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Flashcards covering the wave nature of light, quantum effects, Bohr's theory, and the fundamentals of quantum mechanics and quantum numbers based on lecture notes.
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Wave
A continuously repeating change or oscillation in matter or in a physical field.
Electromagnetic Wave
A wave consisting of oscillations in electric and magnetic fields traveling through space.
Wavelength (λ)
The distance between any two identical points on adjacent waves.
Frequency (ν)
The number of wavelengths that pass a fixed point in one unit of time, usually measured in Hertz (Hz) or s−1.
Speed of Light (c)
The wave speed for light, equal to 3.00×108m/s, related to wavelength and frequency by the equation c=νλ.
Electromagnetic Spectrum
The entire range of frequencies and wavelengths of electromagnetic radiation.
Diffraction
The property of waves where they spread out when they encounter an obstacle about the size of their wavelength.
Planck's Constant (h)
A fundamental constant assigned a value of 6.63×10−34J⋅s used in the energy formula E=hν.
Quantized
The property of having only specific, allowed values, such as the vibrational energies of atoms which can only be hν, 2hν, 3hν, etc.
Photoelectric Effect
The ejection of electrons from the surface of a metal when light exceeding a certain threshold frequency shines on it.
Photon
A particle of light proposed by Einstein that carries energy proportional to its frequency (E=hν).
Wave-Particle Duality of Light
The concept that light displays characteristics of both waves (frequency) and particles (photons).
Continuous Spectrum
A spectrum that contains all wavelengths of light.
Line Spectrum
A spectrum showing only certain colors or specific wavelengths of light, produced when atoms are heated.
Energy-Level Postulate
Bohr's idea that an electron can have only certain quantized energy values, given for hydrogen by En=−RH/n2.
Rydberg Constant (RH)
A constant used in calculating the energy of an electron in a hydrogen atom, valued at 2.179×10−18J.
Atomic Absorption
The process where an atom takes in light to move an electron from a lower energy level to a higher energy level (nf>ni), resulting in a positive ΔE.
Atomic Emission
The process where an atom releases light as an electron moves from a higher energy level to a lower energy level (nf<ni), resulting in a negative ΔE.
Quantum Mechanics
The branch of physics that mathematically describes the wave properties of submicroscopic particles like electrons.
Heisenberg's Uncertainty Principle
A principle stating it is impossible to know both the exact position (Δx) and momentum (mΔvx) of a particle simultaneously.
Wave Function (ψ)
A mathematical expression defined by Erwin Schrodinger that describes the probability of finding an electron at a given point around the nucleus.
Atomic Orbital
A wave function described by three quantum numbers (n, l, ml) that representing a region of space with a high probability of finding an electron.
Principal Quantum Number (n)
The quantum number on which the energy of an electron primarily depends, defining the energy level or shell (n=1,2,3,…).
Angular Momentum Quantum Number (l)
The quantum number that distinguishes subshells of different shapes, with values from 0 to (n−1), denoted as s, p, d, and f.
Magnetic Quantum Number (ml)
The quantum number that distinguishes orbitals of a given energy and shape but having different orientations, with values from −l to +l.
Spin Quantum Number (ms)
The quantum number referring to the two possible orientations of an electron's spin axis, with values of +1/2 or −1/2.
s Orbital
An atomic orbital that is spherical in shape.
p Orbital
An atomic orbital consisting of two lobes along a straight line through the nucleus.
Electronegativity trend down a group
Decreases. Each new shell adds more distance and electron shielding between the nucleus and bonding electrons, so the nucleus attracts shared electrons less effectively.
Electronegativity
Pull of an atom to its bonding electrons
Ionization energy
The energy required to remove a valance electron
Atomic radius
1/2 of the distance between a nuclei of two identically bonded atoms
Emission spectra
Pattern in which certain elements emit light
When elements are heated they emit light in a line spectrum based on the lights frequency
Line spectrum
Shows only certain colors/specific wavelengths of light
continuous spectrum
All Wavelength/frequencies of light, rainbow
Basis of the Bohr model
Electrons remain in fixed, orbits and transferred between orbits and discrete jumps, releasing and absorbing energy
Only works for H
Ground state
The lowest energy level/state and electron would exist at
Excited state
Highest energy level/state electron would exist at
Changes and energy level/states
Positive change in energy; when energy is absorbed, when electron is excited
Negative change and energy; when energy is released as photons, when electron falls back to ground state
Continlus
Equation to show change and energy/jump of electrons
E=- RH/n²
E=joules
Rydberg equation
Change in energy = RH (1/n²i-1/n²f)
Shows change of energy of electrons as it moves between energy levels
The sign of change in energy shows the direction of the energy because frequency and wavelength can’t be negative
Change in energy is equal to the energy of the photon
Effective nuclear charge
The pool that the nucleus has on an outer electron, it is lower than the number of protons because the core electrons block the full strength of the nucleus
Quantum theory
Describing the behavior of matter and energy at atomic and sub, atomic scales, particles behave like waves and exist in photons
Origins of quantum theory
Plancks discovery of photons with the photoelectric effect
Quantum mechanics
Branch of physics, that mathematically describes wave properties of sub microscopic particles
Electron affinity
The energy change that occurs an electron is acquired by a neutral atom makes an anion
History and development of the periodic table
Mendeleev made the first periodic table which was grouped by properties
Mostly defined atomic number and arranged the table by that
Newland made the law of octanes
Mendeleev
He organized elements by properties and looked for trends
Saw that when the elements were arranged by atomic weight, they were grouped in similar properties
Created first periodic table 1869
Left empty space is in periodic table for future elements to be discovered
Henry Mosley
1911
Found a pattern of nuclear charge in the number of protons creating the modern definition of atomic number
John newlands
Proposed the law of octanes
When elements are arranged by increasing atomic weight, every eighth element would have similar properties
This law broke down after calcium on the table, but remains true for periods 2 and 3
Effective nuclear charge
The pulling force valance electrons actually feel by the nucleus
This is lower than the actual force of the nucleus because of the shielding affect of the core electrons
Periods: increases across (same amount of core electrons so effect is the same but there and more ve and p)
Group: stay about the same
Ionization trends
periods: increase across periods
-as you add protons and electrons the same energy levels there is a stronger effective nuclear charge meaning there’s a stronger pull on the electrons inward
Groups: decrease
As you add energy levels the valence electrons become farther from the nucleus
Electronegativity trends
Periods: increase across periods
as you add protons and electrons in the same energy level the effect nucleus charge increases
The stronger the nucleur charge pulls the shared bonded electrons inward toward the nufelus
groups: decrease down groups
As you add energy levels, the valence electrons become farther from the nucleus so the effective nuclear charge is decreasing in the atom/nucleus is not attracting electrons as well
Atomic radius trends
Periods: decrease across a period
as you add protons and electrons in the same energy level the nucleur charge increases and pulls valence electrons inward
group: increases down a group
As you add energy levels the size of the atom increases and you increase the distance beteeen p and ve