You Gotta Know These 20th Century Physicists Flashcards

1
Q

reconciled Rutherford’s results from the gold foil experiment with Max Planck’s quantum theory to create a model of the atom in which electrons resided in specific energy levels at specific stable radii

A

Niels Bohr

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2
Q

His model was the basis for Johann Balmer’s work with spectroscopy and Johannes Rydberg’s energy formula

A

Niels Bohr

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3
Q

He and his son fled to the U.S. in World War II under the pseudonym “Baker,” and contributed to the Manhattan Project.

A

Niels Bohr

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4
Q

proposed that all particles have a characteristic wavelength dependent on their momentum, which Einstein endorsed

A

Louis de Broglie

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5
Q

In opposition to the probabilistic interpretation of quantum mechanics, he later worked to define a purely causal interpretation, but his work remained unfinished until David Bohm refined it in the 1950s.

A

Louis de Broglie

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6
Q

quantified the wave-particle duality of quantum mechanics

A

Louis de Broglie

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7
Q

had an annus mirabilis (miracle year)

A

Albert Einstein

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8
Q

explained the photoelectric effect in terms of quantized electromagnetic radiation

A

Albert Einstein

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9
Q

formed the foundation for modern statistical physics by explaining the seemingly-random motion of particles in a fluid, a behavior called Brownian motion

A

Albert Einstein

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10
Q

reconciled Maxwellian electrodynamics with classical mechanics by positing a finite, constant speed of light, a theory now known as special relativity

A

Albert Einstein

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11
Q

published his theory of general relativity, which generalized special relativity to account for gravitational fields

A

Albert Einstein

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12
Q

best known to the public as a main contributor to the Manhattan Project

A

Enrico Fermi

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13
Q

applied the Pauli exclusion principle to subatomic particles to create Namesake-Dirac statistics, which accurately predicted the low-temperature behavior of electrons. Particles that obey these statistics are fermions.

A

Enrico Fermi

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14
Q

suggested the existence of the neutrino in order to balance nuclear beta-decay chains.

A

Enrico Fermi

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15
Q

created quantum electrodynamics

A

Richard Feynman

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16
Q

developed a mathematical formalism called the path integral formulation of quantum theory that utilized the “sum over histories,”

A

Richard Feynman

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17
Q

developed namesake diagrams, which illustrate the interaction of subatomic particles

A

Richard Feynman

18
Q

accomplished bongo player and sketch artist.

A

Richard Feynman

19
Q

was one of the first to explain the implications of the Big Bang theory of cosmology

A

George Gamow

20
Q

correctly predicted the abundance of hydrogen and helium in the early universe, nicknamed Alpher-Bethe-namesake theory (an intentional pun on the first three letters of the Greek alphabet, alpha, beta, and gamma)

A

George Gamow

21
Q

theorized that the the heat from the Big Bang would still be visible as the cosmic microwave background radiation

A

George Gamow

22
Q

Arno Penzias and Robert Wilson, as well as two later observers, John Mather and George Smoot, did receive Nobels for Cosmic Microwave Background Radiation although this physicist didn’t

A

George Gamow

23
Q

known for his matrix interpretation of quantum theory, which constructs observable quantities as operators that act on a system

A

Werner Heisenberg

24
Q

His famous uncertainty principle states that the more accurately an object’s position can be observed, the less accurately its momentum can

A

Werner Heisenberg

25
Q

discovered the allotropic forms of hydrogen.

A

Werner Heisenberg

26
Q

solved the ultraviolet catastrophe, which was a predicted unbounded increase in the amount of radiation emitted at high frequencies

A

Max Planck

27
Q

His namesake Law of Radiation superseded the Rayleigh-Jeans Law

A

Max Planck

28
Q

suggested that electromagnetic energy could only be emitted in specific packages, called quanta (singular quantum)

A

Max Planck

29
Q

posited that the energy of this photon was equal to its frequency times a fixed value h, now known as his namesake constant.

A

Max Planck

30
Q

his gold foil experiment provided the first evidence that each atom is made up of a large, positively-charged nucleus, surrounded by a cloud of negatively-charged electrons

A

Ernest Rutherford

31
Q

an early leader in nuclear fission techniques, having discovered the decay of carbon-14 and providing the impetus for modern carbon dating

A

Ernest Rutherford

32
Q

discovered the proton and neutron, the latter in cooperation with James Chadwick

A

Ernest Rutherford

33
Q

He is the only native New Zealander with an element named after him (Rutherfordium)

A

Ernest Rutherford

34
Q

contributed to the early formulations of quantum theory as a foil to Werner Heisenberg, Niels Bohr, and Paul Dirac, criticizing their Copenhagen interpretation of quantum mechanics with thought experiments like his famous namesake Cat

A

Erwin Schrödinger

35
Q

formulated both the time-independent and time-dependent namesake equations, which are partial differential equations that describe how quantum systems behave

A

Erwin Schrödinger

36
Q

work was the basis for Heisenberg’s matrix formalism, Feynman’s path-integral formalism, and quantum mechanical perturbation theory

A

Erwin Schrödinger

37
Q

these two scientists isolated and experimented on radioactive materials

A

Marie and Pierre Curie

38
Q

one of the first to attempt a generalization of quantum theory to relativistic speeds, the result of which was the namesake equation.

A

Paul Dirac

39
Q

predicted the existence of quarks

A

Murray Gell-Mann

40
Q

determined the charge of the electron by meticulously observing oil droplets in an electric field and noting the time it took them to fall a certain distance

A

Robert Millikan

41
Q

oversaw much of the Manhattan Project, but was later stripped of his security clearance during the McCarthy-era Red Scare, as a result of his acquaintance with communists and his enmity with Edward Teller.

A

Robert Oppenheimer

42
Q

his namesake exclusion principle prohibits most types of particles from occupying the same state, and forms the basis for chemical bonds.

A

Wolfgang Pauli