General Physics, 2nd Edition
2nd Edition
ISBN: 9780471522782
Author: Morton M. Sternheim
Publisher: WILEY
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Chapter 30, Problem 32E
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a) For each of the following nuclear equations, state the atomic number, mass number, and symbol X of the missing reactants or products.
i. He +Au
→ 4X +?H
197
A =
Z =
X:
ii. in +Ba
→ 4X +y
56
A =
Z =
X:
iii. 137CS
Ba +4X+7
55
56
A =
Z =
X:
iv. in +X → P +H
A =
Z =
X:
v. 210BI
83
81
A =
Z =
X:
b) Choose the correct symbol for the missing particle in the following equation:
Na - Ne +9e+
11
10
Calculate the threshold energy for the following
reactings:
(i) n+Th²³2 → Th²³1 + 2n
(ii)n+Th232 → Th²33 + y
1 E:17
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Example: which of the following are possible reaction
Xe+Sr +2,n
1- 'n+ U →*
2– ¿n+ U →* Sn + Mo +3¿n
→ I+ Nb+3,n
235
140
94
54
38
1
235
132
101
2- n+U
50
1
239
127
3- n+ Pu
94
41
Chapter 30 Solutions
General Physics, 2nd Edition
Ch. 30 - Prob. 1RQCh. 30 - Prob. 2RQCh. 30 - Prob. 3RQCh. 30 - Prob. 4RQCh. 30 - Prob. 5RQCh. 30 - Prob. 6RQCh. 30 - Prob. 7RQCh. 30 - Prob. 8RQCh. 30 - Prob. 9RQCh. 30 - Prob. 10RQ
Ch. 30 - Prob. 11RQCh. 30 - Prob. 12RQCh. 30 - Prob. 1ECh. 30 - Prob. 2ECh. 30 - Prob. 3ECh. 30 - Prob. 4ECh. 30 - Prob. 5ECh. 30 - Prob. 7ECh. 30 - Prob. 8ECh. 30 - Prob. 9ECh. 30 - Prob. 10ECh. 30 - Prob. 11ECh. 30 - Prob. 12ECh. 30 - Prob. 13ECh. 30 - Prob. 14ECh. 30 - Prob. 15ECh. 30 - Prob. 16ECh. 30 - Prob. 17ECh. 30 - Prob. 18ECh. 30 - Prob. 19ECh. 30 - Prob. 20ECh. 30 - Prob. 21ECh. 30 - Prob. 22ECh. 30 - Prob. 23ECh. 30 - Prob. 24ECh. 30 - Prob. 25ECh. 30 - Prob. 26ECh. 30 - Prob. 27ECh. 30 - Prob. 28ECh. 30 - Prob. 29ECh. 30 - Prob. 30ECh. 30 - Prob. 31ECh. 30 - Prob. 32ECh. 30 - Prob. 33ECh. 30 - Prob. 34ECh. 30 - Prob. 35ECh. 30 - Prob. 36ECh. 30 - Prob. 37ECh. 30 - Prob. 38ECh. 30 - Prob. 39ECh. 30 - Prob. 40ECh. 30 - Prob. 41ECh. 30 - Prob. 42ECh. 30 - Prob. 43ECh. 30 - Prob. 44ECh. 30 - Prob. 46ECh. 30 - Prob. 47ECh. 30 - Prob. 48ECh. 30 - Prob. 49ECh. 30 - Prob. 51ECh. 30 - Prob. 52ECh. 30 - Prob. 53ECh. 30 - Prob. 54ECh. 30 - Prob. 55ECh. 30 - Prob. 56ECh. 30 - Prob. 57ECh. 30 - Prob. 58ECh. 30 - Prob. 59ECh. 30 - Prob. 60ECh. 30 - Prob. 61ECh. 30 - Prob. 62ECh. 30 - Prob. 63ECh. 30 - Prob. 64ECh. 30 - Prob. 65E
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- (a) Write the complete reaction equation for electron capture by 15O. (b) Calculate the energy released.arrow_forwardWhich of the following completes the reaction 98 42 Mo → on? 97 , Мо 42 100 Ru 44 93 Nb 41 99 Tc 43arrow_forwardDetermine the resultant reactions at A and B. (ANS: RA = 18.03kN, 33.69° N of E and RB = 33.54kN) 3m MATHalino.com Figure P-351 40 KN 1m Barrow_forward
- Select the missing product of this nuclear reaction: 235 U + n 92 1 1 90 → ? + 2 n + Rb 37 O A. 144 Cs 55 о в. 146 Cs 55 C. 143. 53 O D. 143 Хе 54arrow_forwardA. Direction: Complete the table by filling up the missing particle, nucleus or name of decay. Write your answers on the spaces provided. Just write alpha, beta or gamma on the 3rd column. Number 1 serves as an example. 1. 210 84 → He + 206 82 Alpha 2. 3. 4. 5. 6. 1³N → 144 Nd→ ¹³N - 41 Ar + _je + 130 140 Ce CLarrow_forward15. A star initially has 1040 deuterons. It produces energy via the 3 4 processes, H² +₁H² →→ ₁H³ + p and, H² + ₁H³ → ₂Heª + n. 1 the If the average power radiated by the star is 10¹6 W, deuteron supply of the star is exhausted in a time of the order of (a) 106 S (c) 10 ¹² s (b) 108 s (d) 10¹6 s The mass of the nuclei are as follows M(H²) = 2.014 amu; M(n) = 1.008 amu; M(p) = 1.007 amu; M(He* )= 4.001 amu. 4arrow_forward
- Learning Check Nuclear Reaction: 1. n + 137 Ва 56 →? +y 2. n + 14N → ? + }H 3. п + 1,c -? + }H 4. n + 1ºB → 3Li + ? 5. р+ 13с -? +n Nuclear Fission: 235 1. n + 2U → ? + Sr + 2n 93 38 2. n + 232U → 137 96 331 + 33Y+ ?narrow_forwardNuclear Fission: 1. n+ 2U → ? + 3gSr + 2n 2. n+ 235U → 1I 137 + 33Y+ ?narrow_forwardAnother set of reactions that result in the fusing ofhydrogen into helium in the Sun and especially in hotter starsis called the carbon cycle. It is12C + 1H → 13N + γ,13N → 13C + e+ + ve,13C + 1H → 14N + γ,14N + 1H → 15O + γ,15O → 15N + e+ + ve,15N + 1H → 12C + 4He.Write down the overall effect of the carbon cycle (as wasdone for the proton-proton cycle in2e− + 41H → 4 He + 2ve + 6γ ). Note the number of protons ( 1H ) required and assume that the positrons ( e+ ) annihilate electrons to form more γ rays.arrow_forward
- 10) Now you have a nucleus with 13 protons at x = 6.2 Angstroms on the x-axis. How much work would it take to bring in ANOTHER nucleus with 7 protons from 1 m away and place it at y = 8.0 Angstroms on the y-axis? 70.0 eV 116.7 eV -12.6 eV 129.3 eVarrow_forward9. How many grams of 235 U are consumed in one year, in order to supply the energy needs of a household that uses 28.0 92 kWh of energy per day, on the average? 178 srg 78 srgl srg178arrow_forwardIdentify the conserved quantities in the following processes. A° + u- + v. (c) K- + p → £° +n (a) E- (b) Kg → 27° (d) 2° → A° + y (e) et + e- -→ µt + µ (f) p +n → A + E- (g) Which reactions cannot occur? Why not?arrow_forward
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