1. Atomic structure Flashcards

1
Q

Principal vs azithumal/angular momentum vs magnetic vs spin quantum number

A

Energy level/shell, n, max # of e- w/in a shell: 2n^2 vs subshell, l, max # of e- w/in a subshell: 4l + 2, ranges from 0 to n-1 (ie. In the first shell, you have one subshell which is l=0; in the second shell, you have two subshells which are l=0 and l=1; etc); energy of subshells inc with increasing l values (ex: 3d has more energy than 4s, but lower than 4p) vs # of orbitals, ranges b/w l and -l including 0 vs spin and momentum, either +1/2 or -1/2

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2
Q

Balmer series vs Lyman series vs Paschen series in atomic emission spectrum of hydrogen from Bohr model

A

H+ emission lines transitioning from n>2 to n=2 vs n>1 to n=1 vs n>/=4 to n=3

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3
Q

Heisenberg uncertainty principle

A

Can’t find e-‘s momentum and position simultaneously; if one of them has more certainty, then the other has more uncertainty

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4
Q

How to find energy of e- going b/w energy levels

A

E = -RH(1/n^2 initial minus 1/n^2 final)

-RH (Rydberg unit of energy aka energy of e-) is a constant: 2.18E-18 J/e-

Energy of e- b/w energy levels corresponds to EXACT energy of a photon —> can use Planck’s eqn

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5
Q

Avogadro’s number

A

6.02E23

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6
Q

Planck’s eqn and constant

A

Describes energy of a quantum
E = hf
h = 6.626E-34 J*s

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7
Q

Ground state vs excited state

A

State of lowest energy (usually closest to nucleus) vs state of higher than nml energy (usually farther from nucleus)

As e- move from lower to higher energy levels, they get AHED: absorbs energy, higher potential, excited, distant from nucleus

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8
Q

How to find electromagnetic energy of photons

A

E = hc/lambda

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9
Q

Pauli exclusion principle vs Aufbau principle/building up principle

A

No 2 e- can have same set of 4 quantum numbers (ie. Only max of 2 e- in each orbital and the 2 e- in the orbitals must have opposite spins) vs e- full from lower to higher energy subshells

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10
Q

Paramagnetic vs diamagnetic vs ferromagnetic

A

Magnetic field will cause parallel spins in unpaired e- —> weak attraction (ex: gold, aluminum, copper) vs material that only has paired e- and has no net magnetic field —> repelled by magnetic field (ex: wood, plastic, glass) vs have unpaired e- and magnetic dipoles oriented randomly —> no net magnetic dipole, BUT is still strongly attracted to a magnetic field (ex: iron, nickel and cobalt)

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11
Q

Spectroscopic notation

A

It’s electron config; s represents l=0 subshell, p represents l=1 subshell, d represents l=2 subshell, and f represents l=3 subshell

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12
Q

Mass number vs atomic number symbols

A

A vs Z

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13
Q

n + l rule

A

The lower the sum of n+l —> the lower the energy of subshell (ie. the closer the e- is to the nucleus). If 2 subshells have same n+l value —> the lower n value has lower energy. This rule determines which e-or subshell = closer to nucleus

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14
Q

Electron config for cations

A

When you move back an element —> you remove a subshell with highest n value first (ex: nml e- config for Mn is [Ar]4s^23d^5, for Mn+ is [Ar]4s^13d^5)

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15
Q

Bohr model vs Quantum mechanical model

A

e- = in fixed orbit outside of nucleus vs e- in orbitals or clouds outside of nucleus

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16
Q

Is it possible to move up/down multiple energy levels in Bohr’s model?

A

Yep, as long as the e- absorb/emit the EXACT photon energy needed to reach the shell

17
Q

What’s the relationship b/w energy and stability? vs Energy and freq?

A

Inverse vs direct

18
Q

Electrostatic force

A

Attractive force b/w nucleus and valence e-, or force b/w charged particles; inc up (cuz of dec radius) and right (cuz of inc Zeff) on periodic table. Derived from Coulumbs law. Proportional to (charge of e-*Zeff)/r^2

19
Q

What is the shielding effect?

A

Valence e- don’t feel attractive force from nucleus b/c core e- shield them from nucleus; affect Zeff

20
Q

What happens to energy differences when you inc energy levels (aka n)?

A

energy differences become smaller as you inc energy lvls (ex: Ne will have higher energy diff when moving b/w energy lvls than Xe)