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A comprehensive overview of radioactivity, covering its types, detection methods, and measurement techniques. It delves into the processes of radioactive decay, including alpha and beta decay, and explores the differences between nuclear reactions and chemical reactions. The document also examines nuclear fission and fusion reactions, explaining their mechanisms and providing examples of nuclear equations. It concludes with a discussion of artificial radioactivity and the energy released in nuclear reactions, including the concept of binding energy.
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RADIOACTIVITY (Lecture2)
A nuclear reaction is different from a chemical reaction. In a chemical reaction, atoms of the reactants combine by a rearrangement of extra-nuclear electrons but the nuclei of the atoms remain unchanged. In a nuclear reaction, on the other hand, it is the nucleus of the atom which is involved. The number of protons or neutrons in the nucleus changes to form a new element. A study of the nuclear changes in atoms is termed Nuclear Chemistry. A number of elements such as uranium and radium are unstable. Their atomic nucleus breaks of its own accord to form a smaller atomic nucleus of another element. The protons and neutrons in the unstable nucleus regroup to give the new nucleus. This causes the release of excess particles and energy from the original nucleus, which we call radiation. The elements whose atomic nucleus emits radiation are said to be radioactive. The spontaneous breaking down of the unstable atoms is termed radioactive disintegration or radioactive decay. The disintegration or decay of unstable atoms accompanied by emission of radiation is called Radioactivity. TYPES OF RADIATIONS The radioactive radiations are of three types. These were sorted out by Rutherford (1902) by passing them between two oppositely charged plates. The one bending towards the negative plate carried positive charge and were named alpha (α) rays. Those bending towards the positive plate and carrying negative charge were called beta (β) rays. The third type of radiation, being uncharged, passed straight through the electric field and were named gamma (ϒ) rays. α, β and ϒ-rays could be easily detected as they cause luminescence on the zinc sulphide screen placed in their path.
Alpha (α), beta (β) and gamma (ϒ) rays differ from each other in nature and properties. There chief properties are : (a) Velocity; (b) Penetrating power; (c) Ionisation.
ALPHA RAYS
(1) Nature. They consist of streams of α-particles. By measurement of their e/ m, Rutherford showed that they have a mass of 4 a.m.u and charge of +2. They are helium nucleus and may be represented as (^2) 4 α or (^2) 4 He.
(2) Velocity. α-particles are ejected from radioactive nuclei with very high velocity, about one-tenth that of light.
(3) Penetrating power: Because of their charge and relatively large size, α- particles have very little power of penetration through matter. They are stopped by a sheet of paper, 0.01 mm thick aluminium foil or a few centimetres of air.
(4) Ionisation. They cause intense ionisation of a gas through which they pass. On account of their high velocity and attraction for electrons, α-particles break away electrons from gas molecules and convert them to positive ions.
BETA RAYS
(1) Nature. They are streams of β-particles emitted by the nucleus. From their deflection electric and magnetic fields, Becquerel showed that β-particles are identical with electrons. They have very small mass (1/1827 a.m.u) and charge of -1. A beta (β)- particle is symbolized as - 0 β or 0 -1e.
(2) Velocity. They travel about 10 times faster than α-particles. Their velocity is about the same as of light.
(3) Penetrating power. β-Particles are 100 times more penetrating in comparison to α- particles. This is so because they have higher velocity and negligible mass. β-particles can be stopped by about 1 cm thick sheet of aluminium or 1 m of air.
(4) Ionisation. The ionisation produced by β-particles in a gas is about one- hundredth of that of α-particles. Though the velocity of β-particles is higher but the mass being smaller, their kinetic energy is much less than α-particles. Hence they are poor ionisers.
GAMMA RAYS
(1) Nature. Unlike α and β-rays, they do not consist of particles of matter. ϒ- Rays are a form of electromagnetic radiation of shorter wavelength than X- rays. They could be thought of as high-energy photons released by the nucleus during α- or β-emissions. They have no mass or charge and may be symbolized as (^0) 0 γ. (2) Velocity. Like all forms of electromagnetic radiation, ϒ-rays travel with the velocity of light.
(3) Ionising power: Their ionising power is very weak in comparison to α and β- particles. A ϒ-photon displaces an electron of the gas molecule to yield a positive ion. Since the chances of photon-electron collisions are small, ϒ-rays are weak ionisers.
(3) Geiger-Muller Counter: This device is used for detecting and measuring the rate of emission of α- or β-particles. It consists of a cylindrical metal tube (cathode) and a central wire (anode). The tube is filled with argon gas at reduced pressure (0.1 atm). A potential difference of about 1000 volts is applied across the electrodes. When an α- or β-particle enters the tube through the mica window, it ionises the argon atoms along its path. The argon ions (Ar
) are drawn to the cathode and electrons to anode. Thus for a fraction of a second, a pulse of electrical current flows between the electrodes and completes the circuit around. Each electrical pulse marks the entry of one α- or β-particle into the tube and is recorded in an automatic counter. The number of such pulses registered by a radioactive material per minute, gives the intensity of its radioactivity.
(4) Scintillation Counter: Rutherford used a spinthariscope for the detection and counting of α-particles. The radioactive substance mounted on the tip of the wire emitted α-particles. Each particle on striking the zinc sulphide screen produced a flash of light. These flashes of light (scintillations) could be seen through the eye-piece. With this device it was possible to count α-particles from 50 to 200 per second.
A modern scintillation counter also works on the above principle and is widely used for the measurement of α- or β-particles. Instead of the zinc sulphide screen, a crystal of sodium iodide with a little thallium iodide is employed. The sample of the radioactive substance contained in a small vial, is placed in a ‘well’ cut into the crystal. The radiation from the sample hit the crystal wall and produce scintillations. These fall on a photoelectric cell which produces a pulse of electric current for each flash of light. This is recorded in a mechanical counter. Such a scintillation counter can measure radiation up to a million per second. (5) Film Badges: A film badge consists of a photographic film encased in a plastic holder. When exposed to radiation, they darken the grains of silver in photographic film. The film is developed and viewed under a powerful microscope. As α- or β-particles pass through the film, they leave a track of black particles. These particles can be counted. In this way the type of radiation and its intensity can be known. However, ϒ-radiation darken the photographic film uniformly. The amount of darkening tells the quantity of radiation. A film badge
is an important device to monitor the extent of exposure of persons working in the vicinity of radiation. The badge-film is developed periodically to see if any significant dose of radiation has been absorbed by the wearer.
TYPES OF RADIOACTIVE DECAY: According to the theory put forward by Rutherford and Soddy (1903), radioactivity is a nuclearproperty. The nucleus of a radioactive atom is unstable. It undergoes decay or disintegration by spontaneous emission of an α- or β-particle. This results in the change of proton-neutron composition of the nucleus to form a more stable nucleus. The original nucleus is called the parent nucleus and the product is called the daughter nucleus.
α-Decay When a radioactive nucleus decays by the emission of an α-particle (α- emission) from the nucleus, the process is termed α-decay. An alpha particle has four units of atomic mass and two units of positive charge. If Z be the atomic number and M the atomic mass of the parent nucleus, the daughter nucleus will have; atomic mass = M – 4 and atomic number = Z – 2
Thus an α-emission reduces the atomic mass by 4 and atomic number by 2. For example, Radium decays by α-emission to form a new element Radon as in:
β-Decay When a radioactive nucleus decays by β-particle emission (β-emission), it is called β-decay. A free β-particle or electron does not exist as such in the nucleus. It is produced by the conversion of a neutron to a proton at the moment of emission. Neutron p + e This results in the increase of one positive charge on the nucleus. The loss of a β-particle from the nucleus does not alter its atomic mass. For a parent nucleus with atomic mass M and atomic number Z, the daughter nucleus will have atomic mass = M and atomic number = Z + 1 Thus a β-emission increases the atomic number by 1 with no change in atomic mass. An example of β-decay is the conversion of lead-214 to bismuth-214,
8 – 12 = -b
-4 = -b b = 4
Thus the number of α- particles emitted = 6 and the number of β- particles emitted = 4.
Example 2: is a β-emitter and is an α-emitter. What will be the atomic masses and atomic numbers of daughter elements of these radioactive elements? Predict the position of daughter elements in the periodic table.
Solution
underdoes β-decay i.e
Comparing the atomic masses, we have:
210 = 0 + b b = 210
Comparing the atomic numbers, we are going to get:
82 = -1 + a a = 82 + 1 a = 83
Thus the daughter element will have the same atomic mass 210 and its atomic number will be 83. It will occupy one position right to the parent element.
(b) undergoes α-decay i.e
Comparing the atomic masses, we get;
236 = 4 + b
b = 236 – 4 b = 232
and comparing the atomic number, we get
88 = 2 + a a = 88 – 2 a = 86
Thus the daughter element will have atomic mass 232 and its atomic number will be 86. It will occupy two positions to the left of the parent element.
RADIOACTIVE DISINTEGRATION SERIES
A radioactive element disintegrates by the emission of an α- or β- particle from the nucleus to form a new ‘daughter element’. This again disintegrates to give another ‘daughter element’. The process of disintegration and formation of a new element continues till a non radioactive stable element formed as the product. The whole series of elements starting with the parent radioactive element to the stable end-product is called a Radioactive Disintegration Series. Sometime, it is referred to as a Radioactive Decay Series or simply Radioactive Series. All the natural radioactive elements belong to one of the three series : (1) The Uranium Series (2) The Thorium Series (3) The Actinium Series
The Uranium Series: It commences with the parent element uranium-238 and terminates with the stable element lead-206. It derives its name from uranium-238 which is the prominent member of the series and has the longest half-life.
The Thorium Series: It begins with the parent element thorium 232 and ends with lead-208 which is stable. This series gets its name from the prominent member thorium-232.
The Actinium Series: It starts with the radioactive element uranium-235. The end-product is the stable element lead-207. This series derives its name from the prominent member actinium-227.
RATE OF RADIOACTIVE DECAY: The decay of a radioactive isotope takes place by disintegration of the atomic nucleus. It is not influenced by any external conditions. Therefore the rate of decay is characteristic of an isotope and depends only on the number of atoms present. If N be the number of
The activity of a radioactive sample is usually determined experimentally with the help of a Geiger –muller counter CALCULATIONS OF HALF-LIFE From equation (1) we can write:
Where x is a constant
No is the number of atom at time t=0, X=ln No
Substituting the value of X in (3)
2.303log ……………………………………………………..4
2.303log
The value of decay constant can be found experimentally by finding the number of disintegrations per second with the help of Geiger Muller counter. Hence, half-life of the isotope concerned can be calculated by using equation 5.
Example 1. Calculate the half-life of radium-226 if 1g of it emits 3.7 × 10 10 alpha particles per second.
Solution
Rate of decay = Rate of emission of α-particles; Recall that;
N = 3.7 x 10 10 per second The number of atoms of radium present (N) in 1g of sample =
From equation (5) stated earlier ,
Substituting the value of and N in equation (1) above;
Example 2: Calculate the disintegration constant of cobalt 60 if its half-life to produce Nickel – 60 is 5.2 years.
Solution
CALCULATIONS OF SAMPLE LEFT AFTER TIME T
It follows from equation stated earlier that:
Knowing the value of , the ratio of N 0 /N can be calculated. If the amount of the sample present to start with is given, the amount left after lapse of time t can be calculated.
Example 4: Cobalt-60 disintegrates to give nickel-60. Calculate the fraction and the percentage of the sample that remains after 15 years. The disintegration constant of cobalt-60 is 0.13 yr -1
SOLUTION
The fraction remaining is the amount at time t divided by the initial amount.
Hence the fraction remaining after 15 years is 0.14 or 14 per cent of that present originally. Example 5: How much time would it take for a sample of cobalt-60 to disintegrate to the extent that only 2.0 per cent remains? The disintegration
constant is 0.13 yr
From the equation above:
t = 30 years.
TUTORIAL QUESTIONS
is broken or fissioned into two or more fragments. This is accomplished by bombarding an atom by alpha particles ( ), neutrons ( ), protons ( ), deutrons ( ), etc. All the positively charged particles are accelerated to high kinetic energies by a device such as a cyclotron. This does not apply to neutrons which are electrically neutral. The projectile enters the nucleus and produces an unstable ‘compound nucleus’. It decomposes instantaneously to give the products. NUCLEAR FUSION REACTIONS: These reactions take place by combination or fusion of two small nuclei into a larger nucleus. At extremely high temperatures the kinetic energy of these nuclei overweighs the electrical repulsions between them. Thus they coalesce to give an unstable mass which decomposes to give a stable large nucleus and a small particle as proton, neutron, positron, etc. For example, Two hydrogen nuclei,( ) , fused to produce a deuterium nucleus ( ).
NUCLEAR EQUATIONS: Similar to a chemical reaction, nuclear reactions can be represented by equations. These equations involving the nuclei of the reactants and products are called nuclear equations. The nuclear reactions occur by redistribution of protons and neutrons present in the reactants so as to form the products. Thus the total number of protons and neutrons in the reactants and products is the same. Obviously, the sum of the mass numbers and atomic numbers on the two sides of the equation must be equal. If the mass numbers and atomic numbers of all but one of the atoms or particles in a nuclear reaction are known, the unknown particle can be identified. How to write a nuclear equation
(a) Disintegration of radium-236 by emission of an alpha particle ( ),
Mass Number; REACTANT = 236 PRODUCTS = 232 + 4 = 236 Atomic Number REACTANT = 88 PRODUCTS = 86 + 2 = 88
b) Disintegration of phosphorus-32 by emission of a beta particle ( ),
Mass Number; REACTANT = 32 PRODUCTS = 0 + 32 = 32 Atomic Number REACTANT = 15 PRODUCTS = -1 + 16 = 15
(c) Fission of Argon-40 by bombardment with a proton
Mass Number; REACTANT = 40 + 1=41 PRODUCTS = 40 + 1 =41 Atomic Number REACTANT = 18 + 1 =19 PRODUCTS = 19 + 0 = 19
(d) Fission of uranium-235 by absorption of a neutron ( )
Mass Number; REACTANT = 235+1=236 PRODUCTS = 141+92+3=236 Atomic Number REACTANT = 92+0=92 PRODUCTS = 56+36+0=92.
Exercise: Complete the nuclear equation and identify the missing element.
ARTIFICIAL RADIOACTIVITY: Many stable nuclei when bombarded with high speed particles produce unstable nuclei that are radioactive. The radioactivity produced in this manner by artificial means is known as artificial radioactivity.
ENERGY RELEASED IN NUCLEAR REACTIONS: According to Albert Einstein, mass can be converted into energy and vice versa. His famous equation relating mass and energy is:
……………………………………….(1)
where E = energy ; m = mass and c = velocity of light. In nuclear reactions, a
= 1.2 x 10