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The Modern Nuclear Atom
The Modern Nuclear Atom

... and protons but different numbers of neutrons. • Atomic number = number of protons • Mass number = the sum of the protons and neutrons in an atom’s nucleus ...
Chapter 4-Arrangement of Electrons in Atoms
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Chapter 5 Sec. 2 Bohr`s Model and the Quantum Mechanical Model
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R - University of St Andrews
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... When viewed at high resolution, transitions split. Transitions between any two Bohr energy states involve several spectral lines. This is known as fine structure. Explanation: each energy level actually consists of several distinct states with almost the same energy. The first theory that justified ...
Powerpoint handout
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... Bohr derived a more general formula to predict the observed energies of light: Each electron’s energy is determined by which level it is in. The levels are designated by whole numbers, n. ...
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The Quantum Atom (section 18)
The Quantum Atom (section 18)

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spectral lines

...  This led to the classic model of the atom- similar to the solar system  Distant electrons orbit a massive nucleus due to electrical forces of attraction.  Rutherford’s model was very appealing but there were some “minor” problems that had to be solved.  What held the nucleus together to be so s ...
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Physics of the Atom

LT1: Electron.NOTES - Simpson County Schools
LT1: Electron.NOTES - Simpson County Schools

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CHAPTER 4 TEST REVIEW GUIDE
CHAPTER 4 TEST REVIEW GUIDE

Radiation and quantised orbits
Radiation and quantised orbits

... But in his model, Bohr directly assumed that the orbits in which electrons revolve are NON RADIATING. According to him, the orbits are quantised, but then what happened to classical theory of electrodynamics? ...
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Bohr model



In atomic physics, the Rutherford–Bohr model or Bohr model, introduced by Niels Bohr in 1913, depicts the atom as a small, positively charged nucleus surrounded by electrons that travel in circular orbits around the nucleus—similar in structure to the solar system, but with attraction provided by electrostatic forces rather than gravity. After the cubic model (1902), the plum-pudding model (1904), the Saturnian model (1904), and the Rutherford model (1911) came the Rutherford–Bohr model or just Bohr model for short (1913). The improvement to the Rutherford model is mostly a quantum physical interpretation of it. The Bohr model has been superseded, but the quantum theory remains sound.The model's key success lay in explaining the Rydberg formula for the spectral emission lines of atomic hydrogen. While the Rydberg formula had been known experimentally, it did not gain a theoretical underpinning until the Bohr model was introduced. Not only did the Bohr model explain the reason for the structure of the Rydberg formula, it also provided a justification for its empirical results in terms of fundamental physical constants.The Bohr model is a relatively primitive model of the hydrogen atom, compared to the valence shell atom. As a theory, it can be derived as a first-order approximation of the hydrogen atom using the broader and much more accurate quantum mechanics and thus may be considered to be an obsolete scientific theory. However, because of its simplicity, and its correct results for selected systems (see below for application), the Bohr model is still commonly taught to introduce students to quantum mechanics or energy level diagrams before moving on to the more accurate, but more complex, valence shell atom. A related model was originally proposed by Arthur Erich Haas in 1910, but was rejected. The quantum theory of the period between Planck's discovery of the quantum (1900) and the advent of a full-blown quantum mechanics (1925) is often referred to as the old quantum theory.
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