Mostrar mensagens com a etiqueta Guyana. Mostrar todas as mensagens
Mostrar mensagens com a etiqueta Guyana. Mostrar todas as mensagens

Quantum theory


Shortly after Einstein’s paper on the photoelectric effect, Ernest Rutherford’s experiments led to the idea of an atom as a ‘miniature solar system’ in which the electrons orbit around a nucleus. To explain why atoms radiate light at the frequencies observed, Niels Bohr (1885–1962) proposed that the angular momentum of each orbiting electron is an exact multiple of the basic unit h/2pi.
In 1923 Louis de Broglie (1892–1987) suggested that if light waves can behave as particles, then perhaps other particles (such as electrons) can also behave as waves; this was rapidly verified experimentally. In de Broglie’s theory Bohr’s electron orbits are precisely those whose circumference is an integer number of wavelengths.
 Twenty-five years after Planck’s quantum hypothesis, physicists still had no coherent understanding of quantum theory, but in 1925 Erwin Schrödinger (1887–1961) learned of de Broglie’s idea that particles can also behave like waves, and found the appropriate partial differential equation to describe these waves. Earlier, Werner Heisenberg (1901–1976) took an algebraic approach, representing quantities such as the position and momentum of an electron by infinite matrices, and deducing his famous ‘Uncertainty Principle’ that it is theoretically impossible to determine them both at the same time.
In 1928 Paul Dirac (1902–1984) derived an equation for the electron that was consistent with Einstein’s theory of relativity, unlike those of Schrödinger and Heisenberg. This equation explained electron spin and led him to predict the existence of antiparticles, such as the positron which was detected four years later.  
[Austria 1987; Denmark 1985; France 1994; Germany 2001; Guyana 1995; Sweden 1982]

The growth of learning - O crescimento da aprendizagem


The renaissance in mathematical learning during the Middle Ages was largely due to three factors: the translation of Arabic classical texts into Latin during the 12th and 13th centuries, the establishment of the earliest European universities, and the invention of printing. The first of these made the works of Euclid, Archimedes and other Greek writers available to scholars, the second enabled groups of like-minded people to meet and discourse on matters of common interest, and the last enabled scholarly works to be available at modest cost to the general populace.
The first European university was founded in Bologna in 1088, and Paris and Oxford followed shortly after. The curriculum was in two parts. The first part, studied by those aspiring to a Bachelor’s degree, was based on the ancient ‘trivium’ of grammar, rhetoric and logic. The second part, leading to a Master’s degree, was based on the quadrivium, the Greek mathematical arts of arithmetic, geometry, astronomy and music, as shown on the Netherlands Antilles stamps; the works studied would have included Euclid’s Elements and Ptolemy’s Almagest.
[Germany 1957; Guyana 1999; Italy 1988; Netherland Antilles 1966]