Introduction to Atomic Physics

Choose a study mode

Play Quiz
Study Flashcards
Spaced Repetition
Chat to Lesson

Podcast

Play an AI-generated podcast conversation about this lesson
Download our mobile app to listen on the go
Get App

Questions and Answers

What is atomic physics?

The scientific study of the structure of the atom, its energy states, and its interactions with other particles and with electric and magnetic fields.

What are the components of an atom?

A small nucleus consisting of protons and neutrons surrounded by rapidly moving electrons.

What is the mass and charge of a neutron and a proton?

Protons and neutrons have about the same mass (1.00728 amu and 1.00867 amu respectively), and a neutron is electrically neutral while a proton has a positive charge (+1.6 x 10^-19 Coulomb).

What does the equation A=Z+N represent?

<p>A is the atomic mass number of an atom, Z is the atomic number (number of protons), and N is the number of neutrons.</p> Signup and view all the answers

Which atomic model suggested that all matter consists of extremely small particles called atoms?

<p>Dalton's atomic model (A)</p> Signup and view all the answers

What significant discovery did J.J. Thomson make in 1897?

<p>He discovered the electron, a negatively charged particle.</p> Signup and view all the answers

In 1911, Ernest Rutherford concluded that the atom contained a dense, positively charged region at its center called the _____ .

<p>nucleus</p> Signup and view all the answers

What did Niels Bohr propose about electron orbits in 1913?

<p>He proposed the quantized shell model of the atom, which explained how electrons have stable orbits around the nucleus.</p> Signup and view all the answers

The _____ constant () is used in the equation relating wavelength and energy transitions in atomic spectra.

<p>Rydberg</p> Signup and view all the answers

What is time dilation?

<p>Time passes more slowly for an observer in relative motion compared to a stationary observer.</p> Signup and view all the answers

What effect does special relativity predict about the mass of an object as it approaches the speed of light?

<p>It increases. (B)</p> Signup and view all the answers

What is the mass-energy equivalence formula?

<p>E = mc²</p> Signup and view all the answers

What are atomic orbitals?

<p>Atomic orbitals are mathematical functions that describe the location and wave-like behavior of an electron in an atom.</p> Signup and view all the answers

What do Hund's rules describe?

<p>They describe how electrons fill orbitals in a way that maximizes the number of unpaired electrons.</p> Signup and view all the answers

What principle states that no two electrons in the same atom can have identical values for all four of their quantum numbers?

<p>Pauli Exclusion Principle (C)</p> Signup and view all the answers

Electromagnetic radiation can be described as the flow of _____ through space.

<p>photons</p> Signup and view all the answers

What is the consequence of absorption of a quantum of energy by an atom?

<p>It can take the atom from a lower to a higher state of energy.</p> Signup and view all the answers

Which rule related to electronic transitions requires no change in the total electron spin?

<p>ΔS = 0 Rule (A)</p> Signup and view all the answers

Flashcards

Atomic Physics

Study of atom structure, energy states, and interactions with particles/fields.

Quantum mechanics role

Quantum mechanics is crucial.

Atom Configuration

Protons and neutrons in the center, surrounded by moving electrons.

Nuclear Symbol

Represents protons, neutrons, and electrons.

Signup and view all the flashcards

Isotopes

Atoms of the same element with different neutron numbers.

Signup and view all the flashcards

Dalton's Atomic Model

Each element has same atoms.

Signup and view all the flashcards

Dalton's ratios

Atoms combine in simple ratios.

Signup and view all the flashcards

Thomson's Model

Atoms are like plum pudding.

Signup and view all the flashcards

Rutherford's Conclusion

Atoms are mostly empty space.

Signup and view all the flashcards

Atomic Nucleus

Dense, positive center of an atom.

Signup and view all the flashcards

Bohr's Model

Electrons orbit at specific energy levels.

Signup and view all the flashcards

Energy Transitions

Electrons release energy moving orbits.

Signup and view all the flashcards

Modern Atomic Model

Atoms have nucleus in a cloud of electrons.

Signup and view all the flashcards

Atomic Spectra

Unique light patterns show element composition.

Signup and view all the flashcards

Continuous Spectrum

Light wavelengths vary continuously.

Signup and view all the flashcards

Line spectrum

Wavelengths are separate values/colors.

Signup and view all the flashcards

Angular Momentum

Momentum is multiple of h/2π.

Signup and view all the flashcards

Relativistic effects

The laws of physics are same for all.

Signup and view all the flashcards

Time Dilation

Time slows for moving objects.

Signup and view all the flashcards

Length Contraction

Length decreases for moving objects.

Signup and view all the flashcards

Relativistic Mass

Mass increases near light's speed.

Signup and view all the flashcards

Simultaneity

Events are relative.

Signup and view all the flashcards

Mass-Energy Equivalence

Mass converts to energy and vice versa.

Signup and view all the flashcards

Spin-Orbit Coupling

Magnetic interaction results.

Signup and view all the flashcards

Quantum Numbers

Four numbers describe atom.

Signup and view all the flashcards

Principal Number

Energy/size, all at level.

Signup and view all the flashcards

Spin direction

Electron can only be in two directions.

Signup and view all the flashcards

Pauli's Exclusion

Can't share number value.

Signup and view all the flashcards

Atomic Orbital

Describes location/behavior of electron.

Signup and view all the flashcards

Hund's Rule

Each subshell is singly so no double.

Signup and view all the flashcards

Perturbation

Study via approximation.

Signup and view all the flashcards

Fine Structure

Splitting due to a term.

Signup and view all the flashcards

Perturbation Method

Shifts energy from system by level.

Signup and view all the flashcards

Commuting operators

Application won't change result.

Signup and view all the flashcards

Chemical bond and vibration

Absorbed radiation.

Signup and view all the flashcards

Emission Specra

Is to determine composition.

Signup and view all the flashcards

Transition

Change physical state to another.

Signup and view all the flashcards

Selection rules

Restrictions in mechanics.

Signup and view all the flashcards

Study Notes

Introduction to Atomic Physics

  • Atomic physics scientifically explores the structure of atoms, their energy states, and interactions with particles, electric, and magnetic fields.
  • Quantum mechanics has proven to be applicable in atomic physics, establishing itself as a cornerstone of modern physics.
  • An atom's configuration is a small nucleus of protons and neutrons surrounded by rapidly moving electrons.
  • The atomic diameter is typically around 10^-10 meters, while the nucleus is about 10^-15 meters.
  • Protons and neutrons possess approximately the same mass, around 1.00728 and 1.00867 amu, respectively, and are about 1800 times heavier than electrons.
  • Neutrons are electrically neutral, while protons have a positive charge of +1.6 x 10^-19 Coulombs.
  • The charge of a proton is exactly opposite the negative charge of an electron.
  • In a neutral atom, electrons orbiting the nucleus equals to the number of protons in the nucleus.

Atomic Number and Isotopes

  • An important equation for atomic components is A = Z + N, where A is the atomic mass number, Z is the atomic number, and N is the neutron number.
  • The atomic number (Z) signifies the number of protons in the nucleus, characterizing a chemical element.
  • A denotes the atomic mass number; N denotes the number of neutrons within the nucleus.
  • Elements are characterized by Z (number of protons); elements sharing the same Z but differing in N and A are termed isotopes.
  • A hydrogen atom has A=1 indicating one proton, one electron, and zero neutrons.

Early Atomic Models

  • Scientists throughout history have attempted to understand the structure of the atom by proposing various models.
  • In 1808, John Dalton proposed that each element consists of identical atoms.
  • In 1811, Amedeo Avogadro suggested elements consist of particles with two or more atoms combined.
  • Avogadro termed these molecules, estimating molecules in hydrogen or oxygen gas to be pairs of atoms.

Dalton's Atomic Model

  • Dalton's atomic model was based on experimental results.
  • The model claimed that all matter consists of small particles called atoms.
  • Atoms are indestructible and resist changes.
  • Atoms cannot be created, destroyed, divided, or transformed into other types.
  • The conclusions were based on the law of conservation of mass in the late 1700s.
  • Every element is characterized by a unique atomic mass.
  • All atoms of a single element have identical shape, size and mass.
  • Atoms combine in chemical reactions in small whole-number ratios to form what is known as molecules.
  • Atoms of different types can form molecules with simple whole-number ratios like carbon monoxide and carbon dioxide which have differing quantities of carbon and oxygen atoms.

Thomson's Atomic Model

  • J.J. Thomson discovered the negatively charged electron in 1897.
  • Atoms are large positively charged bodies with negatively charged electrons scattered throughout.
  • The model is known as the "plum-pudding" model from 1904.
  • Electrons sit in a uniform sphere of positive charge, like blueberries in a muffin.

Rutherford's Experiment and Conclusions

  • In 1911, Ernest Rutherford, found the majority of alpha particles passed through a gold foil.
  • Some alpha particles deflected at angles, with a fraction bouncing back.
  • Rutherford concluded the atom contains a dense, positively charged nucleus at its center.
  • The positive charge and most of the mass are concentrated in the nucleus.
  • The atom mostly contains empty space with relatively smaller, negatively charged electrons.

Bohr's Atomic Model

  • In 1913, Niels Bohr (a student of Rutherford) proposed his shell model of the atom to explain stable electron orbits around the nucleus.
  • Classical mechanics and electromagnetic theory made Rutherford's model unstable, because charged particles moving along a curve emit electromagnetic radiation.
  • Bohr stated each orbit has a unique energy level, with distance from nucleus determining the force on electrons.
  • Energy is absorbed when electrons move to a higher orbit, and released when electrons fall to a lower energy orbit.

Modern Quantum Atomic Model

  • In 1926, Erwin Schrödinger employed mathematical equations to describe the probability of locating electrons in specific locations via the Schrödinger equation.
  • It defines electron position as a region where location is highly probable.
  • In modern models, atoms contain a nucleus of protons and neutrons surrounded by an ill-defined cloud of electrons.
  • Representing electrons as a cloud accounts for their probabilistic behavior.
  • Quantum mechanics continues to advance atomic theory and subatomic particles called Quarks were found in the 1960s.

Hydrogen Atom Spectroscopy

  • Atomic spectra arise from transitions between the energy states (levels) of individual atoms.
  • These are analytical tools which determine the composition of matter.
  • Studying the sun's radiation spectrum aided in understanding its atomic composition.
  • Scientists observed specific emission spectra lines when hydrogen atoms were excited.
  • Spectra were observed to be not continuous.
  • Understanding quantum mechanics describes how spectral lines arise.
  • Lines in the hydrogen spectrum can be classified into series named after their discoverers, which correlate to the energies from transitions between energy levels.
  • The wavelengths can be calculated using a simple enough relation involving Rydberg's constant.

Rydberg Constant and Spectral Series

  • The mentioned relation accurately predicts the spectral lines.

  • The equation for wavelength (and energy via E=hv) involving transition from n1 to n2 state was presented:

  • _R_H is Rydberg's constant equating to 10973731.6 m^-1 or 1.097 x 10^7 m^-1.

  • Note that n1 < n2 holds true.

  • Lyman series (n1=1), Balmer series (n1=2), Paschen series (n1=3) appear.

  • E = hv relates to the energy of electromagnetic waves.

  • C = vλ relates to the speed of electromagnetic wave which travels at 3 * 10^8 m/s.

Spectrum Types and Angular Momentum

  • Continuous spectrum happens when light wavelengths vary continuously, while line spectrum happens when light wavelengths come in separate values

  • The angular momentum of an electron with mass m and velocity v going along a orbit with radius r satisfies the following relation:

  • Where n is a positive integer and known as the principal quantum number.

Time Dilation

  • Special relativity, proposed by Albert Einstein in 1905, introduced a new understanding of space and time.
  • Laws of physics are the same in all inertial frames of reference.
  • The speed of light (c = 300,000 km/s) is constant for all observers.
  • The theory challenges classical Newtonian physics.
  • Time dilation is a relativistic effect where time passes slowly for a moving observer.
  • The clock on the spaceship runs slow or about 6 years while the Earth observer measures 10 years.
  • This becomes significant at speeds approaching that of light.
  • GPS satellites use time dilation to correct their clocks, ensuring accurate positioning because atomic clock rates are offset by about 38 microseconds per day.
  • Particle accelerators use time dilation to achieve high particle energies.
  • v2 Equation: Δt′ = Δt √1 − 𝑐2

Length Contraction

  • Length contraction happens as object velocity approaches light speed.
  • Length reduces along direction of motion for stationary observer.
  • Hendrik Lorentz independently contributed to this phenomenon, called Lorentz contraction. 𝑣2
  • L′ = 𝐿 √1 − 𝑐2

Relativistic Mass Increase

  • As objects moves closer to light speed, its relativistic mass increases.
  • Acceleration becomes more difficult and requires infinite energy to reach the speed of light. m
  • m′ = 2 √1− 𝑣2 𝑐

Simultaneity

  • Simultaneity is challenged in special relativity; simultaneous events for one observer may not be simultaneous for another in relative motion.
  • Ultimately, Einstein concluded that simultaneity is relative.

Equations for Relativistic Energy and Momentum

  • New equations for energy and momentum reduce to classical equations at low speeds.
  • These equations are essential for understanding particles at relativistic speeds, confirmed by particle physics. m 𝑐2
  • Energy: E = 2 √1− 𝑣2 𝑐 m𝑣
  • Momentum: p = 2 √1− 𝑣2 𝑐

Mass-Energy Equivalence

  • Mass and energy are equivalent is explained by the equation E = mc².
  • The equation explains the energy that is released during nuclear reactions and the foundation for nuclear weapons and energy.
  • Mass converts into sunlight during nuclear fusion of hydrogen atoms in the sun, which creates solar power.

Spin Orbit Coupling and Fine Structure

  • Conventional atomic theory can not account for spectral lines consisting of closely spaced sets.
  • Transitions between energy levels which is characterized by the principle quantum number n was not sufficient.
  • Besides Bohr and Sommerfield's model, emission spectrum of hydrogen had fine structure, additional lines which could not be explained above.
  • Additional relativistic correction in Bohr and Sommerfield's model was also able to explain certain fine structure.
  • The theory was unable to account for alkali atoms however, which has a sole electron orbiting outside a spherically symmetric core.
  • Uhlenbeck, Goudsmit and Dirac introduced electron spin, originating the idea of spin-orbit coupling, accounting for fine structure.

The Quantum Physics of Spin–Orbit Coupling

  • A magnetic dipole can be explained as an example of spin orbit coupling in a magnetic field.
  • The energy of said magnetic dipole is represented as E = ½ I w2.
  • An electron acts like a magnet due to spin.
  • An electron orbiting the nucleus behaves like a magnet.
  • The interaction of the spin and orbital motion of the electron will cause it to couple and this is called spin-orbit coupling.
  • The orientation between the two magnetic moments causes the orbital energy to be slightly altered.
  • The orange color of the sodium lamp, due to Na D line, can be used as a paradigm line with the emission at 17000 cm^-1.
  • Spin-orbit interactions satisfy relativistic and quantum mechanics, using the more complex Dirac equation.
  • Looking closely at the transitioned lines reveals a separation into two bands.

Fine-Structure Doubling and Angular Momentum

  • Fine-structure doubling of spectral lines stems from magnetic interaction between spin and orbital angular momenta, termed spin-orbit coupling.
  • Spin-orbit's classical model includes an electron circling nucleus that find itself in a magnetic field.
  • The magnetic field applies to and interacts with the electron’s spin causing a kind of internal Zeeman Effect.
  • Each electron has orbital angular momentum L and spin angular momentum S that contribute to total angular momentum J.
  • Orbital angular momenta Li of electron are coupled into L and this is equivalent to S being coupled into Si J = L + S (1). Quantized angular momenta L, S, and J have magnitude:
  • l=√(l+1)ħ, s=√(s+1)ħ, and J=√(j+1)ħ (2). j = l + s= l ± ½ (3), where j is l coupled with s.
  • If l = 0, then, j has the single value j=1/2 ((j = – ½ is not allowed as j is non-negative
  • Jz, the J component in the z direction, is Jz = mj ћ (4), where mj = (-j), (-j + 1),... , (j – 1), (j) (5).

Examples of Jz Orientation

  • When l= 1 the orbital and spin angular-momentum vectors cannot be exactly parallel/antiparallel (showed in Figures)
  • Possible Jz orientations for l = 1 (equation 3) j = 3/2 and j=1/2 that correspond to l = 1, with equation (4), mj = (-j), (-j + 1),... , (j – 1), (j).
  • For the j=3/2 state, equation (4) and (5) gives mj = −3/2 , −1/2, 1/2 , 3/2

Quantum Numbers and Orbitals

  • Four quantum numbers describe electrons (n, l, ml, ms).
  • The first three define certain orbital, while the last defines the electron occupation number.
  • 'n' the principal quantum number defines electron level and orbital size
  • Orbitals sharing 'n' are in the equal shell
  • Hydrogen atoms with n=1 electrons are in the base state while having n=2 electrons would indicate excitation. Number of equal value 'n' orbitals is n².
  • 'l' (0 to n-1) the secondary quantum number defines shell shape and distinguishes shell. Letters prevent "n and l" confusion
  • The energy (n) and the shape (l) specifies direction, and this 'ml equal to -l to +l specifies orbitals.
  • Every subs hell with 2l + 1 orbitals is divisible by the number, where s has one, p has three etc as shown.

Spin and Diamagnetism Exclusion

  • The spin is defined by ms, as 'spin axis' orientation'. It may measure as -0.5 to 0.5
  • A spinning electron forms magnetic field in one out of two ways
  • Two electron share an orbital which leads to spin pairing, hence diamagnetism
  • Paramagnetic atoms with an unbalanced are weakly magnetic.
  • "No two electron can share all 4 key numbers" Pauli states.
  • Hence every orbitals has at most 2 electrons spinning and opposite direction.

Hund's Rule and Atomic Orbitals Definition

  • In quantum mechanics, atomic orbitals are equations representing location and wave properties of atom electrons. Orbitals are for calculating probabilities of electrons near atom nucleus.
  • Atomic orbitals solve the Schrodinger Equation and describe likely locations.
  • The Schrödinger Equation defines atomic orbitals.
  • The description of time is separate in the Schrodinger Equation.
  • In reference to hydrogen-like atoms these equations are: (equations shown)

Essential Points of Atomic Orbitals

  • A space has a high chance of containing a pair of electrons.
  • Orbitals reveal electron placement in an atom.
  • Energy levels/subshells define different shapes where electrons are found.
  • Solutions determine Schrodinger's equations.
  • Orbitals show boxes linked by levels using small arrows.

Electronic Configuration Rules

  • 3 rules organize the e configuration.
  • The Aufbau rule says the electrons fill the lowest energy
  • Pauli Exclusion says the orbitals contain at most two electrons and that they are anti-aligned
  • Hund's rule says that sublevels contain a single electron in each orbital till occupied, anti-aligned to increase spin.
  • You first full the second then first main number
  • Filling follows "s" or the sublevel marking
  • Li or Lithium and Be or Beryllium are examples

Studying That Suits You

Use AI to generate personalized quizzes and flashcards to suit your learning preferences.

Quiz Team

Related Documents

More Like This

Atomic Structure and Quantum Mechanics
21 questions
Atomic Structure and Quantum Mechanics
40 questions

Atomic Structure and Quantum Mechanics

WellEstablishedDialect3586 avatar
WellEstablishedDialect3586
Use Quizgecko on...
Browser
Browser