Notes, summaries, assignments, exams, and exercises for Physics for University

Understanding Semantic Roles: Agent, Experiencer, and More

Physics3.23 KB

Understanding Semantic Roles

Unit 6

Agent: The initiator/doer of the action (‘David cooked the chicken’)
Experiencer: The entity that feels or perceives something (‘David saw the dog’)
Patient: The entity undergoing the effect of some action and some change of state (‘David cooked the chicken’) - Sometimes used interchangeably with theme.
Theme: The entity which is moved by an action (‘Fred threw the rock’), whose location is described (‘The book is in the library’), or is experienced or perceived (‘David saw the dog’) - Sometimes used interchangeably with patient.
Beneficiary: The entity for whose benefit an event took place / the entity which is intended to possess the theme but may actually not do so. (‘Jones made a new
...
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Experimental Determination of Refractive Index Using Light and Microwaves

Physics4.87 KB

Study of Reflection and Refraction of Electromagnetic Waves

Objectives

  • Measure the refractive index of a prism for electromagnetic waves in the visible range (light) and for microwaves.
  • Measure the angle of reflection of electromagnetic waves.
  • Determine the critical angle when a ray of light passes from a medium of higher refractive index to one of lower refractive index, leading to total internal reflection.

Theoretical Background and Planning

Refraction occurs when a wave changes its propagation speed upon passing from one medium to another. This phenomenon changes the direction of the ray when it is incident obliquely to the interface between two media with different refractive indices.

This relationship is governed by Snell's Law:

n1 sin θi =...

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Fundamental Physics Laws: Momentum, Energy, and Motion

Physics2.29 KB

Angular Momentum Conservation

The law of conservation of angular momentum states that when no external torque acts on an object, its angular momentum remains constant.

Inverse Square Law

The inverse-square law dictates that a physical quantity's intensity is inversely proportional to the square of the distance from its source.

Energy Conservation

The law of conservation of energy states that energy cannot be created or destroyed, only transformed or transferred.

Momentum Conservation

In an isolated system, the total momentum of two objects before a collision equals their total momentum after the collision.

Energy Degradation

The first law of thermodynamics asserts that the universe's total energy is constant. The second law states that this energy's...

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Geophysical Principles: Elasticity, Magnetism, and Radiometric Dating Formulas

Physics4.66 KB

Fundamental Concepts in Earth Physics

Elastic Moduli and Seismic Waves

Elastic Moduli Definitions

  • Young's Modulus (Y): Describes the fractional change in length of an object when subjected to a tensile stress. The formula is: Y = (F/A) / (ΔL/L₀)
  • Bulk Modulus (K): Describes how a fractional change in volume depends on the applied pressure.
  • Shear Modulus (G): Describes how an angle of shear depends upon a tangential stress.

Seismic Wave Types

  • P-wave (Primary Wave): Characterized by compressional and expansion motion.
  • S-wave (Secondary Wave): Characterized by shear motion.

Demonstration of Radiometric Age Dating

Derivation of the Decay Equation

If the decay rate is equal to $\lambda$, the probability that a given nucleus will decay in a time interval...

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Cosmochemistry: Unveiling the Universe's Origin and Evolution

Physics2.85 KB

In the Beginning

Certain questions about our existence on Earth are so fundamental that they have been incorporated into religious mythologies. These questions not only concern the origin of the Earth and the evolution of life but also extend to the origin of the universe and to the nature of space and time. Did the universe have a beginning, and will it ever end? What existed before the universe formed? Does the universe have limits, and what exists beyond those limits? It is proper to raise these questions at the beginning of a geochemistry course because they are within the scope of cosmochemistry.

The Big Bang

The universe started like a bubble in a stream. At first, it was not there, and suddenly it formed and expanded rapidly as though it...

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Diffraction Grating Experiment: Calculating Wavelengths

Physics3.62 KB

Diffraction Grating Experiment

Subject:

Calculate the d-spacing (d) of diffraction grating and determine wavelengths of different light sources.

Planning:

A diffraction grating is an optical component that separates light into its constituent wavelengths. There are two main types of diffraction gratings: reflection gratings and transmission gratings. A diffraction grating consists of a surface with a series of closely spaced parallel lines or slits. These can be etched onto a flat metal surface (reflection grating) or a glass plate (transmission grating). When monochromatic light (light of a single wavelength) is incident on a diffraction grating, the emerging waves interfere constructively at specific angles, resulting in a pattern of constructive...

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Diffraction Grating Analysis and Laser Wavelength Measurement

Physics3.24 KB

Study of Diffraction Phenomena and Light Wavelengths

Objectives

  • To determine the emission wavelength of a laser using a diffraction grating with an electromagnetic wave.
  • To determine the wavelength of each color of white light using a diffraction grating.
  • To determine the emission wavelength of the laser based on the phenomenon of diffraction of an electromagnetic wave.

Planning

The diffraction grating is a device that separates light into its components. Two types exist: reflection gratings and transmission gratings. A transmission diffraction grating is built by parallel lines equally spaced on the flat surface of a glass plate, while a reflection grating uses a metal surface. These slots scatter light; the spaces between the grooves behave like...

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Properties of Laser Light: Monochromaticity, Coherence, and More

Physics1.95 KB

Properties of Laser Light

1. Monochromaticity

Unlike discharge lamps that emit on all atomic transitions, laser emission typically corresponds to a single atomic transition of the gain medium. The spectral line width can be much smaller than the atomic transition's due to the influence of the optical cavity.

2. Coherence

Laser beams exhibit high spatial and temporal coherence.

Spatial coherence describes the regularity of the optical phase across a beam's cross-section.

Temporal coherence refers to the duration over which the beam's phase remains well-defined. The temporal coherence time (tc) is generally the reciprocal of the spectral linewidth (ν). Consequently, the coherence length (lc) is: lc = ctc = c/ν.

3. Directionality

A key characteristic...

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Cosmology Fundamentals: The Big Bang, Hubble's Law, and the Universe's Fate

Physics3.36 KB

What is Cosmology?

Cosmology Defined

Cosmology is the study of the origin, present structure, evolution, and density of the universe.

The Cosmological Principle

The cosmological principle is the basic assumption that physical laws are true everywhere in the universe, not just on Earth.

The Expanding Universe

Galactic Recession

We observe galaxy clusters receding from us, which implies that the universe is expanding. Galaxies farthest from us are moving away the fastest; the farther the distance, the faster the speed.

Hubble's Law

Hubble's Law states that a galaxy’s velocity of recession (v) is directly proportional to its distance from us (d). The formula is v = Hd.

The Hubble Constant

The Hubble constant (H) is a crucial value that gives the rate at...

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Cylindrical Heat Transfer & Exchanger Principles

Physics42.53 KB

Heat Conduction Through a Single-Layer Cylinder


wJ8GGTzzNKds8ZsHJnHapD8jcgj4sMKw1o4VgFiG

From this equation, the following is derived:

0FsfbzOOoqa164o7n7Enm3kUECY6YJXTPiVvQ8ln

Boundary Conditions

  • t(r = r1) = t1
  • t(r = r2) = t2

We are looking for a function t = f(r). The resulting equation is t = B * ln(r) + C.

BXDwhoFtLpH + AAAAAElFTkSuQmCC

== LkXLYLD2ZIdZOUwAAOw


t1 = B * ln(r1) + C

t2 = B * ln(r2) + C

CSYyYmaGbmaOiQwG0yPDFQi5qWcVdfOFRb0NiLLI

Where Ar represents the average area.

The values for t, where t = B * ln(r) + C, are shown below:

Dqq8DQdhAOAAoKyIYJzIo7JIdiEnStBW1 + pJCBjk

3Lq7bNmzjtAtLjO4gstYMJF5ojfOdtonidQDIunL


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To refer to the inner area, the expression is divided and multiplied by r1:

== ZqErACtosKEQQQAAOw

To refer to the outer area, the expression is divided and multiplied by r2:

yMWgwodSrSoUYs9l336CasYjAcmRAqxFi3nTJZ9P

Cylinder Heat Transfer Coefficient: Fouling & Clean

The standard heat transfer rate varies during operation due to fouling of the exchanger walls.

The coefficient is at its minimum when fully fouled and at its maximum (clean) at the beginning...

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