Sunday, October 31, 2010

Dulong–Petit law











The Dulong–Petit law, a chemical law proposed in 1819 by French physicists and chemists Pierre Louis Dulong and Alexis Thérèse Petit, states the classical expression for the specific heat capacity of a crystal. Experimentally the two scientists had found that the heat capacity per weight (the mass-specific heat capacity) for a number of substances was close to a constant value, after it had been multiplied by the presumed weights of the atoms of the substance. These atomic weights had recently been suggested by Dalton.
The modern theory of the heat capacity of solids states that it is due to lattice vibrations in the solid, and was first derived in crude form from this assumption by Albert Einstein, in 1907. The Einstein solid model thus gave for the first time a reason why the Dulong-Petit law should be stated in terms of the classical heat capacities for gases.

Equivalent forms of statement of the law

An equivalent statement of the Dulong-Petit law in modern terms is that, regardless of the nature of the substance or crystal, the specific heat capacity (measured in joule per kelvin per kilogram) is equal to 3R/M, where R is the gas constant (measured in joule per kelvin per mole) and M is the molar mass (measured in gram per mole).
Dulong and Petit did not state their law in terms of the gas constant R (which was not then known). Instead, they measured the values of heat capacities (per weight) of substances and found them smaller for substances of greater "atomic weight" as inferred by Dalton. Dulong and Petit then found that when multiplied by these atomic weights, the value for the heat capacity (which would now be the heat capacity PER MOLE in modern terms) was nearly constant, and equal to a value which was later recognized to be 3 R.
In other modern terminology, the dimensionless heat capacity is equal to 3.

Application limits

Despite its simplicity, Dulong–Petit law offers fairly good prediction for the specific heat capacity of solids with relatively simple crystal structure at high temperatures. It fails, however, at room temperatures for light atoms bonded strongly to each other, such as in metallic beryllium, and in carbon as diamond. In the very low (cryogenic) temperature region, where the quantum mechanical nature of energy storage in all solids manifests itself with larger and larger effect, the law fails for all substances. For crystals under such conditions, the Debye model, an extension of the Einstein theory that accounts for statistical distributions in atomic vibration when there are lower amounts of energy to distribute, works well.

Derivation

A system of vibrations in a crystalline solid lattice can be modelled by considering harmonic oscillator potentials along each degree of freedom. Then, the free energy of the system can be written as
F=N\varepsilon_0+k_BT\sum_\alpha \log\left(1-e^{-\hbar\omega_{\alpha}/k_BT}\right)
where the index α sums over all the degrees of freedom. In the 1907 Einstein model (as opposed to the later Debye model) we consider only the high-energy limit:
k_BT\gg\hbar\omega_\alpha. \,
Then
1-e^{-\hbar\omega_\alpha/k_BT} \approx \hbar\omega_\alpha/k_BT. \,
and we have
F=N\varepsilon_0+k_BT\sum_{\alpha}\log\left(\frac{\hbar\omega_{\alpha}}{k_BT}\right)
Define geometric mean frequency by
\log\bar{\omega}=\frac{1}{M}\sum_\alpha \log\omega_\alpha,
where M measures the total number of degrees of freedom of the system.
Thus we have
F=N\varepsilon_0-Mk_BT\log k_BT+Mk_BT\log\hbar\bar{\omega} \,
Using energy
E=F-k_BT\frac{\partial F}{\partial T},
we have
E=N\varepsilon_0+Mk_BT. \,
This gives specific heat
C=\frac{\partial E}{\partial T}=Mk_B,
which is independent of the temperature.

Saturday, October 30, 2010

The hypothetico deductive model or method

The hypothetico-deductive model or method, first so-named by William Whewell,[1][2] is a proposed description of scientific method. According to it, scientific inquiry proceeds by formulating a hypothesis in a form that could conceivably be falsified by a test on observable data. A test that could and does run contrary to predictions of the hypothesis is taken as a falsification of the hypothesis. A test that could but does not run contrary to the hypothesis corroborates the theory. It is then proposed to compare the explanatory value of competing hypotheses by testing how stringently they are corroborated by their predictions.

Saturday, August 21, 2010

Vector Video Tutorial



Vector Algebra




Vector Algebra

A scalar is a value that can be represented by a single number.
A vector is also quantity that has both magnitude (size) and direction. Vectors are often written in bold type, to distinguish them from scalars. Velocity of a moving point is an example of a vector quantity.In two dimensional space a vector may be represented by two scalar components, in three dimensions a vector may be represented by three scalar components. Most simply these are Cartesian coordinates.  However in 2D vectors can be written in polar coordinates and in 3D they can be written in spherical or cylindrical coordinates.

Elementary Vector Algebra Vector Arithmetic Notes
Vectors follow obvious rules of addition and subtraction. Also the multiplication of a vector by a scalar is straightforward. For example if a = (a1,a2,a3),b = (b1,b2,b3) are vectors and a is a scalar then


a + b = (a1,a2,a3)+(b1,b2,b3) = (a1+b1,a2+b2,a3+b3)


a - b = (a1,a2,a3)-(b1,b2,b3) = (a1-b1,a2-b2,a3-b3)


aa = (aa1,aa2,aa3)
Dot Product
The dot product of two vectors a and b is defined as follows:



a . b = (a1,a2,a3).(b1,b2,b3) = a1 b1+ a2 b2+ a3 b3
Cross Product
The cross product of two vectors a and b is defined as follows:

a ×b = (a1,a2,a3) ×(b1,b2,b3) = (a2 b3 - a3 b2, a3 b1 - a1 b3, a1 b2 -a2 b1)

Wednesday, August 18, 2010

The Gradient

The gradient is a vector operation which operates on a scalar function to produce a vector whose magnitude is the maximum rate of change of the function at the point of the gradient and which is pointed in the direction of that maximum rate of change. In rectangular coordinates the gradient of function f(x,y,z) is:

If S is a surface of constant value for the function f(x,y,z) then the gradient on the surface defines a vector which is normal to the surface.
http://hyperphysics.phy-astr.gsu.edu/hbase/gradi.html

Monday, August 16, 2010

Scientific Revolution

701- Jethro Tull invents the seed drill.

1709- Bartolomeo Cristofori invents the piano.

1711- Englishmen, John Shore invents the tuning fork.

1712- Thomas Newcomen patents the atmospheric steam engine.

1717- Edmond Halley invents the diving bell.

1722- French C. Hopffer patents the fire extinguisher.

1724- Gabriel Fahrenheit invents the first mercury thermometer.

1733- John Kay invents the flying shuttle.

1745- E.G. von Kleist invents the leyden jar, the first electrical capacitor.

The Scientific Revolution

The "Scientific Revolution" is a period of about 150 years during which the classical world view presented in the works of Aristotle, Ptolemy, and Galen was replaced by the fundamental ideas of modern science. Historians generally date it from the publication of Copernicus' De revolutionibusin 1543 to that of Newton's Principiain 1687. The most important new ideas developed during this time were:
- the mechanical philosophy
- the corpuscular philosophy, including atomism
- the experimental philosophy

Important persons:

Nicolaus Copernicus (1473-1543) Poland, astronomy
William Gilbert (1540-1603) England, magnetism
Tycho Brahe (1546-1601) Denmark, astronomy
Francis Bacon (1561-1627) England, method
Galileo Galilei (1564-1642) Italy, astronomy, mechanics
Johann Kepler (1571-1630) Germany, astronomy, optics
Pierre Gassendi (1592-1655) England, atomism
Rene Descartes (1596-1650) France, all fields
Robert Hooke (1635-1703) England, microscopy
Isaac Newton (1642-1727) England, physics, mathematics

Important events and publications:

1543 Copernicus, On the Revolution of the Heavenly Spheres
1572 Tycho Brahe observes a new star (nova)
1573 Brahe, On the new star
1577 Tycho Brahe measures the parallax of a comet
1580 Tycho Brahe begins construction of his observatory on Hven
1588 Brahe, On recent phenomena of the aetherial world
1596 Kepler, Mysterium cosmographicum
1600 Gilbert, On the magnet
1602 Brahe, Introduction to the New Astronomy
1605 Bacon, The Advancement of Learning
1609 Kepler, The New Astronomy
1610 Galileo, The Starry Messenger
1613 Galileo, Letters on Sunspots
1616 Copernicus' book is put on the Index of Prohibited Books
1619 Kepler, On the Harmony of the World
1620 Bacon, New Organon
1627 Bacon, New Atlantis
1632 Galileo, Dialogue concerning the Two Chief World Systems
1637 Descartes, Discourse on Method, Geometry, Optics
1638 Galileo, Discourse on Two New Sciences
1642 Descartes, Principles of Philosophy
1649 Gassendi, Synthesis of the Epicurean Philosophy
1660 Royal Society founded in London
1661 Robert Boyle, The Sceptical Chymist
1666 Academy of Sciences founded in Paris
1665-6 Newton's annus mirabilis
1687 Newton, Mathematical Principles of Natural Philosophy