dpps___4__nulcear_physics___radioactive__10-6-14

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  • 8/11/2019 DPPS___4__Nulcear_Physics___Radioactive__10-6-14

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    CAREER POINT

    PRACTICE PROBLEM SHEET

    PHYSICS

    Topic Nuclear Physics & Radioactivity-1

    Q.1 A star of mass M0, radius R0contracts to radius R. Energy radiated by the star assuming uniform density in

    each case while temperature remains unchanged is -

    (1M0c! (! M0c

    !

    !

    0

    "1R

    R(#M0c

    !

    0

    "1R

    R($M0c

    !

    #

    0

    "1R

    R

    Q.2 %he total energy E of a sub-atomic particle of rest mass m0 mo&ing at non-relati&istic speed

    & is -

    (1E' m0c! (!E'

    !

    1m0&

    ! (#E' m0c!

    !

    1m0&

    ! ($E' m0c!"

    !

    1m0&

    !

    Q.3 )f udenotes 1 atomic mass unit. *ne atom of an element has mass e+actly eual to Au, where A is mass

    number of element -

    (1A' 1 (!A' 1!

    (#A' 1 ($ A can tae up any integral &alue from 1 to 110

    Q.4 /ast neutrons can easily be slowed down by -

    (1 the use of lead shielding (! passing them through hea&y water

    (# elastic collisions with hea&y nuclei ($ applying a strong electric field

    Q.5 hich of the following statements is correct -

    (1 eta rays are same as cathode rays (! 2amma rays are high energy neutrons

    (# Alpha particles are singly ioni3ed helium atoms ($ 4rotons and neutrons ha&e e+actly the same mass

    Q.6 Mar the correct statement -

    (1 E&ery element has only two stable isotopes

    (! All isotopes of e&ery element are radioacti&e

    (# *nly one isotope of each element is stable

    ($ 5uclei of different elements can ha&e the same number of neutrons

    Q. %he chemical beha&iour of an atom depends upon -

    (1 the number of nucleons in its nucleus (! the number of protons in its nucleus

    (# the number of neutrons in its nucleus ($ the number of electrons in its atom

    Q.! 6uring a nuclear fusion reaction 7CAREER POINT, CP Tower, IPIA, Road No.1, Kota (Raj.), Ph: 0744-3040000 1

    CP Live Enthuse Class XII -2015

    PRE

    "PPS #$ - 0% 6iscussion on 71"-6-2"14

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    (1 a hea&y nucleus breas into two fragments by itself

    (! a light nucleus bombarded by thermal neutrons breas up

    (# a hea&y nucleus bombarded by thermal neutrons breas up

    ($ two light nuclei combine to gi&e a moderate nucleus and possibly other products

    Q.# oron rods in a nuclear reactor are used to -

    (1 absorb e+cess neutrons (! absorb alpha-particles

    (# slow down the reaction ($ speed up the reaction

    Q.1" hich of the following statement (s is (are correct 8

    (1 %he rest mass of a stable nucleus is less than the sum of the rest masses of its separated nucleons.

    (! %he rest mass of a stable nucleus is greater than the sum of the rest masses of its separated nucleons.

    (# )n nuclear fusion, energy is released by fusing two nuclei of medium mass (appro+imately. 100 amu

    ($ 5one of these

    Q.11 9et mpbe the mass of a proton, m

    nthe mass of neutron, M

    1the mass of a

    105e!0nucleus and M

    !the mass of a

    !0:a$0

    nucleus. %hen -

    (1 M!' !M

    1(! M

    !; !M

    1(# M

    !< !M

    1($ M

    1< 10 (m

    n m

    p

    Q.12 *rder of magnitude of density of =ranium nucleus is,>mp' 1.? @ 10"!?g

    (1 10!0gBm# (! 101?gBm# (# 101$gBm# ($ 1011gBm#

    Q.13 inding energy per necleon &ersus mass number cur&e for nuclei is shown in the figure. , C, D and are

    four neclei indicated on the cur&e. %he process that would release energy is 7

    (1 D! (! C (# !D ($ C ' D

    Q.14 )n a star all Felium nuclei are con&erted into o+ygen. )f atomic mass of MFe

    ' $.00!= and atomic mass of

    o+ygen M0' 1G.HHH$=, then the reaction energy per atom of o+ygen -

    (1 10.! MeI (! 0 MeI (# G.!$ MeI ($ !0.$ MeI

    Q.15 %he nucleus of element C (A ' !!0 undergoes -decay. )f J-&alue of the reaction is G.G MeI, then

    appro+imate inetic energy of -particle is -

    (1 G. MeI (! G.$ MeI (# $.H MeI ($ .G MeI

    CAREER POINT, CP Tower, IPIA, Road No.1, Kota (Raj.), Ph: 0744-3040000 !

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    ANSWERS$

    1.%4 6ensity of star of mass M0, radius R0 is '

    #0

    0

    #

    $R

    M

    *n contracting the new mass becomes

    M'#

    $R#'M0

    #

    0

    R

    R

    9oss in mass due to contraction ' " M

    Loss = M0 M

    Energy radiated ' c!M

    2.%3 E' mc!

    E' m0c!

    !B1

    !

    !

    "1

    c

    V

    Kincec

    &