30 Worksheet (A2) Data needed to answer questions can be found in the Data, formulae and relationships sheet. 1
2
a b
Write down Einstein’s famous equation relating mass and energy. Determine the change in energy equialent to a change in mass! i of 1." g ii equal to that of an electron $%.1 × 1"&'1 (g ( g).
a
b
1# .-
.
Determine the mass of each of the following particles in terms of u! i an /particle of mass .0 × 1" (g (g ii a carbon1' atom of mass #.1 × 1" (g (g. Determine the mass of each of the following particles in (ilograms! i a proton of mass 1."1 u ii a uranium#'0 nucleus of mass #'2.%% u.
3
3tate three qu quantities consered in all nuclear reactions.
4
a b
E4plain why e4ternal energy is required to 5split’ a nucleus. Define the binding energy of of a nucleus.
c
+he binding energy of the nuclide
6
[#] [#]
*n nuclear physics, it is common practice to quote the mass of a nuclear particle in terms of the unified atomic mass unit, u. +he unified atomic mass unit u is defined as onetwelfth of the mass of an atom of the carbon isotope
5
[1]
1. 76
[1] [1] [1] [1] ['] [1] [1]
is 1#7 8e9. -alculate the binding energy
per nucleon.
[#]
Define the half-life of of a radioactie isotope. +he halflife of a particular isotope is #" minutes. : sample initially contains N " nuclei of this isotope. Determine the number of nuclei of the isotope left in t he sample after! i #" minutes ii 1." hour.
[1]
[1] [#]
+he actiity of an /source is 02" ;q. +he (inetic energy of each /particle is 7. < 1" &12 =. +he isotope in the source has a ery long halflife. a -alculate the number of /particles emitted by the source in! i 1 second ii 1 hour. b Determine the total energy released by the source in a time of 1 second. c 3tate the rate at which energy is emitted from this /source.
[1] [1] ['] [1]
a b
:3 and : >eel ?hysics
6riginal material @ -ambridge Aniersity ?ress #"1"
1
30 Worksheet (A2)
7
+he binding energy per nucleon against nucleon number graph for some common nuclides is shown below.
a
*dentify the most stable nuclide. E4plain your answer.
b
Ase the graph to estimate the binding energy for the nucleus of
c
Ase the gr graph to estimate the energy released in the following fusion reaction. # 1
d
8
[#] 1# .-
B
#
.
[#] [2]
2
+ 1 B → # Be
+he fusion reaction shown in c is one of the many that occur in the interior of stars. 3tate the conditions necessary to initiate such reactions in stars.
[#]
Ase the data gien below to determine the binding bi nding energy and the binding energy per nucleon of the nuclide
#'0 %# A
.
mass of proton = 1."" u mass of neutron = 1.""% 1.""% u
:3 and : >eel ?hysics
[] mass mass of ura urani nium um#' #'0 0 nucl nucleu euss = #'2.%%# u
6riginal material @ -ambridge Aniersity ?ress #"1"
2
30 Worksheet (A2)
9
a b
Describe the process of induced nuclear fission. +he diagram shows the fission of uranium#'0 in accordance with the nuclear equation! #'0 1 %0 1'% %# A + " n → '7 3r + 02 Ce +
i ii
[1]
1
#" n
-opy the diagram, adding labels to identify the neutrons, the strontium nuclide and the 4enon nuclide. E4plain why energy is released in the reaction aboe.
[1] [#]
iii Ase the following data to determine the energy released in a single fission reaction
inoling
#'0 A %#
and
1 "n
.
[0]
mass of
#'0 A = %#
mass of
%0 '7 3r =
mass of
1 "n
mass of
1'% 02
'.%"# × 1" (g
1.0 × 1" (g
=
1.00 × 1" (g
Ce
#.'" × 1" (g
=
10 6ne of the neutroninduced fission reactions of uranium#'0 may be represented b y the following nuclear equations. #'0 %# A #'. %#
A
1 "n
→
12. 0
→
#'. %# A
>a
7 '0 ;r
' "1 n
+he binding energies per nucleon for these nuclides are! #'. %#
A, .0% 8e9
12. 0
>a, 7.21 8e9
7 '0 ;r,
-alculate the energy released in 8e9 when the 11 +he halflife of the radon isotope
##" 7.
7.0% 8e9.
#'. %# A
nu nucleus undergoes fission.
[']
Fn is 0 s.
a
Determine the decay constant in s &1.
b
-alculate the actiity of a sample containing ." × 1"1" nuclei of
['] ##" 7.
Fn .
[']
12 +he actiity of a radioactie source containing 7." × 1"12 undecayed nuclei is 0." × 1"% ;q. a Determine the decay constant in s &1. b -alculate the halflife of the nucleus. c Bow many undecayed nuclei will be left after 2" hoursG 13 a b
Define the decay constant of of a nucleus. +he thorium isotope
## %"
[1]
+h has a halflife of 17 days.
: particular radioactie source contains 2." × 1"1# nuclei of the isotope i
['] ['] [']
Determine the decay constant for the thorium isotope
## %"
## %"
+h .
+h in s&1.
[']
ii What is the initial actiity of the sourceG iii -alculate the actiity of the source after ' days.
['] [#]
14 : sample of roc( is (nown to contain 1." Hg of the radioactie radium isotope
##. 77 Fa
.
+he halflife of this particular isotope is 1"" years. +he molar mass of radium## is ## g. ##. 77 Fa
a
Determine the number of nuclei of the isotope
b
-alculate the actiity from decay of the radium## in the sample.
:3 and : >eel ?hysics
in in the roc( sample.
6riginal material @ -ambridge Aniersity ?ress #"1"
[#] [']
3
30 Worksheet (A2)
15 *n a process referred to as 5annihilation’, a particle interacts with its antiparticle and the entire mass of the combined particles is transformed into energy in the form of photons. +he following equation represents the interaction of a proton $p) and its antiparticle, the antiproton $ p ). 1 1 1 p + −1 p →
I+I
+he antiproton has the same mass as a proton J the onl y difference is that it has a negatie charge. Determine the waelength λ of of each of the two identical photons emitted in the reaction aboe. $8ass of a proton = 1. × 1" (g (g.)
[0]
16 Does fusion or fission produce more energy per (ilogram of fuelG :nswer this question by considering the fusion reaction in 7 c and the fission reaction in 9 b. $+he mol molaar ma masses ses of of hy hydrogen# an and ur uranium ium#'0 ar are # g an and #' #'0 g, g, re respe spectiely. ly.)
[]
17 3ome astronomers beliee that our solar system was formed 0." < 1" % years ago. :ssuming that all uranium#'7 nuclei were formed before this time, what fraction of the original uranium#'7 nuclei remain in the s olar system todayG +he isotope of uranium #'7 %# A
has a halflife of 2.0 × 1"% y. y.
[2]
+otal!
:3 and : >eel ?hysics
1""
3core!
6riginal material @ -ambridge Aniersity ?ress #"1"
Thank you for interesting in our services. We are a non-profit group that run this website to share documents. We need your help to maintenance this website.