Solving polynomial equations, descartes theorem

A large part of the algebra courses at upper secondary-school level are devoted to solving equations or factorization of polynomials. This is often the same thing.

Some terminology. All of these are the same:
Solving a polynomial equation.
Finding roots of a polynomial equation p(x)=0.
Finding zeros of a polynomial equation p(x)
Factorizing a polynomial function p(x).

There is a factor for every root and vice versa.
(x-r) is a factor if and only if r is a root according to the Factor theorem.

How to solve equations step-by-step:
1. If solving an equation, put it in standard form with 0 on one side and simplif.
2. Know hoewmany roots to expect.
3. Find one factor or root. (Several techniques available)
4. Divide by your factor. This leaves you with a new reduced polynomial. whose degree is 1 less. For the rest of the problem you’ll work with the reduced polynomial and not the original.
5. Now you have a quadratic or linear equation which you already know how to solve.
Write down the solution.

There is no general solution for solving equations of degree 5 and higher.
Try to factorize the polynomial as much as possible.
Equations of degree four or less can be solved by stanard methods.

A plynomial of degree n will have n roots some of which may be multiple roots. This is according to the Fundamental theorem of Algebra.

Descartes Rule of Sign:
Tells you the how many positiv or negative real zeroes the polynomial has.
1. The number of positive roots of p(x)=0 is either equal to the number of variations in sign of p*(x) or less than that by an even numer.
2. The number of negative roots of p(x) = 0 is either equal to the number of variations in sign of p(-x)=0 or less than that by an even number.

Complex Roots

If a polynomial has real coefficients, then either all roots are real or there are an even number of non-real complex roots, in conjugate pairs.

For example, if 5+2i is a zero of a polynomial with real coefficients, then 5−2i must also be a zero of that polynomial. It is equally true that if (x−5−2i) is a factor then (x−5+2i) is also a factor.

This is true because when you have a factor with an imaginary part and multiply it by its complex conjugate you get a real result:

(x−5−2i)(x−5+2i) = x²−10x+25−4i² = x²−10x+29

If (x−5−2i) was a factor but (x−5+2i) was not, then the polynomial would end up with imaginaries in its coefficients, no matter what the other factors might be. If the polynomial has only real coefficients, then any complex roots must occur in conjugate pairs.

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The area of the circle

‘Minute Physics’ derives the area of the circle with a string of pearls and a ruler:

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Modular arithmetic & the Chinese Rest Theorem

modular arithmetic (sometimes called clock arithmetic) is a system of arithmetic for integers, where numbers ”wrap around” upon reaching a certain value—the modulus.

An example of this is the clock which starts repeating itself when it has reached 12. Therefore it is said that the clock follows an arithmetic modulo 12.  

Ex: If you add 7 hours to 8 o’clock the result is not 15 since when thee clock reaches zero it starts over from zero once again so the result is 7+8=3 in this arithmetic.

For a positive integer n, two integers a and b are said to be congruent modulo n,
a=b mod(n)
if the the remainder is the same when a and b are divided by n.

if their difference a − b is an integer multiple of n. The number n is called the modulus of the congruence.

a \equiv b \pmod n,\, 
e.g. 14

14≡12 (mod 2)

An example of an application of this mathematical tool is the Chinese Remainder Theorem.

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Exceldiagrams

Excel is a versatile programme for e.g. statisitics.

Learn more!

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Asteroid-passage

In the evening today February the 15th. an asteroid flies by close to the Earth only about 27 600 km away. It measures about 40 m in length and is similar to the one responsible for the Tunguska (Siberia) impact in  1908. It deforestated everything within 30 km.

NASA provides more information.

Yesterday meteorites impacted Russia in the Tjeljabinsk-region injuring 200 people.

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Conical sections

280px-Conic_section_-_clean

The force of gravity determines the trajectories of the celestial bodies. Mathematical analysis reveals that there are three types of trajectories possible for a body moving in a gravitational field determined by Newton’s law of gravity.

  • If one of the bodies has very high speed relative to the other the moving body traces out a hyperbola. The equation for this is
    x 2/a2 – y 2/b=1
  • If the speeds of the bodies are beelow a certain threshold value they move in an elliptical curve. x 2/a2 + y 2/b2 =1
  • The limiting case between the hyperbola and the ellipse is the parabola. y=ax

Those geometrical objects can be illustrated by slicing the cone according to the figure above.

Publicerat i Geometri, Gymnasiematematik(high school math), matematik 2c | Märkt , , , | Lämna en kommentar

Thermodynamics 2 Entropy

M106-HST-Lgendler

A collection of rembrandts self-portraits serve as an illustration of the passage of time

When left to itself snow spontaneously would never build a snowman.
It will only form different kinds of heaps . This can be undestood as the consequence of statistics: There are more possible arrangements of  the atoms constituting the snow leading to unordered heaps than arrangements resulting in the much more ordered state of a snowman,.

This cicumstance can be described with the concept of statistical weight.

The statistical weight (is the number of microscopic states(ways of arranging the atoms) %omega;corresponding to a certain macroscopic state(the large scale object).
The entropy, S, is defined as
S = k ln Ω
It is a measure of the disorder of the system. In all spontaneous processes the entropy increases because statistically the state with the greatest statistical Weight is more probable.
Such a process is irreversible.

In an adiabatic process no Heath is exchanged with The surroundings.

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Thermodynamics 1


Världens största ånglok, Big Boy, är exempel på en värmemaskin vars effektivitet beror på temperaturskillnaden mellan vattenångan och den omgivande luften.
A spacecraft enters  the atmosphere with a velocity of appr. 40 000 km

The temperature is a measure of the heat content of a body.
Heat or thermal energy is a form of energy that moves from hotter to cooler bodies.

The average kinetic energy of a molecule with an absolute temperature T is given by

E = 3kT/2.

Since temperature is a measure of heat heat is a measure of the kinetic energy of the constituents of the medium of a certain temperature.

If the temperature increases the movements of the individual atoms also gets more violent until the chemical bondings are broken up and the atoms become free.

This is how an element changes from solid to liquid to gaseous form.

Those are the three states of aggregation of matter. In stars a fourth state is possible: the plasma state.

Atoms and molecules never rest (this is the third law of thermodynamics) and when they bounce together electrons in the atoms are excited and within nanoseconds they deexcite by emission of low-energetic electromagnetic radiation so-called Infra-red radiation or heat-radiation.

According to Heisenberg’s uncertainty-principle it’s impossible for an atom to be at rest because this would imply that we have exact knowledge about the speed of the atom. The Heisenberg uncertainty principle δp˙δx>h
then postulates that the uncertainty in the position of the atom must be infinite.

This radiation from e.g. the Sun is perceived as heat and it drives the atoms of the skin into  oscillations whereby the temperature in the skin is increased.

All materials having a temperature in excess of absolute zero emits heatradiation.  This process occurs until the temperature of the body and its surroundings are equal.

Then the body emits and absorbs the same amount of heat energy and an equilibrium has been established.

The first postulate of thermodynamics states that the energy of an isolated system is constant. Energy can not be created or destroyed only transformed between different forms.

kinetic energy

potential energy

nuclear energy

radiation energy

Värmekapaciteten. Kan uttryckas med hjälp av frihetsgraderna med hjälp av ekvipartitionsprincipen. Den anger hur mycket energi som krävs för att öka temperaturen 1C. För ett kg av ämnet.

C=0,5(ntr + nrot + nvib2)R.

Van der Waals gaslag
(P+a/v)(V-b)=kT.

a/V anger växelverkan mellan gasmolekylerna medan b är ett mått på den volym gasmolekylerna upptar.

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Science RSS-feed

For your service and convenience; I have added an RSS-feed from Daily Telegraph as a widget in  the meny list to the right. Just click on  the link and the latest Science and Tech-News will flow into your computer.

Today I read that the ten most important British inventions are:

  1. The reflector telescope (Newton) England
  2. The www (Tim Berners-Lee) England
  3. Penicillin(Fleming) Scotland
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Merry Christmas & Happy New Year

bildbildbild

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