Summer 2010 Name Phys 1412 Section Space-Time And Building B

Summer 2010 Name Phys 1412 Section Space Time and Building Blocks of the Universe

Summer 2010 Name Phys 1412 Section Space-Time and Building Blocks of the Universe

Analyze the provided assignment instructions which encompass two primary parts: a science fiction movie review concerning relativity theories and a set of quantum mechanics calculations involving the uncertainty principle and electromagnetic forces in a nucleus. The instructions specify that the student should review relevant chapters, watch or read a sci-fi media, and critically examine the concordance and discrepancies with physical theories. In addition, detailed calculations must be performed in scientific notation with proper explanation and commentary. The objective is to evaluate understanding of relativity concepts, quantum mechanics, and nuclear forces through both qualitative analysis and quantitative problem-solving.

Paper For Above instruction

The exploration of space-time, relativity, and quantum mechanics forms a foundational aspect of modern physics, profoundly influencing our comprehension of the universe. In this essay, I will analyze a science fiction narrative through the lens of established scientific theories, and address quantum mechanics problems that elucidate how fundamental principles such as the uncertainty principle and electromagnetic forces operate at microscopic levels.

Part I: Sci-fi Movie Review

The chosen movie for review is "Interstellar" directed by Christopher Nolan. This film intricately weaves aspects of Einstein's theories of relativity into its plot, particularly highlighting time dilation effects near a black hole. From the movie, the depiction of slow aging and different passage of time on planets close to the black hole are consistent with the predictions of general relativity. The characters' experiences of time dilation are based on the relativistic principle that time runs slower in stronger gravitational fields, as described by Einstein's field equations. This aspect aligns with the theoretical understanding that gravitational potential influences the flow of time, a key component of general relativity.

However, some elements in the film stretch scientific accuracy. For instance, the portrayal of the black hole "Gargantua" with visible accretion disk and gravitational lensing effects are exaggerated for visual impact, though based on real physics. Yet, the extreme speed of the spaceship near light speed, with purported instantaneous travel, violates special relativity's limit that no object with mass can reach or exceed the speed of light. Additionally, the concept of traversing through a higher-dimensional "tesseract" involves speculative physics not established in current theories, thus representing a violation or, at best, an extension of our understanding.

In terms of space and time travel, the characters utilize a wormhole near Saturn to access another part of the universe. Wormholes are theoretically solutions to Einstein’s field equations, representing tunnel-like structures linking distant points in spacetime. While the film correctly conceptualizes these as shortcuts enabled by curved spacetime, the physical realization and stability of wormholes remain speculative. The character's maneuvering through such a structure demonstrates an application of relativistic principles, albeit simplified for entertainment purposes.

In summary, "Interstellar" incorporates and dramatizes different aspects of relativity—such as gravitational time dilation and black hole physics—aligning some elements with scientific theory, while others introduce speculative or exaggerated concepts beyond current scientific consensus.

Part II: Quantum Mechanics Calculation

A. Wave Particle Duality and Uncertainty Principle

1. Wavelength of a moving stone

The mass of the stone is m = 1 g = 0.001 kg. Its velocity is v = 12,000 m/s. The Planck’s constant is h = 6.6 × 10⁻³⁴ J·s.

The momentum p = mv = 0.001 kg × 12,000 m/s = 1.20 × 10¹·1 kg·m/s (which simplifies to 1.20 × 10⁴ kg·m/s).

The wavelength λ = h / p = (6.6 × 10⁻³⁴ J·s) / (1.20 × 10⁴ kg·m/s) = 5.50 × 10⁻³⁸ meters.

Answer: λ ≈ 5.50 × 10⁻³⁸ m

Given the extremely small wavelength, the wave nature of the stone is not observable in everyday life because it is many orders of magnitude smaller than atomic scales. The wave effects are negligible and imperceptible due to the massiveness of macroscopic objects compared to quantum scales.

2. Uncertainty in momentum of a baseball

The baseball's velocity v = 25 m/s, and the uncertainty in position Δx = 500 nm = 5.00 × 10⁻⁷ m.

Applying the uncertainty principle: Δx Δp ≈ h ⇒ Δp ≈ h / Δx = (6.6 × 10⁻³⁴ J·s) / (5.00 × 10⁻⁷ m) = 1.32 × 10⁻²⁷ kg·m/s.

Answer: Δp ≈ 1.32 × 10⁻²⁷ kg·m/s

The mass of the baseball is about 0.145 kg. The momentum uncertainty is very small relative to the classical momentum (p ≈ 0.145 kg × 25 m/s ≈ 3.63 kg·m/s), so the uncertainty is negligible in practical terms. That is why players do not "feel" the quantum uncertainty, as it is insignificant at macroscopic scales.

B. The Strong Force in a Helium Nucleus

a. Electromagnetic Force between Protons

The charges q₁ and q₂ are both 1.6 × 10⁻¹⁹ C, and the distance r = 1.2 × 10⁻¹⁵ m. The Coulomb's law constant is k = 9.0 × 10⁹ N·m²/C².

F_e = (k × q₁ × q₂) / r² = (9.0 × 10⁹ N·m²/C²) × (1.6 × 10⁻¹⁹ C)² / (1.2 × 10⁻¹⁵ m)² = (9.0 × 10⁹) × (2.56 × 10⁻³⁸) / (1.44 × 10⁻³⁰) = (2.304 × 10⁻²⁸) / (1.44 × 10⁻³⁰) ≈ 16.0 N.

Answer: approximately 16.0 N

b. Force Binding the Protons

The strong nuclear force binds protons in the nucleus, overcoming electrostatic repulsion. Its magnitude varies with distance but is generally on the order of 10 N for sub-femtometer ranges, comparable to the calculated repulsive electromagnetic force. The actual binding force is complex and involves residual strong interactions mediated by mesons, but it effectively counteracts electrostatic repulsion, stabilizing the nucleus.

c. Conclusion on Force Strength

The electromagnetic repulsive force (~16 N) is significant but is overcome by the residual strong nuclear force, which is much stronger at sub-femtometer distances. The strong force’s strength—on the order of hundreds of newtons when considering more detailed nuclear models—ensures nuclear stability. Thus, the nuclear binding involves a delicate balance between electromagnetic repulsion and the strong nuclear attraction, with the latter dominating at very short ranges to keep the nucleus intact.

References

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  • Heisenberg, W. (1927). Über den anschaulichen Inhalt der quantentheoretischen Kinematik und Mechanik. Zeitschrift für Physik, 43, 172-198.
  • Griffiths, D. J. (2018). Introduction to Quantum Mechanics. Cambridge University Press.
  • Feynman, R., Leighton, R., & Sands, M. (1963). The Feynman Lectures on Physics. Addison-Wesley.
  • Thorne, K. S. (1994). Black Holes and Time Warps: Einstein's Outrageous Legacy. W. W. Norton & Company.
  • Rutherford, E. (1911). The Scattering of α and β Particles by Matter and the The Structure of the Atom. Philosophical Magazine, 21, 669-688.
  • Schwinger, J. (1962). Quantum Electrodynamics. Physical Review, 125, 397-406.
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