ข้ามไปยังเนื้อหา

AQA A-Level Physics

A-Level · AQAPhysics58 โน้ต ใน 13 โฟลเดอร์, 358 KB

โน้ตทบทวน 58 รายการ สร้างโดย cookie แบ่งเป็น 13 ส่วนตามหัวข้อของหลักสูตร

Notes for AQA A-Level Physics (7408), in a folder for each of the specification's content sections in its order, with one note for each sub-topic or group of sub-topics and the required practicals in the topics they belong to. The five optional sections (astrophysics, medical physics, engineering physics, turning points in physics, electronics) each have their own folder. Delete the options and the folders your course leaves out.

เมื่อเพิ่มแล้ว สำเนาจะอยู่ในโน้ตของคุณ ในโฟลเดอร์ใหม่พร้อมโฟลเดอร์ย่อยด้านล่าง เพื่อให้คุณแก้ไขและเปลี่ยนเป็นแฟลชการ์ดหรือชุดคำถามได้ การดาวน์โหลดจะได้ไฟล์ Markdown ในรูปแบบ zip ซึ่งเปิดได้ในแอปจดโน้ตทุกแอป

มีอะไรอยู่ข้างใน

  • Measurements and their errors
    • Units, errors and estimation9 KB
  • Particles and radiation
    • The atom, isotopes and unstable nuclei5 KB
    • Antiparticles, photons and interactions7 KB
    • Hadrons, leptons and quarks7 KB
    • The photoelectric effect6 KB
    • Electrons in atoms and wave-particle duality7 KB
  • Waves
    • Progressive waves and polarisation6 KB
    • Stationary waves7 KB
    • Interference and diffraction8 KB
    • Refraction and optical fibres6 KB
  • Mechanics and materials
    • Vectors, moments and equilibrium6 KB
    • Motion in a straight line and projectiles7 KB
    • Newton's laws and momentum6 KB
    • Work, energy and power5 KB
    • Bulk properties of solids and the Young modulus7 KB
  • Electricity
    • Charge, current, resistance and I-V characteristics4 KB
    • Resistivity, thermistors and superconductivity5 KB
    • Circuits and potential dividers6 KB
    • EMF and internal resistance4 KB
  • Further mechanics and thermal physics
    • Circular motion5 KB
    • Simple harmonic motion6 KB
    • Simple harmonic systems, damping and resonance7 KB
    • Thermal energy transfer5 KB
    • Ideal gases and kinetic theory8 KB
  • Fields and their consequences
    • Gravitational fields and potential5 KB
    • Orbits of planets and satellites5 KB
    • Electric fields and potential6 KB
    • Capacitors5 KB
    • Charging and discharging a capacitor5 KB
    • Magnetic fields and forces6 KB
    • Electromagnetic induction6 KB
    • Alternating currents and transformers6 KB
  • Nuclear physics
    • Rutherford scattering and the radiations7 KB
    • Radioactive decay6 KB
    • Nuclear instability and nuclear radius6 KB
    • Mass, energy and binding energy5 KB
    • Induced fission and nuclear power6 KB
  • Astrophysics
    • Telescopes7 KB
    • Classifying stars7 KB
    • The life and death of stars7 KB
    • Cosmology and exoplanets7 KB
  • Medical physics
    • The eye and vision6 KB
    • The ear and hearing6 KB
    • ECG, ultrasound, fibre optics and MR8 KB
    • X-ray imaging7 KB
    • Radionuclide imaging and therapy8 KB
  • Engineering physics
    • Rotational dynamics6 KB
    • The first law of thermodynamics and p-V diagrams6 KB
    • Engines, the second law and heat pumps7 KB
  • Turning points in physics
    • The electron6 KB
    • The nature of light7 KB
    • Wave-particle duality and electron microscopes5 KB
    • Special relativity7 KB
  • Electronics
    • Discrete semiconductor devices6 KB
    • Analogue and digital signals and LC filters6 KB
    • Operational amplifiers6 KB
    • Digital logic and astables5 KB
    • Communication systems7 KB

โน้ตรายการแรก

Measurements and their errors / Units, errors and estimation

SI units

Every physical quantity is a number multiplied by a unit, and the whole of physics is built on a small set of base units from which every other unit is derived. The base quantities you need are mass (kilogram, kg), length (metre, m), time (second, s), amount of substance (mole, mol), temperature (kelvin, K) and electric current (ampere, A).

A derived unit is a combination of base units. The newton is the force that gives a mass of 1 kg an acceleration of 1 m s−21\,\mathrm{m\,s^{-2}}, so 1 N=1 kg m s−21\,\mathrm{N} = 1\,\mathrm{kg\,m\,s^{-2}}. The joule is a newton metre, 1 J=1 kg m2 s−21\,\mathrm{J} = 1\,\mathrm{kg\,m^2\,s^{-2}}, and the watt is a joule per second, 1 W=1 kg m2 s−31\,\mathrm{W} = 1\,\mathrm{kg\,m^2\,s^{-3}}. Writing an equation's units in base units is a quick check that the equation can be right: both sides must reduce to the same combination.

Prefixes and standard form

Prefixes scale a unit by a power of ten, so that very large and very small values can be written without long strings of zeros.

PrefixSymbolFactor
teraT101210^{12}
gigaG10910^{9}
megaM10610^{6}
kilok10310^{3}
centic10−210^{-2}
millim10−310^{-3}
microμ\mu10−610^{-6}
nanon10−910^{-9}
picop10−1210^{-12}
femtof10−1510^{-15}

Standard form writes a number as a×10na \times 10^n with 1≤a<101 \le a < 10, so 0.000 047 m0.000\,047\,\mathrm{m} is 4.7×10−5 m4.7\times10^{-5}\,\mathrm{m} or 47 μm47\,\mu\mathrm{m}.

Converting between units

Some units of the same quantity are not related by a simple power of ten, and you convert using their definitions. The electronvolt is the energy gained by an electron accelerated through a potential difference of 1 V, so 1 eV=1.60×10−19 J1\,\mathrm{eV} = 1.60\times10^{-19}\,\mathrm{J}. The kilowatt hour is the energy transferred by a 1 kW device in one hour, so 1 kW h=1000 W×3600 s=3.6×106 J1\,\mathrm{kW\,h} = 1000\,\mathrm{W}\times3600\,\mathrm{s} = 3.6\times10^{6}\,\mathrm{J}.

Random and systematic errors

An error is the difference between a measured value and the true value. Two different kinds behave differently, and the remedy for each is different too.

A random error makes repeated readings scatter unpredictably either side of the true value. It comes from things such as reaction time, small fluctuations in the reading or the difficulty of judging a scale. Taking many readings and averaging them reduces its effect, and a graph drawn through many points averages it out.

A systematic error shifts every reading by the same amount or the same proportion in one direction. A zero error on a micrometer, a stopwatch that runs slow or a meter that is wrongly calibrated all do this. Repeating the measurement does nothing to it. It is reduced by calibrating the instrument against a known standard, checking the zero, or changing the method. On a graph a systematic error shows as a non-zero intercept where the line should pass through the origin.

Vocabulary of measurement
TermMeaning
Precisionhow closely repeated readings agree with each other; small scatter means high precision
Accuracyhow close a reading is to the true value
Repeatabilitythe same person, apparatus and method give the same results over a short time
Reproducibilitydifferent people or different apparatus and methods give the same results
Resolutionthe smallest change in the quantity that the instrument can show

A set of readings can be precise but inaccurate, when a systematic error moves them all to the wrong place, and a set can be centred on the true value but imprecise, when the random scatter is large.

Uncertainty

Every measurement is quoted with an uncertainty, a range within which the true value is expected to lie. The absolute uncertainty has the units of the quantity, the fractional uncertainty is the absolute uncertainty divided by the value, and the percentage uncertainty is the fractional uncertainty multiplied by 100.

percentage uncertainty=Δxx×100% \text{percentage uncertainty} = \frac{\Delta x}{x}\times 100\%

A single reading from a scale is usually given an uncertainty of half the smallest division, or the smallest division if the readings are hard to judge. A digital meter's uncertainty is normally taken as one in the last digit. For repeated readings the uncertainty can be estimated as half the range between the largest and smallest readings (the spread), when the number of readings is small. A reading of a length from a ruler starts at one end and finishes at the other, so if both ends have to be read the uncertainties add.

The number of significant figures in a result should match its uncertainty. Quoting 9.812 345 m s−29.812\,345\,\mathrm{m\,s^{-2}} when the uncertainty is 0.1 m s−20.1\,\mathrm{m\,s^{-2}} claims a precision that the measurements never had, and 9.8±0.1 m s−29.8\pm0.1\,\mathrm{m\,s^{-2}} is the honest statement.

Combining uncertainties
  • When quantities are added or subtracted, add their absolute uncertainties.
  • When quantities are multiplied or divided, add their percentage (or fractional) uncertainties.
  • When a quantity is raised to a power nn, multiply its percentage uncertainty by nn.

Subtracting two nearly equal readings gives a small difference with the full sum of the absolute uncertainties, so its percentage uncertainty can become large. That is why a length found as the difference between two close readings is best measured directly.

Worked example

A cylinder has a mass m=0.250±0.002 kgm = 0.250\pm0.002\,\mathrm{kg}, a diameter d=4.00±0.05 cmd = 4.00\pm0.05\,\mathrm{cm} and a length L=10.0±0.1 cmL = 10.0\pm0.1\,\mathrm{cm}. Find its density with its uncertainty.

The volume is V=π(d/2)2LV = \pi (d/2)^2 L, and the density is ρ=m/V\rho = m/V, so ρ∝m d−2L−1\rho \propto m\,d^{-2}L^{-1}. The percentage uncertainties are

mass:0.0020.250×100=0.8%diameter:0.054.00×100=1.25%, counted twice because it is squared, so 2.5%length:0.110.0×100=1.0% \begin{aligned} \text{mass:}\quad & \tfrac{0.002}{0.250}\times100 = 0.8\% \\ \text{diameter:}\quad & \tfrac{0.05}{4.00}\times100 = 1.25\%, \text{ counted twice because it is squared, so } 2.5\% \\ \text{length:}\quad & \tfrac{0.1}{10.0}\times100 = 1.0\% \end{aligned}

The total is 0.8+2.5+1.0=4.3%0.8 + 2.5 + 1.0 = 4.3\%.

The value of the density, with lengths in metres, is

ρ=0.250π×(0.0200)2×0.100=0.2501.257×10−4=1.99×103 kg m−3 \rho = \frac{0.250}{\pi \times (0.0200)^2 \times 0.100} = \frac{0.250}{1.257\times10^{-4}} = 1.99\times10^{3}\,\mathrm{kg\,m^{-3}}

and 4.3%4.3\% of this is about 0.09×1030.09\times10^{3}, so ρ=(1.99±0.09)×103 kg m−3\rho = (1.99\pm0.09)\times10^{3}\,\mathrm{kg\,m^{-3}}.

Graphs, error bars and gradients

A point on a graph can carry error bars, short lines above and below (and, if needed, to the left and right) showing its uncertainty. The bar length is the absolute uncertainty in that reading. If the uncertainty in one axis is too small to draw it can be left off, and the uncertainty in the other axis is then the one that matters.

A straight-line graph is analysed through its gradient and intercept. The best-fit line is the one that passes through all the error bars with points balanced on either side. To find the uncertainty in the gradient, draw the worst acceptable line, which is the steepest or shallowest line that still passes through all the error bars, and compare its gradient with the best line.

uncertainty in gradient=∣ mbest−mworst ∣ \text{uncertainty in gradient} = \left|\, m_{\text{best}} - m_{\text{worst}} \,\right|

The percentage uncertainty in the gradient is that value as a percentage of the best gradient. The uncertainty in the intercept is found the same way, by comparing the intercept of the best line with that of the worst line. A gradient should be measured with a large triangle, spanning most of the line, because a small triangle magnifies the reading uncertainty.

When a relationship is not linear it can often be made so. If y=axny = ax^n then plotting lg⁡y\lg y against lg⁡x\lg x gives a straight line of gradient nn and intercept lg⁡a\lg a. If y=aekxy = ae^{kx} then plotting ln⁡y\ln y against xx gives gradient kk and intercept ln⁡a\ln a.

Estimation and orders of magnitude

An order of magnitude is the nearest power of ten. Estimating to the nearest order of magnitude is a skill of its own: choose sensible values for the quantities involved, combine them with the physics, and accept an answer that may be out by a factor of a few.

Some useful sizes to hold in mind: a person's mass is about 102 kg10^2\,\mathrm{kg}, a car's about 103 kg10^3\,\mathrm{kg}, a walking speed is about 1 m s−11\,\mathrm{m\,s^{-1}}, an atom's diameter is about 10−10 m10^{-10}\,\mathrm{m} and a nucleus's about 10−15 m10^{-15}\,\mathrm{m}, and the Earth's radius is about 6×106 m6\times10^{6}\,\mathrm{m}.

Worked example

Estimate the gravitational potential energy gained by a person climbing a flight of stairs. Take a mass of 70 kg70\,\mathrm{kg} and a height gain of about 3 m3\,\mathrm{m}.

ΔEp=mgΔh≈70×10×3≈2×103 J \Delta E_p = mg\Delta h \approx 70\times 10\times 3 \approx 2\times10^{3}\,\mathrm{J}

which is of order 103 J10^{3}\,\mathrm{J}. Using g=10 m s−2g = 10\,\mathrm{m\,s^{-2}} instead of 9.819.81 makes a difference of 2%, which is far smaller than the uncertainty in the other estimates and so does not matter here.

และอีก 57 รายการ เมื่อคุณเพิ่มหรือดาวน์โหลด

รีวิว

ยังไม่มีรีวิวที่เขียนไว้ เพิ่มโน้ตเหล่านี้ลงในของคุณ แล้วคุณจะเป็นคนแรกที่เขียนรีวิว