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NUCLEUS The central core of the atom which contains all the positive charge and most of its mass.It consists of Property Protons Neutrons Nature of Charge Positive Neutral Value of charge + 1.6 × 10 19 C 0 Mass 1.6726 × 10 27 kg = 1.007825 a.m.u 1.6750 × 10 27 kg = 1.008665 a.m.u. These two constituents of a nucleus (protons and neutrons) are called nucleons. !! Hydrogen nucleus consists of a single proton alone, the nuclei of other elements consist of both neutrons and protons. The different types of nuclei are often called nuclides. Note. Since neutron is a neutral particle, it has high penetrating power and very low ionising power. Further, electric and magnetic fields have no affect on it. ATOMIC NUMBER AND MASS NUMBER (i) Atomic number (Z): The number of protons in a nucleus is called the atomic number. In a neutral atom, the number of electrons is equal to the atomic number Z. (ii) Mass number (A): The total number of nucleons (protons plus neutrons) is called mass number. This name is used since the mass of a nucleus is very closely A times the mass of one nucleon. Clearly, neutron number, N = A Z Nuclear notation (Nuclide) : To specify a given nucleus, we need give only A and Z. A nucleus is represented by a special symbol which takes the form: z X A Here X is the chemical symbol for the element. PROPERTIES OF ATOMIC NUCLEUS (i) Size of nucleus: Radius R of the nucleus is given by; 3 / 1 0 A R R here, R o =1.2 x 10 15 m (ii) Nuclear density: EINSTEIN'S MASS-ENERGY RELATION Mass and energy are interconvertible. E = m c 2 where c = velocity of light ( = 3 × 10 8 ms 1 )

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  • NUCLEUS

    The central core of the atom which contains all the positive charge and most of its mass.It consists of

    Property Protons Neutrons

    Nature of Charge Positive Neutral

    Value of charge + 1.6 1019 C 0

    Mass 1.6726 1027 kg = 1.007825

    a.m.u

    1.6750 1027 kg = 1.008665

    a.m.u.

    These two constituents of a nucleus (protons and neutrons) are called nucleons.

    !! Hydrogen nucleus consists of a single proton alone, the nuclei of other elements consist of both neutrons

    and protons. The different types of nuclei are often called nuclides.

    Note. Since neutron is a neutral particle, it has high penetrating power and very low ionising power.

    Further, electric and magnetic fields have no affect on it.

    ATOMIC NUMBER AND MASS NUMBER

    (i) Atomic number (Z): The number of protons in a nucleus is called the atomic number.

    In a neutral atom, the number of electrons is equal to the atomic number Z.

    (ii) Mass number (A): The total number of nucleons (protons plus neutrons) is called mass number. This

    name is used since the mass of a nucleus is very closely A times the mass of one nucleon.

    Clearly, neutron number, N = A Z

    Nuclear notation (Nuclide) : To specify a given nucleus, we need give only A and Z. A nucleus is

    represented by a special symbol which takes the form: z X A

    Here X is the chemical symbol for the element.

    PROPERTIES OF ATOMIC NUCLEUS

    (i) Size of nucleus: Radius R of the nucleus is given by;

    3/1

    0 ARR here, Ro =1.2 x 10 15 m

    (ii) Nuclear density:

    EINSTEIN'S MASS-ENERGY RELATION

    Mass and energy are interconvertible. E = m c2

    where c = velocity of light ( = 3 108 ms1)

  • ISOTOPES ISOBARS ISOTONES

    The nuclei that have the same

    number of protons (Z) but

    different number of neutrons

    (different A) are called isotopes.

    The atoms of different elements

    which have the same mass

    number A but differ in their

    atomic number Z are called

    isobars.

    The nuclei of isobars have

    different number of protons (Z)

    and different number of neutrons

    (A Z).

    The nuclides which contain the

    same number of neutrons are

    called isotones.

    6C11, 6C

    12, 6C13, 6C14, 6C

    15 and 6C16

    are isotopes of carbon

    11Na23 and 12Mg

    23 are the isobars.

    15P31 and 16S

    32 are the isotones

    because the nuclides of both

    contain the same (i.e. 16)

    neutrons.

    NUCLEAR FORCE

    The strong forces of attraction which firmly hold the nucleons in

    the nucleus are known as nuclear forces.

    Properties of nuclear forces:

    (i) They are charge independent i.e. they are the same between p

    and n or between p and p or between n and n.

    (ii) They are short-range forces upto 10-15m.

    (iv) They have saturation character i.e. they abruptly become zero

    as the inter-nucleon distance is increased to a certain value (about 1014 m). Therefore, nuclear forces do not

    increase with the increase in the number of nucleons.

    (v) They are strongest i.e. their magnitude is so high that a huge energy is required to divide a nucleus into

    its constituents.

    MASS DEFECT

    The difference between the actual mass of the nucleus and the sum of masses of the constituent nucleons is

    called mass defect i.e

    Mass defect, m =[zMp + (AZ) Mn ] M where M = actual mass of the nucleus and A = mass number

  • NUCLEAR BINDING ENERGY

    It is the energy with which the nucleons are held together within the nucleus.

    It is measured by the total energy required to liberate all the nucleons from the nucleus (i.e. to

    disintegrate the nucleus completely into its constituent particles) .

    Eb = 2

    !! m should be in kg. If it is in amu then use 1 amu = 931.5MeV

    ORIGIN

    A nucleus is formed by coming together of the constituent nucleons. It has been observed experimentally

    that the mass of the nucleus is always less than the sum of the masses of its constituent nucleons. This

    energy liberated contribute the decrease in mass (mass defect)

    BINDING ENERGY PER NUCLEON

    Ebn = Eb / A=2/A

    Greater the binding energy per nucleon, the greater is the stability of the nucleus

    BINDING ENERGY CURVE

    In heavy nuclei number of proton is

    large therefore due to large repulsion

    binding energy decreases.

    Following are the characteristics of

    the curve:

    (i) The curve rises as A (mass number)

    increases and reaches a value of about 8

    MeV per nucleon above A ~ 15.

    (ii) The nuclei with A ~ 60 have the

    greatest binding energy per nucleon and

    are also the most stable nuclei.

    (iii) The very small and very large nuclei have less binding energy per nucleon indicating that these nuclei

    are held less tightly than those in the middle of the periodic table.

    (iv) Except for a few light nuclei, the average binding energy per nucleon is about the same (i.e. about 8

    MeV) for all nuclei. This proves the saturation character of the nuclear forces.

    (v) The binding energy curve is used to analyze nuclear processes such as fission and fusion

  • (a) For fission:

    From curve it is clear that B.E. / nucleon for a heavy nucleus is lower therefore it is unstable but when it

    breaks down , then it forms two medium weight nuclei (lie in the middle portion on curve) which have

    more B.E. / nucleon than heavy one and hence more stable .Therefore energy released in this process.

    (b)For fusion:

    From curve it is clear that B.E. / nucleon for lighter nuclei is lower therefore they are unstable but when

    they fused together , then they forms a heavy nucleus (lie in the middle portion on curve) which has more

    B.E. / nucleon than lighter ones and hence more stable. Therefore energy released in this process.

    FACTORS UPON WHICH STABILITY OF A NUCLEUS DEPENDS

    (i) In general, the greater the value of binding energy per nucleon, the greater is the stability of the nucleus.

    (ii) Nuclei having n/p ~ 1 but not less than one.

    NATURAL RADIOACTIVITY

    The process of spontaneous disintegration of the nuclei of heavy elements with the emission of certain

    types of radiations is known as natural radioactivity.

    The elements whose nuclei spontaneously disintegrate are called radioactive elements e.g. uranium (Z =

    92), radium (Z = 86) etc.

    LAWS OF RADIOACTIVE DECAY

    The rate of disintegration at any time (i.e. number of atoms that disintegrate per second) is directly

    proportional to the number of radioactive atoms present in the sample at that time. This is known as decay

    law.

    Let at time t = 0 number of atoms in radioactive element is

    number after time t the no. of atoms remain N due to decay. Further after time dt the number of atom dt

    disintegrate.

    Then at time t rate of disintegration will be dN/dt. From decay law

    Ndt

    dNN

    dt

    dN - - - - - - - (1)

    Here is radioactive constant. It is also known as decay constant or disintegration constant.

    The ve sign indicates that as time increases the value of N decreases.

    dtN

    dN

    Integrating both side of equation.

  • dtNN

    dN tN

    No

    0

    t

    NNe dttNLog o

    0

    tN

    NetNLog

    o0

    )0(0 tNLogNLog ee tN

    NLog e

    0

    - - - (2)

    Taking antilog on both the sides

    t

    eN

    N

    0 t

    eNN

    0 - - - - - (4)

    This eq shows that number of radioactive atom decreases exponentially with time. This means that the

    number of radioactive atom decreases rapidly at first and then more and more slowly as time goes on. This

    is shown in graph.

    Decay constant

    Puting t=1/ in eq (4) (i.e = 1/t)

    tteNN

    1

    0

    10

    eNN

    00 37.0 N

    e

    NN

    Hence decay constant may be defined as the reciprocal of time during which the no. of atoms of a

    radioactive substance falls to 1/e or 37% of original number of atoms presents (No).

    Half life(T1/2): - Time in which the radioactive atoms are reduced to half of there initial amount.

    From exponential law of disintegration eq (4) N = No et

    When time t =T , then N=No/2, putting this value in equation.

    21

    20

    0

    T

    e

    TeN

    N

    eT = 2

    Taking log on both the sides

    loge eT = loge 2 T loge e = loge2 T = loge2

    So half-life period

    693.02log TT e

    Average life or Mean Life: - The mean life or average life of a radioactive substance is defined as the ratio

    of total life time of all the radioactive atoms to the total no of such atoms in it. Average life period

    1

    atoms of number Total

    atoms all of periods life the of sum Ta

    The average life and half-life of a radioactive element s are different elements and it is not possible to

    change it.

    Notes:

    (i) For the decay to take place, the mass of the parent nucleus must be greater than the total mass of the

    decay products. In other words, radioactive decay is possible only if

    m (parent) > [m (daughter ) + m (decay particle)]

    If the decay products have more mass than the parent nucleus, then additional energy is required from

    external source to accomplish the decay.

  • (ii) The difference between the initial and final mass energies is called the Q value of the reaction.

    Using E = m c2, we have, Q = [ m (parent) m (daughter) m (decay particle )] c2

    If Q is positive, spontaneous decay may occur but if Q is negative, then spontaneous decay cannot occur.

    The positive Q value is available to the decay products as kinetic energy.

    Activity: Rate of disintegration of a radioactive material.

    A=N

    Unit: Becquerel(Bq) = one disintegration per second.

    ALPHA DECAY

    The phenomenon of emission of -particle from a radioactive nucleus .

    (i) Occurs when no. of p > no. of n (since repulsive force increases)

    (ii) In this process n /p ratio increases.

    e.g. 92U238 90U

    234 + 2He4 + Q

    GAMMA DECAY

    The phenomenon of emission of gamma ray photon

    from a radioactive substance.

    (i) After the emission of alpha or beta particle when an

    excited radioactive nucleus make transition to lower

    energy state then it emits gamma radiations. (to attain

    stability)

    (ii) Energy of gamma ray is order of MeV because

    difference in energy levels in a nucleus is of order of MeV.

    BETA DECAY

    The phenomenon of emission of an electron or positron from a radioactive substance.

    (i) Occurs when no. of p < no. of n

    (ii) In this process n /p ratio decreases.

    e.g. - 15P32 16S

    32 + -1e0 +

    +decay , 11Na22 10Ne

    22 + 1e0 +

  • Mechanism

    In -decay, a neutron is transformed into a proton within nucleus with an antineutrino.

    n p + + -1e0 +

    p n + + 1e0 +

    !! K.E. of beta particle is continuous because energy is shared by antineutrino.

    NUCLEAR REACTION

    Transformation of a stable nucleus into another by bombarding the former with suitable high energy

    particle.

    First successful nuclear reaction was carried out by Rutherford.

    7N14 + 2He

    4 8O17 + 1H

    1 or N(

    NUCLEAR FISSION

    The splitting of a heavy nucleus (A > 230) into two nuclei of comparable masses when it is bombarded

    with a neutron of suitable energy with the release of large amount of energy.

    92U235 + 0n

    1 56Ba144 + 36Kr

    89 + 3 0n1 + 200 MeV

    CHAIN REACTION

    A nuclear reaction in which the particle which start the reaction is also produced during the reaction

    to carry on the reaction further and further.

    e.g. fission of U-235.

    Neutron multiplication factor (or reproduction factor)

    k = Rate of production of neutrons

    Rate of loss of neutrons

    (i) If k > 1. Size of material is super critical. Results in explosion.

    (ii) If k < 1. Size of material is sub critical. Reaction gradually comes to halt.

    (iii) If k = 1.Reaction will be steady or sustained. Size of material is critical and mass is critical mass.

    TYPES OF CHAIN REACTIONS

    1. Explosive chain reaction: A nuclear chain reaction in which fission neutrons keep on increasing till the

    whole of the fissionable material is consumed (or disintegrated) is known as explosive chain reaction.

  • Such a reaction proceeds very quickly with the liberation of huge amount of energy in an extremely short

    time. Therefore, it is accompanied by an explosion.e.g. An atom bomb

    2. Controlled chain reaction. A chain reaction that proceeds slowly without any explosion and in which

    energy released can be controlled is known as controlled chain reaction.e.g. In nuclear reactor

    NUCLEAR REACTOR

    A nuclear reactor is a

    device in which controlled

    fission chain reaction takes

    place.

    Principle. Controlled

    fission chain reaction of U-

    235. The enormous heat

    produced in the fission

    process is used to convert

    water into steam at high

    pressure. The steam passes

    over the blades of a turbine

    and causes it to rotate. An electric generator coupled to the turbine produces electricity.

    Construction:

    (i) Nuclear fuel: The nuclear fuel is sealed in long, narrow metal aluminium tubes called fuel rods. The

    enriched U-235 ensures that at least one of the neutrons produced by a fission reaction has a good chance of

    causing fission in another U-235 nucleus.

    (ii) Moderator: The neutrons released by fission normally move very fast (2 MeV). At this high speed, the

    chance of a neutron being captured by another U-235 nucleus is very small. If the neutron is slowed, its

    chance of capture is much better. The slow neutrons are called thermal neutrons and possess energy of

    the order of 0.0235 eV. In order to slow down the fast fission neutrons, a moderator is used.

    e.g. graphite and heavy water.

    !!Heavy water is preferred

    (i) It does not absorb neutron (ii) It is more effective because mass of hydrogen atom is comparable to

    mass of neutron therefore neutron suffer elastic collision and can be slowed down effectively.

    (iii) Control rods: The control rods keep the net rate of production of neutrons to the required level by

    capturing the necessary proportion of neutrons before they initiate fission. When the control rods are

  • moved upward out of the reactor, the number of neutrons left to produce fission is increased. On the other

    hand, when the control rods are lowered, the number of neutrons for producing fission is decreased.

    e.g. Cadmium or Boron

    Safety rods: To stop the fission immediately when required.

    (iv) Coolant: To remove heat from the reactor core and take it to the place of its utilisation e.g. steam

    turbine. The steam runs the steam turbine coupled to the generator.

    e.g. Liquid sodium and heavy water

    (v) Protective shield: In a nuclear reactor, many types of harmful radiations are emitted. In order to

    prevent these radiations from reaching the persons working near the reactor, the reactor is enclosed in thick

    concrete walls.

    Working: Heat energy produced by fission is taken out with the help of coolant and utilize to produce

    steam.This steam rotates the turbine attached to generator to producd electricity.Spent steam is condensed

    and can be used again and again.

    Uses:

    (i)To generate electric power, (ii)to produce radioactive isotopes for their use in medical science,

    agriculture and industry, (iii) To produce high-velocity beams of neutrons for their use in nuclear physics.

    NUCLEAR FUSION

    The process of combining two light nuclei to form a heavy nucleus with the release of huge amount of

    energy is known as nuclear fusion.

    HOW TO CAUSE FUSION?

    Very high temperature (108K) and Very high pressure.

    As high temperature is required to cause fusion therefore it also called thermo-nuclear reaction.

    SOURCE OF SUN/STAR/STELLAR ENERGY

    Fusion reactions in the sun are responsible for its enormous heat. These reaction takes place in the core of

    the sun where high temperature and pressure is available.

    Proton-proton cycle

    In this reaction, two protons fuse to make a deuteron and finally helium through the following intermediate

    reactions:

    2 1H1 + 2 1H

    1 2 1H2 + 2+1e

    0 + energy ...(i)

    2 1H2 + 2 1H

    1 2 2He3 + energy ...(ii)

  • 2He3 + 2He

    3 2He4 + 2 1H

    1 + energy ...(iii)

    Summing up all the three above equations and canceling out the nuclides which occur on both sides,

    we get,

    4 1H1 2He

    4 + 2 +1e0 + energy

    COMPARISON BETWEEN FISSION AND FUSION

    S.No. Fission Fusion

    1 Splitting of heavy nucleus combining of light nuclei

    2 can be controlled can not be controlled

    3 emit harmful radiations no harmful radiations

    4 less energy than fusion more energy than fission

    Conversion of U-238 into Pu-239

    92U238

    +n 92U239 93Np

    239 + e- +

    93Np239 94Pu

    239 + e- +

    !! Ionising power of alpha particle more is because it has more mass and charge.

    !! Neutron is an unstable particle.

    !! Alpha particles are easily absorbed ,highest Ionising power,deflected by magnetic and elcteric field

    ; beta particles similar to cathode rays, deflected by magnetic and elcteric field; gamma rays similar

    to X rays ,travel with greatest speed,not deflected.

    Atomic Nucleus

    01. Show that nuclear density is constant.

    02. Find an expression for concentration of radioactive atom at any time t, N = N0e-t.

    03. Plot a graph between the Binding energy per nucleon and mass number. And hence explain from the

    graph why some atom undergo fission & some undergo fusion. Write two inferences from the graph.

    04. Draw a graph showing the variation of Nuclear force/potential energy of nucleons with distance. Mark

    the attractive and repulsive region.Write its four properties.

    05. What is a nuclear reactor. Explain its construction & working with a well labeled diagram.

    06. What is radioactivity. Why certain heavy atoms show the phenomenon of radioactivity.

    07. What happens to n / p ratio when

    (i) - Particle is emitted (ii) -, + Particle is emitted (iii) - ray is emitted Explain with example.

    08. Define activity. Write its unit.

    09. Why energy spectrum of - particle is continuous. Draw the distribution of kinetic energy of emitted electron emitted in the decay of 60Co nucleus.

  • 10. Draw the energy level diagram showing the emission of - rays by a 60Co nucleus subsequent to beta decay.

    11. How will you convert 23892U into 239

    94PU.

    12. Write the requirement for controlled thermonuclear reaction.

    13. Name the source of stellar energy & hence define nuclear fusion. Write one reaction for it.

    14. Compare the radius of two nuclei with mass number 1 and 27.

    15. Why heavy water is used to slow down fast moving neutrons.

    16. Define half life period & decay constant of a radioactive substance. Establish a relation between

    them.

    17. Define "disintegration constant " & "meanlife" of a radio active substance. Give the unit for each.

    18. which is more stable 73X or 4

    3Y. Why ?Are they isotope of the same element.

    19. Find the mass number and atomic number for each

    D D1

    D2 D3

    D4 (if for D2 Z = 71, A =176)

    20. A neutron is absorbed by a 63Li nucleus with subsequent emission of an alpha particle. Write the

    corresponding nuclear reaction.

    21. 23892U decays successively to form 234

    90Th, 234

    91Pa, 234

    92U, 230

    90Th , 226

    88Ra & 226

    86Rn. What are the

    radioactive radiation emitted in each decay process.

    22. Which of the following radiations -rays, -rays, -rays are (i) Similar to x-rays (ii) easily absorbed by matter (iii) travel with greatest speed

    (iv) similar to cathode rays

    23. Write the equation for & + decay within a nucleus. 24. Define mass defect and binding energy.

    Numericals

    01. The half life period of a radio active substance is 30 days. What is the time taken for 3/4th of its

    original mass to disintegrate. Calculate the decay constant.

    02. The half life of a radioactive substance is 1.192 x 107 s against alpha decay. Calculate the decay rate

    for 3.18 x 1015 atoms of the substance.

    03. Find the half life period of a radio active material if its activity drops to 1/16th of its initial value in 30

    days. Also find the mean life or average life of the sample and also the disintegration constant.

    04. Calculate B. E/ nucleon of Bi209. Given m(83Bi209 ) = 208.980388 amu , mn = 1.008665 amu & mp =

    1.007825 amu , 1 amu = 931.5 MeV.

    05. A neutron is absorbed by nucleus by the subsequent emission of alpha. Calculate the energy

    released in the following nuclear reaction. Write the corresponding nuclear reaction.Calculate the

    energy released.

    36Li = 6.015126u , 0

    1n = 1.008665 u, 24He = 4.002604u, 1

    3H = 3.016049u

    06. The isotopes of chlorine 35Cl & 37Cl have abundance 75.4 % & 24.6 % respectively. If there

    masses are 34.98 U & 36.98 U, then what is the mass of natural chlorine atom. (35.47u)

    07. The half life of 92238U against -decays is 4.5 x 109 year. What is the activity of 1g sample of 92

    238U .

    (1.23 x104Bq)

    08. Tritium has a half-life of 12.5y against beta decay. What fraction of a sample of pure tritium will

    remains undecayed after 25y.

    09. Given 92238U = 238.050790u, 11H = 1.00783u, 91

    237Pa = 237.05121u. Show that 92238U cannot

    spontaneously emit a proton.

    10. How long an electric lamp of 100W can be kept glowing by fusion of 2kg of Deuterium. The fusion

    reaction can be taken as

    12

    12

    23

    01 32H H He n MeV . (4.9 x104 s)

    11. Two nuclei P,Q have equal number of atoms at t=0. Their half lives are 3 hours and 9 hours

    rexpectively. Compare their rates of disintegration after 18 hours.