Physics

Radioactivity: an introduction

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ATOMIC STRUCTURE

Mass
Charge
Proton
1
+1
Neutron
1
0
Electron
≈ 1/2000
-1

The relative masses of protons, neutrons and electrons and their relative charges are as shown to the right

 

DISINTEGRATION OF UNSTABLE NUCLEI

If a nucleus contains too many or too few neutrons, it is unstable and eventually disintegrates into smaller fragments. The time it takes for different nuclei to suddenly disintegrate can vary from billions of years down to the tiniest fraction of a second.

Unstable nuclei can disintegrate in many ways. The two most common ways that unstable nuclei disintegrate are when

  1. the nucleus breaks in two: one small cluster of 2 protons and 2 neutrons (i.e. a helium nucleus) and another much larger cluster of nucleons.
  2. an electron is ejected from the nucleus.

Very short wavelength electromagnetic radiation is usually emitted (as a photon) almost immediately after the helium nucleus or electron is formed.

Both the helium nucleus and the electron fly off at high speed and the electromagnetic radiation travels at the speed of light, so all three of these can be thought of as rays. The first scientists investigatinf these rays didn't know what they were made of, so they called them by the following names:

The terms alpha rays, beta rays and gamma rays are still used for convenience today. Each individual Helium nucleus ejected is often referred to as an alpha particle. Each electron emitted from the nucleus is often referred to as a beta particle.

The emission of these radiations by unstable nuclei is referred to as radioactivity. The breaking up of unstable nuclei is called radioactive decay or radioactive disintegration.

 

A radioactive decay is associated with:

In a radioactive decay, the nucleus before the decay is called the parent nucleus. This decays into the daughter nucleus.

To be more specific:

Sometimes daughter nuclei are themselves unstable and so decay, forming part of a whole radioactive series of decays. For example, Uranium isotopes, which have a very long half-life, decay via a series of relatively short-lived radioisotopes to produce stable isotopes of lead as the end-products.

You should understand how to complete balanced nuclear equations.

Radioactive emissions are random (sometimes called spontaneous).

HISTORY

Radioactivity was discovered by Becquerel.

 

 

 

TYPES OF RADIOACTIVITY

Radioactivity is the emission of radiations resulting from the disintegration of atomic nuclei.

 

The three main types of radioactive radiation (and these were the ones investigated by the original discoverers) are:

Alpha (α) particles are positively charged and relatively heavy and slow
Beta (β) particles are negatively charged, light and fast
Gamma (γ) rays are electromagnetic radiation with a very short wavelength
An alpha particle is a small cluster of 2 protons + 2 neutrons  i.e.  it is a helium nucleus.
A beta particle is an electron, but unlike other electrons you have studied, it comes from inside the parent nucleus.
A gamma ray is a photon - like a light photon but with much higher energy.

These radiations all - to varying degrees - ionise matter that they travel through.


THE PENETRATING POWER OF THE RADIATIONS

Alpha particles are easy to stop, gamma rays are hard to stop, beta particles are in between


IONISATION

A neutral atom has a cloud of electrons round the nucleus. The total negative charge of this electron cloud exactly balances the positive charge of the nucleus.

An ion is:

When this happens to an atom/molecule or a group of atoms/molecules, we say that it has become ionised and that ionisation has occurred.

Ionizing radiation is radiation that can eject one or more electrons from a neutral atom, thereby creating two charged particles (an ion-pair): (1) the negatively charged electron and (2) the positively charged partially-stripped atom that is left behind. In order to be ionizing, the radiation must be able to deliver enough energy to a single atom to remove an electron.

Each of the three types of radiation - alpha, beta and gamma - cause atoms and molecules to lose electrons from the cloud of electrons round the nucleus, leaving behind positive ions.

Particles that ionise other atoms strongly have a low penetrating power, because they lose energy each time they ionise an atom.

Ionising radiation can be detected using:


PROPERTIES OF RADIOACTIVE RADIATIONS

ALPHA PARTICLES
BETA PARTICLES
GAMMA RAYS
Symbol:
Mass:
Charge:
Speed:
Ionising ability:
Penetrating power:
Stopped by:
α
4 - big, heavy
+2
slow
high
low
paper
Symbol:
Mass:
Charge:
Speed:
Ionising ability:
Penetrating power:
Stopped by:
β
1/2000 - small, light
-1
fast
medium
medium
thin aluminium
Symbol:
Mass:
Charge:
Speed:
Ionising ability:
Penetrating power
Stopped by:
γ
0
0
speed of light
weak
high
thick lead

 

Alpha particles are Helium nuclei, because they are made of 2 protons and 2 neutrons.

WHAT ARE THE RADIATIONS?

A beta particle is an electron. So it has a charge of -1, and a mass of just under1/2000th that of a proton.

 

Gamma rays are electromagnetic waves, like light and radio waves, but with a much shorter wavelength. Thus they have no charge. [ The only real difference between gamma rays and X-rays is that gamma rays originate from within the nucleus, whereas X-rays don't. ]

 

When an alpha particle passes an atom, it tends to attract the oppositely charged outer electrons away from the atom.

Alpha particles have a large charge (+2), so they strongly and easily ionise other atoms that they pass. Ionising atoms requires energy, so alpha particles lose energy and slow down rapidly and as they travel. This is one reason that alpha particles have such a low penetrating power.

HOW DOES RADIATION CAUSE IONISATION?

When a beta particle passes an atom, it tends to push (repel) outer electrons off the atom.

Beta particles affect atoms' outer electrons less than do beta particles, so cause less ionisation, lose less energy, and thus have a longer range - typically a few metres in air.

 

Gamma rays, like alpha and beta particles, ionise atoms and molecules - but much more weakly. They do not 'push or pull' outer electrons from atoms like the alphas and betas do: they give some of the electrons surrounding the nucleus some of their energy, causing the electron to be ejected from the atom.

Because they don't interact much with matter, gamma rays usually don't lose much energy as they travel. So they have a high penetrating power and a very long range. It takes a thick sheet of metal such as lead or concrete to reduce them significantly.


TYPES OF RADIOACTIVE DECAY

In alpha and beta decay, the parent nucleus decays to form a daughter nucleus.

ALPHA DECAY
BETA DECAY
Gamma rays

 

Alpha-decay occurs in very heavy elements, like Uranium. If their nucleus has too many protons (i.e. it is proton-rich), it is unstable. Such a nucleus can become more stable by emitting an alpha particle.

WHEN DOES RADIOACTIVITY OCCUR?

Beta decay occurs in nuclei, such as Strontium-90, that are unstable because they have too many neutrons in their nuclei (i.e. they are very neutron-rich). They become more stable by emitting a beta particle.

 

•  After a nucleus has emitted an alpha- or beta-particle, it may still have too much energy: we say it is in an "excited state".

•  It can get rid of this surplus energy by emitting a photon of very high frequency electromagnetic radiation, i.e. a gamma ray.

•  Gamma rays are given off by most alpha- and beta-emitters alongside the particles themselves. They are not emitted just on their own.

 

Alpha particles carry away some of the energy that was in the nucleus before it disintegrated.

WHAT CHANGES TAKE PLACE?

Beta particles (as with alpha particles) carry away some of the energy that was in the nucleus.

 

Gamma rays carry away usually much more nuclear energy than do alphas or betas.

Gamma rays are not only produced in radioactive decay. They arise from all sorts of high-energy nuclear reactions. e.g. in particle accelerators. They also form a small part of cosmic rays (which are mostly particles).

 

Alpha decay leaves a daughter nucleus that is of a different element to the parent one. When a nucleus emits an alpha-particle:

  • atomic mass decreases by 4.
  • atomic number decreases by 2

e.g. Americium-241 (an α-source used in smoke detectors), which has an atomic number of 95 and an atomic mass of 241, will decay to Neptunium-237 (which has an atomic number of 93 and an atomic mass of 237).

The equation would look like this:

241 Am
237 Np + α
   
95 93 

Now an alpha particle is the same as the nucleus of a Helium atom (2 protons and 2 neutrons). So it helps to balance equations if we write He instead of α as follows:

241 Am
237 Np + 4 He
     
95 93 2

NUCLEAR EQUATIONS FOR RADIOACTIVE DECAY

Beta decay also leaves a daughter nucleus that is of a different element to the parent one.

A beta particle is just an electron. What is an electron doing coming out of a nucleus? Under certain conditions, a neutron can decay, turning into a proton plus an electron. The proton remains in the nucleus, whilst the electron (the beta particle) flies off at high speed.

This means that when a nucleus emits a beta-particle:

  • atomic mass is unchanged
  • atomic number increases by 1

e.g. Strontium-90 undergoes beta decay and forms Yttrium-90

90 Sr
90 Y + β-
   
38 39

Because a beta particle is just an electron, we could write e instead of β in the equation as follows:

90 Sr
90 Y + 0 e
     
38 39 -1

The following is NOT on the GCSE syllabus:

  • Really there are two types of beta decay. The more common kind (and the one that is meant in the GCSE syllabus) is beta-minus decay, in which electrons are ejected from the nucleus. The less common kind is beta-plus decay, in which positrons are emitted.
  • An almost massless particle called an anti-neutrino is emitted alongside the beta-minus particle. In beta-plus decay, the corresponding particle is a neutrino.

 

Unlike alpha and beta decay, the nucleus retains the same composition - i.e. it is still the same element.

In gamma emission:

  • atomic number unchanged
  • atomic mass unchanged.

 

ISOTOPES and RADIOISOTOPES

You can think of different isotopes of an atom being different "versions" of that atom.

Consider a usual carbon atom. It has 6 protons and 6 neutrons - we call it carbon-12 because it has an mass number of 12 (6 protons plus 6 neutrons). If we add a neutron, it's still a carbon atom (carbon-13), but it's a different isotope of carbon. One useful isotope of carbon is carbon-14, which has 6 protons and 8 neutrons. This is the atom we look for when we're carbon dating an object.

So isotopes of an atom have the same number of protons, but a different number of neutrons.

Just because something is called an "isotope" doesn't necessarily mean it's radioactive. Those that are radioactive are called "radioactive isotopes" (or radioisotopes for short). Carbon-14 is a radioisotope, but carbon-12 is not.

[ The terms nuclides and radionuclides are often used instead of isotopes and radioisotopes. They are nearly always interchangeable. ]


ACTIVITY and HALF-LIFE

The half-life of a radioactive substance:

Furthermore:

Activity-Time graph

Half lives of some radioisotopes

Radioactive Parent
Stable Daughter
Half life

Rubidium-87

Strontium-87

49 billion years

Thorium-232

Lead-208

14 billion years

Uranium-238

Lead-206

5 billion years

Potassium-40

Argon- 40

1 billion years

Uranium-235

Lead-207

704 million years

Carbon-14

Nitrogen-14

5730 years

Americium-241   432 years
Cobalt-60   5 years
Iodine-131   1 week
Sodium-24   15 hours
Technetium-99m   6 hours
Bismuth-212   1 minute
Polonium-215   2 milliseconds

NUCLEAR FISSION

Fission means splitting in two.

Sometimes some nuclei do this of their own accord (this is called spontaneous fission). In situations such as a nuclear reactor, 'induced' fission occurs as a result of when large stable nuclei are bombarded with neutrons. when this hapens:

Nuclear reactors use fission to produce nuclear energy.

The energy released by an atom during radioactive disintegration or nuclear fission is very large compared to the energy released when a chemical bond is made between two atoms. Thus a nuclear power station produces much more energy than, say, a coal-fired power station.

The opposite of nuclear fission is nuclear 'fusion', where two nuclei are made to fuse together.


BACKGROUND RADIATION

There are radioactive substances all around us, from:

The radiation from all these sources is called background radiation. The level of background radiation is higher in some places than in others (depending, for example, on rock formations). eg because of (radioactive) radon gas released from rocks. Radon is also released from building materials made using rock.

Describe how to take background radioactivity into account when performing experiments.


DANGERS OF RADIOACTIVITY

Exposure to ionising radiation can be harmful.

When sources of radiation are inside the body:

When sources of radiation are outside the body:

Radiation sickness is illness induced by exposure to ionizing radiation, ranging in severity from nausea, vomiting, headache, and diarrhoea to loss of hair and teeth, reduction in red and white blood cell counts, extensive haemorrhaging, sterility, and death.

Describe the precautions that should be taken when handling radioactive materials. Explain how the effects of radiation depend on the energy and penetration of the emission as well as the amount of exposure.

( Workers who are at risk from radiation often wear a radiation badge to monitor the amount of radiation they have been exposed to over a period of time. The badge is a small packet containing photographic film. The more radiation a worker has been exposed to, the darker the film is when it has been developed. )

USES OF RADIOACTIVITY

Alpha radiation

The following aplications make use of alphas' low penetrating power. The source must have a half life long enough to lst the appliance (a few years).

Beta radiation

Gamma radiation

As regards nuclear weapons, there are strongly differing opinions as to how 'useful' nuclear weapons are to human welfare.

Apply knowledge of the different penetrating abilities to explain why different emissions are suited to each of the above applications.

Candidates should be able to evaluate the appropriateness of radioactive sources for particular uses, including as tracers, in terms of: