A level, I/GCSE, & Functional Skills Tutoring
in Physics & Maths

One-to-one tuition on-line from
Michael A Smith
MInstP BSc(Hons) NatSciPhys & Math
son of David M Smith

A tutor with nineteen years of experience & dedication with extensive knowledge of both physics & maths
at A level, IGCSE, GCSE, & Functional Skills Maths

Introductory session: free & without obligation

Bookings now being taken for June 2023 onwards

Contact Michael on
0 75 84 47 60 13
or via mike.smith@physics.org


Michael A Smith

"Michael is currently tutoring my daughter for her GCSE exams in Physics and Maths and has been doing so for the last two years. We value Michael hugely, not just for his knowledge and teaching skills but also for the fact that he goes the extra mile and I am sure would never give up on a pupil. We also find Michael flexible and good humoured. He explains everything fully when choices need to be made concerning such things as when to take a particular exam, pro;'s and con's of things, informed detailing of the set-up and what to expect, how to structure answers and he keeps me in the loop adequately. We feel very lucky to have him and my daughter's self-esteem and confidence has increased steadily throughout the time he has taught her."

"Michael worked with my son for over a year mostly on A level physics but also some A level maths. He was incredibly patient and kind and helped get our son to a place where he went into his exams feeling much more confident. I would highly recommend using Michael."

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Types of Homework

There are seven types of homework. These are practice, preparation, extension, integration, research, application, & flipped homework.
Each type of homework has its own role for students learning. The important task for teachers is to select homework that will best provide holistic support to a student.

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emf & pd

In any circuit there are components that put energy into the circuit, they provide an electro-motive force (emf), & components that take energy out, they have a potential difference (pd) across them. Both emf & pd are measure in volts, V.

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12 Female Physicists

Marie Curie
only person to have Nobel Prizes in multiple sciences;
Lise Meitner
the 1st woman to be appointed Professor of Physics in Germany;
Maria Goeppert Mayer
proposed the nuclear shell model;
Ruby Payne-Scott
discovered several types of radiation bursts originating from the sun;
Rosalind Franklin
her expertise was instrumental in producing the 1st X-ray diffraction images of DNA, confirming its double helix structure;
Vera Rubin
conducted pioneering work on galaxy rotation rates, providing evidence for the existence of dark matter;
Dame Jocelyn Bell Burnell
co-discovered the 1st radio pulsars;
Katherine Johnson
her calculations of orbital mechanics made possible the 1st & subsequent manned U.S. spaceflights;
Helen Quinn
developed the theory, which is related to matter-antimatter symmetry & explains a possible source of dark matter;
Margaret Reid
is carrying out pioneering on fundamental tests of quantum theory, applications include teleportation & cryptography;
Amanda Barnard
she became the 1st woman & the 1st person in the Southern Hemisphere to win the Feynman Prize in nanotechnology for her work on diamond nanoparticles;
Michelle Simmons
She has established a large research group dedicated to the fabrication of atomic scale devices, the only group worldwide that can create atomically precise devices in silicon.

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Simple Harmonic Motion

Graphs showing SHM for position, velocity and acceleration

One type of motion that repeats. The more well know circular motion (orbital motion for planets) has links to SHM.

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Rules for Divisibility

Divisible by means when you divide one number by another the result is a whole number. Numbers like 555 are clearly divisible by five, but could you see that 555 is also divisible by three, fifteen, 37, 111, & 185? Methods are given here to identify divisibility by integers up to 12, and beyond if should you wish.

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G and E Fields Compared

Force in a Radial Field

Gravitational Field

F= G⁢m1⁢m2 r2

Always attractive

This is a vector

Electric Field

F= k⁢Q1⁢Q2 r2

Can be attractive or repulsive

This is a vector

The radial field equations isn't the only property that is similar between these fields.

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The Conic Sections Collected

Circle,
Ellipse,
Parabola
&
Hyperbola

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Quadratic Sequences

A quadratic sequence has n2 & no higher powers of n in its nth term (Un). The general form of a quadratic sequence is given by Un =a⁢n2+b⁢n+c where a, b & c are numbers that can be thought of as characterising the quadratic sequence & often are to be found.

An example of a quadratic sequence is 1, 4, 9, 16, 25, ... which happens to be the square numbers. Another is 3, 6, 13, 24, 39, ... which is less easily identified as a particular sequence. To determine if a given sequence is indeed a quadratic sequence the second difference needs to be shown to be constant.

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Set Notation

A set is a collection of objects, elements or members. The objects can be any collection you can think of. This collection can be described by listing the elements, or by giving a rule. The list or rule is given in a pair of curly brackets {}. For example: A={6,9,14} or B = { x: x2+5 |x∈ℕ }

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Physics Equations & Data

Equations are central to understanding physics. Each examination boards issues a list of equations for use in their tests which are either to be memorised or given to the candidate in a booklet.

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SUVAT

The Equations of Constant Acceleration

Let s be the displacement, u be the initial velocity, v be the final velocity, a be the constant acceleration, & t be the time taken, then ...

v=u+a⁢t
s =v⁢t -½⁢a⁢t2
s =u⁢t +½⁢a⁢t2
s =u+v2⁢t
v2 =u2 +2as

Further details can be found at Wikipedia: Equations of motion - Uniform acceleration

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Useful Physics Websites

A list of websites grouped according to qualifications that students may find useful in revision & preparation for exams.

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All measurements we make have a level of uncertainty

the Limitation of Physical Measurements

But how do we combine uncertainties?

● Adding / subtracting - ADD ABSOLUTE UNCERTAINTIES
e.g. A ruler with an uncertainty of 0.5⁢mm shows a spring extends from 50.0⁢mm to 63.5⁢mm, so the extension is 63.5-50.5=13.5 with an uncertainty of 0.5+0.5=1. The calculated extension is (13.5±1)⁢mm

● Multiplying / dividing - ADD RELATIVE UNCERTAINTIES
e.g. a force of (45±5)⁢N is applied to a mass of (9±3)⁢kg, what is the acceleration? Using Newton's 2nd Law, the acceleration is given by a=Fm, so a=459=5⁢m⁢s-2 with a certainty given by 545+39=49. The calculated acceleration is 5⁢m⁢s-2±49 or (5±2)⁢m⁢s-2

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Recommended Calculators

A list of calculators that are useful for I/GCSE & A Level Maths or physics

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Moments

In physics, a moment is an expression involving the product of a distance & physical quantity, & in this way it accounts for how the physical quantity is located or arranged.
Moments are usually defined with respect to a fixed reference point; they deal with physical quantities located at some distance relative to that reference point. For example, the moment of force, often called torque, is the product of a force on an object & the distance from the reference point to the object. In principle, any physical quantity can be multiplied by a distance to produce a moment. Commonly used quantities include forces, masses, & electric charge distributions. [scraped from en.wikipedia.org/wiki/Moment_(physics)]

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Photoelectric Effect

The Photoelectric effect provides evidence that electromagnetic waves have particle-like behaviour. In the photoelectric effect, electrons are emitted from a metal’s surface when it absorbs electromagnetic radiation.

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Fraction, Decimals & Percents

You're unlikely to be asked to convert between one seventh & the decimal equivalent of 0.1428571428571 ...
These are, however, the same number, but in different presentations.
See more at mathsisfun.com

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Evolution of Large Mass Stars

The evolution of stars with a mass higher than about 1.4MSun is different from that of smaller mass stars. Stars between 1.4MSun & 3MSun also evolve into red giants, but they end their life as supernovae, leaving behind a neutron star. Stars with a main-sequence mass of more than 3MSun evolve into red supergiants, & when these explode as supernovae they leave behind a black hole.

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