structure of nucleus

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Structure of Nucleus Mahesh Shetti, Wilson College USPH102 unit 1.1 1 All images used from various sources mentioned are purely for educational purpose.

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Page 1: Structure of Nucleus

Structure of Nucleus

Mahesh Shetti,

Wilson College

USPH102 unit 1.1 1

All images used from various sources mentioned are purely for educational purpose.

Page 2: Structure of Nucleus

Size Scale of Atom and Nucleus

All pictures in this section are taken from the book Powers of

10 by Phillip and Philys Morris

USPH102 unit 1.1 2

Page 3: Structure of Nucleus

100 meters

1 meter

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Page 4: Structure of Nucleus

10-1 meters

USPH102 unit 1.1

0.1 meter

10 cm

4

Page 5: Structure of Nucleus

10-5 meters

0.01 mm

10 microns

The size scale of a cell

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Page 6: Structure of Nucleus

10-6 meters

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1

Size scale of blood capillary, bacteria

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Page 7: Structure of Nucleus

10-7 meters

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0.1

Size scale of chromosomes, various cell organelles

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10-8 meters

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0.01

Size scale of DNA

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Page 9: Structure of Nucleus

10-9 meters

USPH102 unit 1.1

1 nm

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Page 10: Structure of Nucleus

10-10 meters

USPH102 unit 1.1

Size scale of atoms

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Page 11: Structure of Nucleus

10-12 meters

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0.01 Å

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Page 12: Structure of Nucleus

10-13 meters

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0.001Å

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Page 13: Structure of Nucleus

10-14 meters

USPH102 unit 1.1

10 fm

Size scale of atomic nucleus

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Page 14: Structure of Nucleus

10-15 meters

USPH102 unit 1.1

1 fm

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Page 15: Structure of Nucleus

Composition of Nuclei

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Page 16: Structure of Nucleus

Rutherford’s

scattering (1911)

Large number of alpha particles did not get scattered.

Some got scattered through very large angles.

This was as if bullets fired on a paper sheet bounced back!!

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Page 17: Structure of Nucleus

Atomic Structure

10-10 meters

10-14m

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Page 18: Structure of Nucleus

Nuclear Atom Concept

USPH102 unit 1.1

Rutherford’s experimental analysis showed:

Scattering happened due to Coulomb repulsion between

positively charge alpha particles and positively charged atom.

Coulomb interaction was only beyond 10–15 to 10–14 m.

This implied all the positive charge was located inside the

region of 10–14m.

Electrons already discovered were carrying negative

charge, and were quite light.

Hence all the mass of the atom also might be lying inside

that small region called nucleus.

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Page 19: Structure of Nucleus

What are isotopes?

USPH102 unit 1.1 19

Ions passed in electric and magnetic field, deviate according to their charge and mass.

This way it is possible to find whether same element has different mass nuclei.

Such nuclei having same atomic number (same element) but different masses are called isotopes.

Page 20: Structure of Nucleus

Some commonly known isotopes

USPH102 unit 1.1 20

Helium

3He (1.4ppm), 4He (remaining)

Carbon

12C (98.9%), 13C(1.07%)

14C (radioactive)

Oxygen

16O (99.75%), 17O (0.04%)

18O (0.2%)

Chlorine

35Cl (76%), 37Cl (24%)

Potassium

39K(93.3%), 40K(0.01%), 41K(6.7%)

Nickel

58Ni (68%), 60Ni (26%),

62Ni (3.6%), 64Ni (0.92%)

Copper

63Cu (69%), 65Cu (31%)

Bromine

79Br (50.7%), 81Br (49.3%)

Lead

204Pb (1.4%), 206Pb (24.1%),

207Pb (22.1%), 208Pb (52.4%)

Uranium

234U (0.0055%), 235U (0.72%)

238U (99.27%)

Page 21: Structure of Nucleus

How do we know that nucleus is made up of

even smaller particles?

USPH102 unit 1.1

Clue 1: Radioactivity

Clue 2: All electrons are similar independent of atoms as

known by cathode ray properties, then all positive

particles also may be similar

Clue 3: Elements have different isotopes and they were

having integer masses

Clue 4: Atomic number (i.e. their position in the periodic

table) and not atomic mass decided the spectral lines of

heavier elements. (Moseley’s work using X-ray diffraction)

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Page 22: Structure of Nucleus

Nucleus of atom

USPH102 unit 1.1 22

Nucleus is made up of

two kinds of particles.

Protons are positively

charged.

Charge on proton is same

as that on electrons.

Neutrons are neutral.

Neutrons were discovered

in 1932, long after atomic

model was developed.

10–15m

Page 23: Structure of Nucleus

How nuclear particles are bound

together?

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Page 24: Structure of Nucleus

Mass defect

USPH102 unit 1.1 24

The mass of a higher nucleus is

observed to be smaller than the

combined mass of protons and

neutrons (in lighter nuclei).

This is called mass defect.

The loss of mass is given out as

energy of fusion. This can be

calculated using mass-energy

relation: E = m c2

The energy is released when

protons and neutrons are bound.

When we provide this energy

(called binding energy) we can

separate protons and neutrons

again.

Page 25: Structure of Nucleus

Mass defect and binding energy calculation

USPH102 unit 1.1

Consider U-235 isotope.

This isotope has mass = 235.04393 amu

There are 92 protons and 143 neutrons.

Each proton has mass = 1.00728 amu

Each neutron has mass = 1.00867 amu

M = 92(1.00728 amu)+143(1.00867 amu))

– 235.04393 amu

M = 1.86564 amu

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Page 26: Structure of Nucleus

USPH102 unit 1.1 26

M = 1.86564 amu / 6.02214x1026 amu/kg

= 3.09797x10–27 kg

E = Mc2

= 3.09797 x 10–27 kg x (2.99792458 x 108 m/s)2

E = 2.7843 x 10-10 J

= 2.7843 x 10-10 /1.602 × 10-19 eV = 1.738GeV

E = 2.7843 x 10-10 J x 6.02 x1023 /kmole

= 1.6762 x 1011 kJ/kmole

This is the binding energy for Uranium nucleus.

Binding energy per nucleon = 1.738/235 GeV/nucleon

= 7.40 MeV/nucleon

Mass defect and binding energy calculation

Page 27: Structure of Nucleus

Binding energy for

different nuclei

• Iron-56 is the most stable

nucleus.

• Fission of heavier nucleus

is exothermic (can emit

energy)

• Fusion of lighter nucleus is

exothermic

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Page 28: Structure of Nucleus

Magic Numbers for nucleus

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Page 29: Structure of Nucleus

Relative abundances as function of Z

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Page 30: Structure of Nucleus

Relative abundance as a function of N

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Page 31: Structure of Nucleus

Magic numbers

More positive binding energy implies more stable nucleus.

By adding extra nucleon, if binding energy is reducing or becoming negative, it means new configuration is less stable.

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Page 32: Structure of Nucleus

Nuclear Stability

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In high Z region, larger

number of neutrons are

needed to make the nucleus

stable. Hence stability curve

deviates from N=Z line.

If number of neutrons are

larger than needed,

(isotopes above stability curve)

such nuclei may become stable

by emitting beta radiations

where neutron is converted to

proton.

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Page 33: Structure of Nucleus

USPH102 unit 1.1 33

If neutrons are less than needed, such nuclei may become stable by emitting positron where proton is converted to neutron.

When both protons and neutrons are very large, the nucleus emits alpha particle or may undergo fission to become smaller nuclei.

In low Z region, higher neutron nuclei can become stable by emitting directly neutron and low neutron nuclei may emit protons.

Nuclear Stability

Page 34: Structure of Nucleus

Ideas in Modern Physics

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Page 35: Structure of Nucleus

de Broglie’s Matter wave (1925)

USPH102 unit 1.1 35

If light can exist as particle and wave both,

even matter should exist with “dual nature”.

What is the difference between

particle representation and wave representation?

Why there is a dilemma?

Page 36: Structure of Nucleus

USPH102 unit 1.1 36

Addition of 3 terms

= 0.5

Construction of matter wave

Page 37: Structure of Nucleus

USPH102 unit 1.1 37

Addition of 100 terms

= 0.02

Construction of matter wave

Page 38: Structure of Nucleus

USPH102 unit 1.1 38

Addition of 100 terms

= 0.1

Construction of matter wave

Page 39: Structure of Nucleus

USPH102 unit 1.1 39

Addition of 100 terms

= 0.5

Construction of matter wave

Page 40: Structure of Nucleus

As the frequency difference increases the position

function narrows.

With smaller range of frequencies the position

function spreads.

But,

Frequency Momentum p = h/

i.e. p x

This is Heisenberg’s Uncertainty Principle

40 Foundation Course in Astronomy and

Astrophysics

Page 41: Structure of Nucleus

Heisenberg’s uncertainty principle (1924)

USPH102 unit 1.1 41

The uncertainty is not due to our inability to measure these quantities precisely. The nature itself does not allow that to happen.

It does not say position cannot be measured precisely.

It says both position and momentum in the same direction cannot be measured precisely simultaneously.

Page 42: Structure of Nucleus

Spontaneous Emissions

USPH102 unit 1.1 42

Why does electron come to lower energy state?

What causes spontaneous emission?

Without any external force/interaction, why does electron

change its state?

E2

E1

E2

E1

E = h

Excited atom

atom jumped to lower state

Emitted photon

After some

arbitrary

time interval

Page 43: Structure of Nucleus

Hawking Radiation

Black holes are black

bodies.

Black bodies emit

radiations in all

wavelengths.

Hence, black holes must

emit radiations.

But, how?

Uncertainty principle

makes it possible.

43 USPH102 unit 1.1

Page 44: Structure of Nucleus

Relativistic formulae

USPH102 unit 1.1 44

Momentum

Mass-Energy Relation

Energy Momentum Relation

Kinetic Energy

Page 45: Structure of Nucleus

Why electrons cannot be there

inside nucleus?

Beta emissions suggested there can be electrons inside the

nucleus. But this theory has other problems:

USPH102 unit 1.1 45

Page 46: Structure of Nucleus

Why electrons cannot be inside nucleus

Problem #1

USPH102 unit 1.1

Beta emissions have energies less than 10MeV.

This energy is higher than rest mass energy of electrons 0.511

MeV.

Consider Uncertainty principle:

= h/2 = 1.055 x 10–34 Js

If electron is confined inside nucleus then x 10–15m

Hence p 5.3 x 10–20 kg-m/s

Relativistic Energy: = 1.59 x 10–11 J

Kinetic energy: = 1.58 x 10–11 J 100MeV

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Page 47: Structure of Nucleus

USPH102 unit 1.1 47

Proton and neutron both have ½ spin.

Nitrogen has mass number 14.

Hence it must have 14 protons and 7 electrons

inside the nucleus.

Hence total odd number of particles should

give odd multiple of ½ spin.

Nitrogen nucleus was shown to have +1 spin.

Why electrons cannot be inside nucleus

Problem #2

Page 48: Structure of Nucleus

Historical developments to

understand nature of nuclear force

USPH102 unit 1.1 48

Page 49: Structure of Nucleus

Rutherford’s

scattering (1911)

Large number of alpha particles did not get scattered.

Some got scattered through very large angles.

This was as if bullets fired on a paper sheet bounced back!!

USPH102 unit 1.1 49

Page 50: Structure of Nucleus

Analysis of Rutherford scattering

USPH102 unit 1.1 50

Rutherford analysed the profile of scattered alpha

particles using Coulomb repulsion.

Particles must be experiencing Coulomb repulsion at a

greater distance than the nuclear size.

When particles approach minimum distance from the

nucleus, their kinetic energy is all converted to

electrostatic potential energy.

2e is charge on alpha particle, Ze is charge on nucleus, R

is distance of closest approach.

Page 51: Structure of Nucleus

Nuclear size

USPH102 unit 1.1 51

Maximum kinetic energy of particles is 7.7MeV

Hence

Substitute:

Z = 79 (for gold foil atoms)

(K.E.)initial = 7.7 MeV = 7.7 x 106 x 1.602 x 10–19 J

1/4 0 = 9 x 109 SI units

R = 3.0 x 10–14 m

Hence size of nucleus is smaller than this.

Page 52: Structure of Nucleus

Is classical mechanics application correct?

USPH102 unit 1.1 52

De Broglie wavelength of 7.7MeV alpha particle is

Hence, = 5 x 10–15 m

Since nucleus was larger than de Broglie wavelength the

classical physics analysis worked in the first place to

determine the approximate size of nucleus.

Page 53: Structure of Nucleus

Nuclear Force

USPH102 unit 1.1 53

Page 54: Structure of Nucleus

Nucleus consists of

Protons and

Neutrons

Strong interaction force is

responsible to hold protons

together inside the nucleus

of atom!

Protons and neutrons are

made of even finer particles

called quarks and strong

interaction is due to

interaction between them.

These quarks are never

found free in nature!

USPH102 unit 1.1 54

Image source: https://in.pinterest.com/

Page 55: Structure of Nucleus

Concept behind Yukawa theory of mesons

USPH102 unit 1.1 55

Electromagnetic interaction

was associated with photons.

The repulsion between two

protons due to their positive

charges can be explained by

the exchange of photons

between the protons.

Using the similar logic

Hideki Yukawa proposed

(in 1935) a mediating

particle for strong force

between nucleons.

Virtual photon

emitted

e– e–

e– e–

force

Continuous

exchange of virtual

photons

e– e–

force force

Page 56: Structure of Nucleus

Yukawa theory of mesons

USPH102 unit 1.1 56

Using relativistic quantum

mechanics, he calculated what

would be the mass of such

particle.

According to his calculations, such

particle would be 300 times

heavier than electron (but lighter

than proton).

In 1947, the British physicist

Cecil Powell and his colleagues

showed that there were two types

of middle mass particles –

Yukawa’s meson and another

lighter lepton (now called muon).

Yukawa got Nobel prize in 1949,

Powell got Nobel in 1950.

Image source:

https://www.britannica.com/biography/Yukawa-Hideki

Page 57: Structure of Nucleus

Some parallel developments

USPH102 unit 1.1

In 1936, Carl Anderson and his

student Seth Neddermeyer noticed a

negatively charged particle with mass

207 times that of electron. Other

observers also started detecting

similar mass particles, but there were

discrepancies in mass of particles.

In 1937 Marietta Blau and her former

student Wambacher published in

Nature about their success in creating

emulsions with long exposure times

that could be used to record the

tracks of fast moving protons. They

recorded disintegration of heavy

nuclei by cosmic particles.

C. V. Raman was so excited that he

took some of the plates to India.

57

Image Source:

https://www.researchgate.net/publication/258706384_Marietta_B

lau_in_the_history_of_cosmic_rays

Page 58: Structure of Nucleus

Photographic plates exposed to cosmic ray particles

These historical plates have not just recorded the particles coming from far off galaxies, they also paved the way

to understand what goes down inside the atom! Plates from Miss Blau’s work.

USPH102 unit 1.1 58

https://scienceblog.at/marietta-blau-entwicklung-bahnbrechender-methoden-auf-dem-gebiet-der-teilchenphysik#.X2hclWgzb_U

Page 59: Structure of Nucleus

Indian Contribution

USPH102 unit 1.1

In 1938 Homi Bhabha pointed out that Yukawa meson

created in the Earth’s atmosphere would quickly decay

via beta radiation and hence would never live long

enough to get detected in lower atmosphere.

In India, D. M. Bose and his student Bibha Chowdhuri

designed a new way to identify atmospheric particles

based on the photographic method. They published

four papers (From 1941 to 1946) in Nature!

They reported observations of a particle that could be

Yukawa meson, but due to World War II, they could not

acquire better emulsions and had to discontinue their

work.

Cecil Powell and his colleagues built on their work and

observed Yukawa mesons to win Nobel Prize.

Yukawa mesons were present only in upper

atmosphere, as predicted by Bhabha.

59

Image source:

https://en.wikipedia.org/wiki/Bibha

_Chowdhuri

Page 60: Structure of Nucleus

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Page 61: Structure of Nucleus

Discovery of neutron

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Bothe and Becker bombarded beryllium with alpha particles from a radioactive source.

It produced neutral radiation which was penetrating but non-ionizing. They thought it could be gamma ray.

Curie and Joliot showed that when you bombarded a paraffin target with this radiation, it ejected protons with energy about 5.3 MeV.

Analyzing collission equations showed that it cannot be gamma ray.

Chadwick bombarded boron with alpha particles and analyze the interaction of the neutral particles with nitrogen. By analyzing the collision equations, he determined the mass of neutral particle close to that of proton.

Page 62: Structure of Nucleus

Fundamental Forces, Elementary

particles and force mediators

USPH102 unit 1.1 62

Page 63: Structure of Nucleus

Fundamental Forces

USPH102 unit 1.1

Gravitational force

Between any two particles that have mass

Electromagnetic force

Between any two particles having charge

Strong force

It is short range only within 10–14m

Between nucleons called hadrons e.g. proton, neutron

Weak force

It is short range only within 10–14m

It is responsible for beta decay process (that converts proton

to neutrons and neutrons to protons)

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Page 64: Structure of Nucleus

Quarks: fundamental particles that are never found independent

USPH102 unit 1.1 64

1st Generation 2nd Generation 3rd Generation

mass

charge

spin

Page 65: Structure of Nucleus

Lepton

USPH102 unit 1.1 65

Electron belongs to family of

fundamental particles called

leptons.

Neutrinos are neutral while

electron, muon and tauon

are with charge –1.

Leptons do not experience

strong interaction.

They experience weak

interaction.

Charged leptons also

experience electromagnetic

interactions.

Generation

Page 66: Structure of Nucleus

Particles made up of quarks (hadrons)

Baryons Mesons

USPH102 unit 1.1 66

They are hadrons made of 3 quarks

proton, neutron, particle

Being hadrons they experience strong interaction

They are controlled by Pauli exclusion principle. i.e. they come under category of fermions.

They are hadrons made of quark and anti-quark

pions, kaons, rho meson

Being hadrons they experience strong interaction

They are not controlled by Pauli exclusion principle. i.e. they come under category of bosons.

Page 67: Structure of Nucleus

Protons and Neutrons are baryons

Proton Neutron

USPH102 unit 1.1 67

Page 68: Structure of Nucleus

pion is a meson

Neutral pion is made of d

quark and anti-quark

USPH102 unit 1.1 68

Image source:

https://readingfeynman.org/tag/neutron-proton-interaction/

Page 69: Structure of Nucleus

K meson (Kaon)

USPH102 unit 1.1 69

Page 70: Structure of Nucleus

Force mediators

USPH102 unit 1.1 70

The fundamental forces act on different particles via force

mediating particles called carrier bosons.

Strong interaction between quarks happen via gluons.

Weak interaction happens via W± and Z0 bosons.

Electromagnetic interactions happen with photons.

The range of force depends on rest mass of force

carriers.

Photons have zero rest mass and range of electromagnetic

interaction is infinite.

W± and Z0 bosons are heavy and their range is limited.

Page 71: Structure of Nucleus

Fundamental particle

USPH102 unit 1.1 71

Page 72: Structure of Nucleus

Fermions and Bosons

USPH102 unit 1.1 72

All particles are classified into two categories – Fermions and Bosons based on their spin moment.

Fermions have half integral spin

They obey Fermi-Dirac statistics

They are restricted by Pauli exclusion principle

Examples – proton, neutron, electron, muon,…

Bosons have integral spin

They obey Bose-Einstein statistics

They are not restricted by Pauli exclusion principle

Examples – photon, alpha particle, pion,…

Depending on which and how many elementary particles constitute given particle, its spin status is decided.

Page 73: Structure of Nucleus

References and extra reading

USPH102 unit 1.1

Powers of 10 - Phillip and Philys Morris

Galileo’s Finger – Peter Atkins

Clues to the Cosmos – Shohini Ghose

Concepts of Modern Physics – Arthur Beiser

Nuclear Physics – Irving Kaplan

Principle of Modern Physics – R. P. Leighton

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