5th Edition

Knight Calc5th EditionPhysics for Scientists and EngineersISBN: 9780137344796Non è quello che usi tu?Cambia libro di testo

Knight Calc 5th Edition

Ch 36: Special Relativity

Problema 63a

Capitolo 36, Problema 63a

A rocket is fired from the earth to the moon at a speed of 0.990c. Let two events be 'rocket leaves earth' and 'rocket hits moon.' In the earth's reference frame, calculate ∆x, ∆t, and the spacetime interval s for these events.

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Step 1: Identify the given values and the quantities to calculate. The rocket's speed is given as 0.990c (where c is the speed of light). The two events are 'rocket leaves earth' and 'rocket hits moon.' In the Earth's reference frame, the distance between the Earth and the Moon (∆x) is approximately 384,400 km. The time interval (∆t) can be calculated using the formula for time: ∆t = ∆x / v, where v is the rocket's speed.

Step 2: Calculate the spatial separation (∆x). Since the problem specifies the Earth's reference frame, the spatial separation is simply the distance between the Earth and the Moon, which is approximately 384,400 km. Convert this distance into meters for consistency with SI units: ∆x = 384,400 × 10³ m.

Step 3: Calculate the time interval (∆t). Use the formula ∆t = ∆x / v, where v = 0.990c. Substitute the values: ∆t = (384,400 × 10³ m) / (0.990 × c). Remember that c = 3.00 × 10⁸ m/s. Perform the division to express ∆t in seconds.

Step 4: Calculate the spacetime interval (s). The spacetime interval is given by the formula: s² = (c∆t)² - (∆x)². Substitute the values for ∆t and ∆x into the equation. Be careful to square each term and ensure the units are consistent. Then, take the square root of s² to find s.

Step 5: Interpret the result. The spacetime interval (s) is an invariant quantity, meaning it is the same in all inertial reference frames. This value provides insight into the relationship between the spatial and temporal separations of the two events in spacetime.

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Relativity of Simultaneity

In the theory of relativity, the simultaneity of events can differ depending on the observer's frame of reference. This means that two events that are simultaneous in one frame may not be simultaneous in another. Understanding this concept is crucial for analyzing events like a rocket leaving Earth and hitting the Moon, as the timing and spatial separation of these events can vary based on the observer's motion.

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Spacetime Interval

The spacetime interval is a measure that combines both spatial and temporal separation between two events in a way that is invariant across different reference frames. It is calculated using the formula s² = c²(∆t)² - (∆x)², where c is the speed of light, ∆t is the time difference, and ∆x is the spatial distance. This concept is essential for understanding how events are related in spacetime, especially in relativistic contexts.

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Lorentz Transformation

The Lorentz transformation equations relate the coordinates of events as observed in different inertial frames moving at a constant velocity relative to each other. These transformations account for the effects of time dilation and length contraction, which are fundamental in special relativity. They allow us to calculate how time intervals and distances change for observers in different frames, which is necessary for solving the problem of the rocket's journey.

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Lorentz Transformations of Velocity

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