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The Hydrogen Atom
By Saadia Shaukat
1
The Hydrogen Atom
➒Introduction
➒Schrodinger equation of Hydrogen atom
➒Quantum number
➒Magnetic Effect
➒Example
2
Introduction
A hydrogen atom is an atom of the chemical element hydrogen.
The electrically neutral atom contains a single positively charged
proton and a single negatively charged electron bound to the nucleus
by the Coulomb force.
General Symbol 1H
➒Protons1
➒Neutrons 0
3
4
Schrodinger Equation of Hydrogen Atom
We know that Schrodinger equation:
𝝏𝟐𝚿
ππ’™πŸ
+
𝝏𝟐𝚿
ππ’šπŸ
+
𝝏𝟐𝚿
ππ’›πŸ
+
πŸ–π…πŸπ
π’‰πŸ
𝑬 βˆ’ 𝒗 𝚿 = 𝟎
We can also write as:
Laplacian
π›πŸ
𝚿 +
πŸ–π…πŸπ
π’‰πŸ 𝑬 βˆ’ 𝒗 𝜳 = 𝟎
5
Continue..
We also know that:
𝛖 = βˆ’
π’π’†πŸ
πŸ’π…πœΊπ’π’“
Here (r) is the distance between electron and radius.
Hydrogen atom is a spherical symmetrical system. We can’t use
cartesian co-ordinates, we use spherical co-ordinates.
6
Conti…
Relation between cartesian and spherical co-
ordinates is given as:
𝛉 = π’„π’π’”βˆ’πŸ
𝒛
𝒓
𝛗 = π­πšπ§βˆ’πŸ ΰ΅—
𝐲
𝐱
𝒓 = π’™πŸ + π’šπŸ + π’›πŸ
7
Conti….
Schrodinger equation in spherical co-ordinates:
𝟏
𝒓
𝝏
𝝏𝒓
π’“πŸ
𝝏𝚿
𝝏𝒓
+
𝟏
π’“πŸπ’”π’Šπ’π›‰
𝝏
𝝏𝜽
π’”π’Šπ’ΞΈ
𝝏𝚿
𝝏𝜽
+
𝟏
π’“πŸπ’”π’Šπ’πŸπœ½
𝝏𝟐
𝝏𝚽𝟐
+
πŸ–π…πŸ
𝝁
π’‰πŸ
𝑬 βˆ’ 𝒗 𝚿
= 𝟎 … … 𝟏
we first separate the radial (r )and angular variables(ΞΈ,Ξ¦).
For this we substitute:
𝚿 𝒓, 𝜽, 𝝓 = 𝑹 𝒓 𝒀 𝜽, 𝝓 … . 𝟐
By solving equation 2) we get:
8
Conti…
𝝏𝚿
𝝏𝒓
= 𝒀
𝝏𝑹
𝝏𝒓
… . πŸ‘
𝝏𝚿
𝝏𝜽
= 𝑹
𝝏𝒀
𝝏𝜽
… . πŸ’
𝝏𝚿
𝝏𝝋
= 𝑹
𝝏𝒀
𝝏𝝋
Again differentiate we get:
𝝏𝟐𝚿
ππ‹πŸ = 𝑹
ππŸπ’€
ππ‹πŸ … . . πŸ“
9
Conti…
By putting equ 3,4 and 5 in equ 1 we get:
𝟏
π’“πŸ
𝝏
𝝏𝒓
π’“πŸ
𝒀
𝝏𝐑
𝝏𝒓
+
𝟏
π’“πŸπ’”π’Šπ’π›‰
𝝏
𝝏𝜽
π’”π’Šπ’ΞΈπ‘Ή
𝝏𝐘
𝝏𝜽
+
𝟏
π’“πŸπ’”π’Šπ’πŸπœ½
𝑹
ππŸπ’€
𝝏𝚽𝟐
+
πŸ–π…πŸπ
π’‰πŸ
𝑬 βˆ’ 𝒗 π‘π˜ = 𝟎
Multiplying above expression by
𝐫𝟐
π‘π˜
we get:
(
𝐫𝟐
π‘π˜
).
𝟏
𝐫𝟐
𝛛
𝛛𝐫
𝐫𝟐𝐘
𝛛𝐑
𝛛𝐫
+
𝐫𝟐
π‘π˜
.
𝟏
π«πŸπ¬π’π§π›‰
𝛛
𝛛𝛉
𝐬𝐒𝐧θ𝐑
π››π˜
𝛛𝛉
+
𝐫𝟐
π‘π˜
.
𝟏
π«πŸπ¬π’π§πŸπ›‰
𝐑
π››πŸπ˜
π››πš½πŸ +
𝐫𝟐
π‘π˜
.
πŸ–π›‘πŸπ›
𝐑𝟐 𝐄 βˆ’ 𝐯 π‘π˜ = 𝟎
10
Conti..
𝟏
𝐑
𝛛
𝛛𝐫
𝐫𝟐
𝛛𝐑
𝛛𝐫
+
𝟏
𝐘
.
𝟏
𝐬𝐒𝐧𝛉
𝛛
𝛛𝛉
𝐬𝐒𝐧θ
π››π˜
𝛛𝛉
+
𝟏
𝐘
.
𝟏
π¬π’π§πŸπ›‰
π››πŸπ˜
𝛛𝛗
+ 𝐫𝟐.
πŸ–π›‘πŸπ›
𝐑𝟐
𝐄 βˆ’ 𝐯 = 𝟎
And now we can write as:
𝟏
𝑹
𝝏
𝝏𝒓
π’“πŸ
𝒅𝐑
𝒅𝒓
+
𝟏
𝒀
.
𝟏
π’”π’Šπ’π›‰
𝝏
𝝏𝜽
π’”π’Šπ’ΞΈ
𝝏𝐘
𝝏𝜽
+
𝟏
𝒀
.
𝟏
π’”π’Šπ’πŸπœ½
𝝏𝟐𝐘
𝝏𝝋
+ π’“πŸ.
πŸ–π…πŸπ
π’‰πŸ
𝑬 βˆ’ 𝒗 = 𝟎
𝟏
𝑹
𝝏
𝝏𝒓
π’“πŸ
𝒅𝐑
𝒅𝒓
+ π’“πŸ.
πŸ–π…πŸπ
π’‰πŸ
𝑬 βˆ’ 𝒗 = βˆ’
𝟏
𝒀
𝟏
π’”π’Šπ’π›‰
𝝏
𝝏𝜽
π’”π’Šπ’ΞΈ
𝝏𝐘
𝝏𝜽
+
𝟏
π’”π’Šπ’πŸπœ½
𝝏𝟐𝐘
𝝏𝝋
11
Conti..
Hence this equation can be correct only if both sides are equal to some
constant.
Let this constant be 𝒍 𝒍 + 𝟏
The radial equation is:
𝟏
𝑹
𝝏
𝝏𝒓
π’“πŸ
𝒅𝐑
𝒅𝒓
+ π’“πŸ.
πŸ–π…πŸπ
π’‰πŸ
𝑬 βˆ’ 𝒗 = 𝒍 𝒍 + 𝟏 … . πŸ”
12
Conti..
And angular equation is:
βˆ’
𝟏
𝒀
𝟏
π’”π’Šπ’π›‰
𝝏
𝝏𝜽
π’”π’Šπ’ΞΈ
𝝏𝐘
𝝏𝜽
+
𝟏
π’”π’Šπ’πŸπœ½
𝝏𝟐𝐘
ππ‹πŸ
= 𝒍 𝒍 + 𝟏 … . πŸ•
Now again we have two variables there for
𝒀 𝜽, 𝝋 = 𝑸 𝜽 𝑭(𝝋)
Put in above expression we get:
βˆ’
𝟏
𝑸𝑭
𝟏
π’”π’Šπ’π›‰
𝝏
𝝏𝜽
π’”π’Šπ’πœ½
𝝏𝐐
𝝏𝜽
𝑭 +
𝟏
π’”π’Šπ’πŸπœ½
𝝏𝟐
𝐅
ππ‹πŸ
𝑸 = 𝒍 𝒍 + 𝟏
13
Conti…
Multiplying above expression with 𝑠𝑖𝑛2ΞΈ we get:
βˆ’
𝟏
𝑸
π’”π’Šπ’πœ½
𝒅
π’…πœ½
π’”π’Šπ’πœ½
𝒅𝐐
π’…πœ½
βˆ’
𝟏
𝑭
π’…πŸπ…
π’…π‹πŸ
= 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸπœ½
Rearrange the equation we get:
𝟏
𝑸
π’”π’Šπ’πœ½
𝒅
π’…πœ½
π’”π’Šπ’πœ½
𝒅𝐐
π’…πœ½
+ 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸπœ½ = βˆ’
𝟏
𝑭
π’…πŸπ…
π’…π‹πŸ
14
Conti..
Again two sides of the equation are function of different variables.
They must be equal to some constant.
β€’ Let this constant be π’Žπ’
𝟐
𝟏
𝑸
π’”π’Šπ’πœ½
𝒅
π’…πœ½
π’”π’Šπ’πœ½
𝒅𝑸
π’…πœ½
+ 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸ
𝜽 = π’Žπ’
𝟐
……. 8
And
βˆ’
𝟏
𝑭
π’…πŸ
𝐅
π’…π‹πŸ
= π’Žπ’
𝟐
… . πŸ—
15
Conti..
Equation 9 can be written as:
π’…πŸπ…
π’…π‹πŸ
= βˆ’π‘­ π’Žπ’
𝟐
π’…πŸπ…
π’…π‹πŸ
+ 𝑭 π’Žπ’
𝟐
= 𝟎 … 𝟏𝟎
For more simplification we multiplying equation 8 with ΰ΅—
𝑸
π’”π’Šπ’πŸΞΈ we get:
16
Conti..
β€’
𝑸
π‘Ίπ’Šπ’πŸπœ½
𝟏
𝑸
π’”π’Šπ’πœ½
𝒅
π’…πœ½
π’”π’Šπ’πœ½
𝒅𝑸
π’…πœ½
+ 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸ
𝜽 = π’Žπ’
𝟐
After simplification we get:
𝟏
π’”π’Šπ’πœ½
𝒅
π’…πœ½
π’”π’Šπ’πœ½
𝒅𝑸
π’…πœ½
+ 𝒍 𝒍 + 𝟏 𝑸 βˆ’
π’Žπ’
𝟐
π’”π’Šπ’πŸπœ½
=0 …..11
Multiplying equation 6 by ΰ΅—
𝐑
𝐫𝟐
𝐑
𝐫𝟐
𝟏
𝐑
𝛛
𝛛𝐫
𝐫𝟐
𝐝𝐑
𝐝𝐫
+ 𝐫𝟐.
πŸ–π›‘πŸπ›
𝐑𝟐
𝐄 βˆ’ 𝐯 = π₯ π₯ + 𝟏
17
Conti..
𝑹
π’“πŸ
𝟏
𝑹
𝒅
𝒅𝒓
π’“πŸ
𝒅𝑹
𝒅𝒓
+
πŸ–π…πŸπ
π’‰πŸ
𝑬 βˆ’ 𝒗 βˆ’
𝒍 𝒍 + 𝟏
π’“πŸ
𝑹 = 0
Thus we break down the Schrodinger equation of hydrogen atom into three
ordinary differential equation, each having a single variable.
We trying to find out acceptable solutions of these equation.
18
Quantum Number
Solution of the Equations
Solution of F(Ο†) equation 10 is:
𝑭 = π‘¨π’†π’Šπ’Žπ’π‹
A is constant.
Since Ο† repeats its value after 2Ο€.
Then:
𝑭(𝝋 + πŸπ…) = 𝑭(𝝋)
π‘¨π’†π’Šπ’Žπ’(𝝋+πŸπ…)
= π‘¨π’†π’Šπ’Žπ’π‹
19
Conti..
π’†π’Šπ’Žπ’(πŸπ…)
= 𝟏
𝒄𝒐𝒔 π’Žπ’πŸπ… βˆ’ π’Šπ’”π’Šπ’ π’Žπ’πŸπ… = 𝟏
𝒄𝒐𝒔 π’Žπ’πŸπ… = 𝟏
This can only happen when π’Žπ’ is zero or positive or negative integer.
β€’ Hence π’Žπ’ = 𝟎, ±𝟏, ±𝟐, Β±πŸ‘, … .
β€’ π’Žπ’ is magnetic quantum number.
20
Conti..
Finding the solution of equation 11
β€’ π‘Έπ’π’Žπ’
𝜽 = π‘΅π’π’Žπ’
𝑷𝒍
π’Žπ’
𝒄𝒐𝒔(𝜽)
π‘΅π’π’Žπ’
is a constant.
𝑷𝒍
π’Žπ’
is associated Legendre polynomial . Solution is acceptable if
𝒍 β‰₯ π’Žπ’
Here l is orbital quantum number.
21
Conti...
For solving equation 12 we must specify v(r).
β€’ In this case: 𝒗 𝒓 = βˆ’
π’π’†πŸ
πŸ’π…πœΊπ’π’“
Then the solution is given as:
𝑹𝒏,𝒍 𝒓 = 𝑡𝒏,𝒍𝒆 ΰ΅—
βˆ’π’›π’“
𝒏𝒂𝒐
πŸπ’π’
𝒏𝒂𝒐
𝑳𝒏+𝟏
πŸπ’+𝟏 πŸπ’›π’
𝒏𝒂𝒐
𝑡𝒏,𝒍 is a constant.
22
Conti..
𝑳𝒏+𝟏
πŸπ’+𝟏
is associated Laguerre polynomial.
Where
β€’ 𝒂𝒐 =
π’‰πŸπœΊπ’
π…ππ’†πŸ
β€’ This solution is only acceptable when E is positive or has one of the negative
values 𝑬𝒏 (which correspond the bound states).
𝑬𝒏 = βˆ’
ππ’›πŸπ’†πŸ’
πŸ–πœΊπ’
πŸπ’‰πŸ
𝟏
π’πŸ
23
Conti…
Where n is an integer which must be equal to or greater than (l+1).
𝒏 β‰₯ 𝒍 + 𝟏
i-e n=l+1,l+2,l+3,…..
Or l=0,1,2,3,…….. (n-1)
n is principle quantum number.
24
Magnetic effect on hydrogen atom
The Dutch physicist Pieter Zeeman (and 1902 physics Nobelist) observed with a state of the art
spectrometer of the time, (which we would now consider pretty crude) that many spectral lines
split in a magnetic field into three (and more) spectral lines, one stays at the original position,
the spacing of the other two depends linearly on the strength of the magnetic field. It is called
the Zeeman effect.
β€’ A good theory of the hydrogen atom needs to explain this !!
25
Normal zeeman effect
β€’ Normal Zeeman effect, which is actually not observed with modern spectrometers,
historically β€œnormal” because of easy explanation
β€’ Model the electron in the H atom as a small permanent magnet.
β€’ Think of an electron as an orbiting circular current loop of I = dq / dt around
some nucleus (that was not known to exist at that time).
β€’ The current loop has a magnetic moment ΞΌ and the period T = 2Ο€r / v. (don’t
confuse this ΞΌ with reduced mass)
β€’ where L = mvr is the magnitude of the orbital
β€’ angular momentum for a circular path.
26
Normal zeeman effect
β€’ When there is no magnetic field to
align them, doesn’t have a effect
on total energy. In an external
magnetic field a dipole has a
potential energy
27
Normal zeeman Effect
β€’ If there is a magnetic field in direction z, it will act on the magnetic moment, this
brings in an (extra) potential energy term into the Hamiltonian operator
β€’ So an external magnetic field should have an effect on atoms, spectral lines are
β€œfingerprint” characteristics of atoms, in an external magnetic field, each spectral
line should be splitting into three lines, distance between two extra lines
proportional to the strength of the magnetic field, tested by experiment, observed,
part of Nobel prize
28
The Normal zeeman effect for Hydrogen
β€’ The potential energy due to the external magnetic field is quantized due to
the magnetic quantum number mβ„“.
β€’ When a magnetic field is applied, the otherwise degenerate 2p level of
atomic hydrogen is split into three different energy states with energy
difference of Ξ”E = ΞΌBB Ξ”mβ„“.
29
Conti…
β€’ The larger B, the larger the
splitting, if B is switched off
suddenly, the three lines combine as
if nothing ever happened, total
intensity of lines remains constant
in the splitting
30
Conti…
𝑼 =
𝒆
πŸπ’Žπ’†
𝑳. 𝑩 =
𝒆𝑩
πŸπ’Žπ’†
𝑳𝒙 = β„πŽπ’π’Žπ’
β€’ What is really observed with good
spectrometers: there are a lot more
lines in atomic spectra when they
are in a magnetic field ! So called
Anomalous Zeeman effect, which
is the only one observed with good
spectrometers !!.
31
32
33
34
35
36
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Schrodinger Equation of Hydrogen Atom

  • 1. The Hydrogen Atom By Saadia Shaukat 1
  • 2. The Hydrogen Atom ➒Introduction ➒Schrodinger equation of Hydrogen atom ➒Quantum number ➒Magnetic Effect ➒Example 2
  • 3. Introduction A hydrogen atom is an atom of the chemical element hydrogen. The electrically neutral atom contains a single positively charged proton and a single negatively charged electron bound to the nucleus by the Coulomb force. General Symbol 1H ➒Protons1 ➒Neutrons 0 3
  • 4. 4
  • 5. Schrodinger Equation of Hydrogen Atom We know that Schrodinger equation: 𝝏𝟐𝚿 ππ’™πŸ + 𝝏𝟐𝚿 ππ’šπŸ + 𝝏𝟐𝚿 ππ’›πŸ + πŸ–π…πŸπ π’‰πŸ 𝑬 βˆ’ 𝒗 𝚿 = 𝟎 We can also write as: Laplacian π›πŸ 𝚿 + πŸ–π…πŸπ π’‰πŸ 𝑬 βˆ’ 𝒗 𝜳 = 𝟎 5
  • 6. Continue.. We also know that: 𝛖 = βˆ’ π’π’†πŸ πŸ’π…πœΊπ’π’“ Here (r) is the distance between electron and radius. Hydrogen atom is a spherical symmetrical system. We can’t use cartesian co-ordinates, we use spherical co-ordinates. 6
  • 7. Conti… Relation between cartesian and spherical co- ordinates is given as: 𝛉 = π’„π’π’”βˆ’πŸ 𝒛 𝒓 𝛗 = π­πšπ§βˆ’πŸ ΰ΅— 𝐲 𝐱 𝒓 = π’™πŸ + π’šπŸ + π’›πŸ 7
  • 8. Conti…. Schrodinger equation in spherical co-ordinates: 𝟏 𝒓 𝝏 𝝏𝒓 π’“πŸ 𝝏𝚿 𝝏𝒓 + 𝟏 π’“πŸπ’”π’Šπ’π›‰ 𝝏 𝝏𝜽 π’”π’Šπ’ΞΈ 𝝏𝚿 𝝏𝜽 + 𝟏 π’“πŸπ’”π’Šπ’πŸπœ½ 𝝏𝟐 𝝏𝚽𝟐 + πŸ–π…πŸ 𝝁 π’‰πŸ 𝑬 βˆ’ 𝒗 𝚿 = 𝟎 … … 𝟏 we first separate the radial (r )and angular variables(ΞΈ,Ξ¦). For this we substitute: 𝚿 𝒓, 𝜽, 𝝓 = 𝑹 𝒓 𝒀 𝜽, 𝝓 … . 𝟐 By solving equation 2) we get: 8
  • 9. Conti… 𝝏𝚿 𝝏𝒓 = 𝒀 𝝏𝑹 𝝏𝒓 … . πŸ‘ 𝝏𝚿 𝝏𝜽 = 𝑹 𝝏𝒀 𝝏𝜽 … . πŸ’ 𝝏𝚿 𝝏𝝋 = 𝑹 𝝏𝒀 𝝏𝝋 Again differentiate we get: 𝝏𝟐𝚿 ππ‹πŸ = 𝑹 ππŸπ’€ ππ‹πŸ … . . πŸ“ 9
  • 10. Conti… By putting equ 3,4 and 5 in equ 1 we get: 𝟏 π’“πŸ 𝝏 𝝏𝒓 π’“πŸ 𝒀 𝝏𝐑 𝝏𝒓 + 𝟏 π’“πŸπ’”π’Šπ’π›‰ 𝝏 𝝏𝜽 π’”π’Šπ’ΞΈπ‘Ή 𝝏𝐘 𝝏𝜽 + 𝟏 π’“πŸπ’”π’Šπ’πŸπœ½ 𝑹 ππŸπ’€ 𝝏𝚽𝟐 + πŸ–π…πŸπ π’‰πŸ 𝑬 βˆ’ 𝒗 π‘π˜ = 𝟎 Multiplying above expression by 𝐫𝟐 π‘π˜ we get: ( 𝐫𝟐 π‘π˜ ). 𝟏 𝐫𝟐 𝛛 𝛛𝐫 𝐫𝟐𝐘 𝛛𝐑 𝛛𝐫 + 𝐫𝟐 π‘π˜ . 𝟏 π«πŸπ¬π’π§π›‰ 𝛛 𝛛𝛉 𝐬𝐒𝐧θ𝐑 π››π˜ 𝛛𝛉 + 𝐫𝟐 π‘π˜ . 𝟏 π«πŸπ¬π’π§πŸπ›‰ 𝐑 π››πŸπ˜ π››πš½πŸ + 𝐫𝟐 π‘π˜ . πŸ–π›‘πŸπ› 𝐑𝟐 𝐄 βˆ’ 𝐯 π‘π˜ = 𝟎 10
  • 11. Conti.. 𝟏 𝐑 𝛛 𝛛𝐫 𝐫𝟐 𝛛𝐑 𝛛𝐫 + 𝟏 𝐘 . 𝟏 𝐬𝐒𝐧𝛉 𝛛 𝛛𝛉 𝐬𝐒𝐧θ π››π˜ 𝛛𝛉 + 𝟏 𝐘 . 𝟏 π¬π’π§πŸπ›‰ π››πŸπ˜ 𝛛𝛗 + 𝐫𝟐. πŸ–π›‘πŸπ› 𝐑𝟐 𝐄 βˆ’ 𝐯 = 𝟎 And now we can write as: 𝟏 𝑹 𝝏 𝝏𝒓 π’“πŸ 𝒅𝐑 𝒅𝒓 + 𝟏 𝒀 . 𝟏 π’”π’Šπ’π›‰ 𝝏 𝝏𝜽 π’”π’Šπ’ΞΈ 𝝏𝐘 𝝏𝜽 + 𝟏 𝒀 . 𝟏 π’”π’Šπ’πŸπœ½ 𝝏𝟐𝐘 𝝏𝝋 + π’“πŸ. πŸ–π…πŸπ π’‰πŸ 𝑬 βˆ’ 𝒗 = 𝟎 𝟏 𝑹 𝝏 𝝏𝒓 π’“πŸ 𝒅𝐑 𝒅𝒓 + π’“πŸ. πŸ–π…πŸπ π’‰πŸ 𝑬 βˆ’ 𝒗 = βˆ’ 𝟏 𝒀 𝟏 π’”π’Šπ’π›‰ 𝝏 𝝏𝜽 π’”π’Šπ’ΞΈ 𝝏𝐘 𝝏𝜽 + 𝟏 π’”π’Šπ’πŸπœ½ 𝝏𝟐𝐘 𝝏𝝋 11
  • 12. Conti.. Hence this equation can be correct only if both sides are equal to some constant. Let this constant be 𝒍 𝒍 + 𝟏 The radial equation is: 𝟏 𝑹 𝝏 𝝏𝒓 π’“πŸ 𝒅𝐑 𝒅𝒓 + π’“πŸ. πŸ–π…πŸπ π’‰πŸ 𝑬 βˆ’ 𝒗 = 𝒍 𝒍 + 𝟏 … . πŸ” 12
  • 13. Conti.. And angular equation is: βˆ’ 𝟏 𝒀 𝟏 π’”π’Šπ’π›‰ 𝝏 𝝏𝜽 π’”π’Šπ’ΞΈ 𝝏𝐘 𝝏𝜽 + 𝟏 π’”π’Šπ’πŸπœ½ 𝝏𝟐𝐘 ππ‹πŸ = 𝒍 𝒍 + 𝟏 … . πŸ• Now again we have two variables there for 𝒀 𝜽, 𝝋 = 𝑸 𝜽 𝑭(𝝋) Put in above expression we get: βˆ’ 𝟏 𝑸𝑭 𝟏 π’”π’Šπ’π›‰ 𝝏 𝝏𝜽 π’”π’Šπ’πœ½ 𝝏𝐐 𝝏𝜽 𝑭 + 𝟏 π’”π’Šπ’πŸπœ½ 𝝏𝟐 𝐅 ππ‹πŸ 𝑸 = 𝒍 𝒍 + 𝟏 13
  • 14. Conti… Multiplying above expression with 𝑠𝑖𝑛2ΞΈ we get: βˆ’ 𝟏 𝑸 π’”π’Šπ’πœ½ 𝒅 π’…πœ½ π’”π’Šπ’πœ½ 𝒅𝐐 π’…πœ½ βˆ’ 𝟏 𝑭 π’…πŸπ… π’…π‹πŸ = 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸπœ½ Rearrange the equation we get: 𝟏 𝑸 π’”π’Šπ’πœ½ 𝒅 π’…πœ½ π’”π’Šπ’πœ½ 𝒅𝐐 π’…πœ½ + 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸπœ½ = βˆ’ 𝟏 𝑭 π’…πŸπ… π’…π‹πŸ 14
  • 15. Conti.. Again two sides of the equation are function of different variables. They must be equal to some constant. β€’ Let this constant be π’Žπ’ 𝟐 𝟏 𝑸 π’”π’Šπ’πœ½ 𝒅 π’…πœ½ π’”π’Šπ’πœ½ 𝒅𝑸 π’…πœ½ + 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸ 𝜽 = π’Žπ’ 𝟐 ……. 8 And βˆ’ 𝟏 𝑭 π’…πŸ 𝐅 π’…π‹πŸ = π’Žπ’ 𝟐 … . πŸ— 15
  • 16. Conti.. Equation 9 can be written as: π’…πŸπ… π’…π‹πŸ = βˆ’π‘­ π’Žπ’ 𝟐 π’…πŸπ… π’…π‹πŸ + 𝑭 π’Žπ’ 𝟐 = 𝟎 … 𝟏𝟎 For more simplification we multiplying equation 8 with ΰ΅— 𝑸 π’”π’Šπ’πŸΞΈ we get: 16
  • 17. Conti.. β€’ 𝑸 π‘Ίπ’Šπ’πŸπœ½ 𝟏 𝑸 π’”π’Šπ’πœ½ 𝒅 π’…πœ½ π’”π’Šπ’πœ½ 𝒅𝑸 π’…πœ½ + 𝒍 𝒍 + 𝟏 π’”π’Šπ’πŸ 𝜽 = π’Žπ’ 𝟐 After simplification we get: 𝟏 π’”π’Šπ’πœ½ 𝒅 π’…πœ½ π’”π’Šπ’πœ½ 𝒅𝑸 π’…πœ½ + 𝒍 𝒍 + 𝟏 𝑸 βˆ’ π’Žπ’ 𝟐 π’”π’Šπ’πŸπœ½ =0 …..11 Multiplying equation 6 by ΰ΅— 𝐑 𝐫𝟐 𝐑 𝐫𝟐 𝟏 𝐑 𝛛 𝛛𝐫 𝐫𝟐 𝐝𝐑 𝐝𝐫 + 𝐫𝟐. πŸ–π›‘πŸπ› 𝐑𝟐 𝐄 βˆ’ 𝐯 = π₯ π₯ + 𝟏 17
  • 18. Conti.. 𝑹 π’“πŸ 𝟏 𝑹 𝒅 𝒅𝒓 π’“πŸ 𝒅𝑹 𝒅𝒓 + πŸ–π…πŸπ π’‰πŸ 𝑬 βˆ’ 𝒗 βˆ’ 𝒍 𝒍 + 𝟏 π’“πŸ 𝑹 = 0 Thus we break down the Schrodinger equation of hydrogen atom into three ordinary differential equation, each having a single variable. We trying to find out acceptable solutions of these equation. 18
  • 19. Quantum Number Solution of the Equations Solution of F(Ο†) equation 10 is: 𝑭 = π‘¨π’†π’Šπ’Žπ’π‹ A is constant. Since Ο† repeats its value after 2Ο€. Then: 𝑭(𝝋 + πŸπ…) = 𝑭(𝝋) π‘¨π’†π’Šπ’Žπ’(𝝋+πŸπ…) = π‘¨π’†π’Šπ’Žπ’π‹ 19
  • 20. Conti.. π’†π’Šπ’Žπ’(πŸπ…) = 𝟏 𝒄𝒐𝒔 π’Žπ’πŸπ… βˆ’ π’Šπ’”π’Šπ’ π’Žπ’πŸπ… = 𝟏 𝒄𝒐𝒔 π’Žπ’πŸπ… = 𝟏 This can only happen when π’Žπ’ is zero or positive or negative integer. β€’ Hence π’Žπ’ = 𝟎, ±𝟏, ±𝟐, Β±πŸ‘, … . β€’ π’Žπ’ is magnetic quantum number. 20
  • 21. Conti.. Finding the solution of equation 11 β€’ π‘Έπ’π’Žπ’ 𝜽 = π‘΅π’π’Žπ’ 𝑷𝒍 π’Žπ’ 𝒄𝒐𝒔(𝜽) π‘΅π’π’Žπ’ is a constant. 𝑷𝒍 π’Žπ’ is associated Legendre polynomial . Solution is acceptable if 𝒍 β‰₯ π’Žπ’ Here l is orbital quantum number. 21
  • 22. Conti... For solving equation 12 we must specify v(r). β€’ In this case: 𝒗 𝒓 = βˆ’ π’π’†πŸ πŸ’π…πœΊπ’π’“ Then the solution is given as: 𝑹𝒏,𝒍 𝒓 = 𝑡𝒏,𝒍𝒆 ΰ΅— βˆ’π’›π’“ 𝒏𝒂𝒐 πŸπ’π’ 𝒏𝒂𝒐 𝑳𝒏+𝟏 πŸπ’+𝟏 πŸπ’›π’ 𝒏𝒂𝒐 𝑡𝒏,𝒍 is a constant. 22
  • 23. Conti.. 𝑳𝒏+𝟏 πŸπ’+𝟏 is associated Laguerre polynomial. Where β€’ 𝒂𝒐 = π’‰πŸπœΊπ’ π…ππ’†πŸ β€’ This solution is only acceptable when E is positive or has one of the negative values 𝑬𝒏 (which correspond the bound states). 𝑬𝒏 = βˆ’ ππ’›πŸπ’†πŸ’ πŸ–πœΊπ’ πŸπ’‰πŸ 𝟏 π’πŸ 23
  • 24. Conti… Where n is an integer which must be equal to or greater than (l+1). 𝒏 β‰₯ 𝒍 + 𝟏 i-e n=l+1,l+2,l+3,….. Or l=0,1,2,3,…….. (n-1) n is principle quantum number. 24
  • 25. Magnetic effect on hydrogen atom The Dutch physicist Pieter Zeeman (and 1902 physics Nobelist) observed with a state of the art spectrometer of the time, (which we would now consider pretty crude) that many spectral lines split in a magnetic field into three (and more) spectral lines, one stays at the original position, the spacing of the other two depends linearly on the strength of the magnetic field. It is called the Zeeman effect. β€’ A good theory of the hydrogen atom needs to explain this !! 25
  • 26. Normal zeeman effect β€’ Normal Zeeman effect, which is actually not observed with modern spectrometers, historically β€œnormal” because of easy explanation β€’ Model the electron in the H atom as a small permanent magnet. β€’ Think of an electron as an orbiting circular current loop of I = dq / dt around some nucleus (that was not known to exist at that time). β€’ The current loop has a magnetic moment ΞΌ and the period T = 2Ο€r / v. (don’t confuse this ΞΌ with reduced mass) β€’ where L = mvr is the magnitude of the orbital β€’ angular momentum for a circular path. 26
  • 27. Normal zeeman effect β€’ When there is no magnetic field to align them, doesn’t have a effect on total energy. In an external magnetic field a dipole has a potential energy 27
  • 28. Normal zeeman Effect β€’ If there is a magnetic field in direction z, it will act on the magnetic moment, this brings in an (extra) potential energy term into the Hamiltonian operator β€’ So an external magnetic field should have an effect on atoms, spectral lines are β€œfingerprint” characteristics of atoms, in an external magnetic field, each spectral line should be splitting into three lines, distance between two extra lines proportional to the strength of the magnetic field, tested by experiment, observed, part of Nobel prize 28
  • 29. The Normal zeeman effect for Hydrogen β€’ The potential energy due to the external magnetic field is quantized due to the magnetic quantum number mβ„“. β€’ When a magnetic field is applied, the otherwise degenerate 2p level of atomic hydrogen is split into three different energy states with energy difference of Ξ”E = ΞΌBB Ξ”mβ„“. 29
  • 30. Conti… β€’ The larger B, the larger the splitting, if B is switched off suddenly, the three lines combine as if nothing ever happened, total intensity of lines remains constant in the splitting 30
  • 31. Conti… 𝑼 = 𝒆 πŸπ’Žπ’† 𝑳. 𝑩 = 𝒆𝑩 πŸπ’Žπ’† 𝑳𝒙 = β„πŽπ’π’Žπ’ β€’ What is really observed with good spectrometers: there are a lot more lines in atomic spectra when they are in a magnetic field ! So called Anomalous Zeeman effect, which is the only one observed with good spectrometers !!. 31
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