ch29 - nuclear physics Flashcards

(52 cards)

1
Q

nucleus before decay

A

parent nucleus

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2
Q

nucleus after decay

A

daughter nucleus

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3
Q

in alpha decay

A

. nucleon number decreases by 4
. proton number decreases by 2

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4
Q

in beta - decay

A

. nucleon number doesnt change
. proton number increases by 1

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5
Q

in beta + decay

A

. nucleon number us unchanged
. proton number decreases by 1

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6
Q

in gamma decay

A

. nucleon number unchanged
. proton number unchanged

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7
Q

in a stable nucleus

A

nucleons are tightly bound by a strong nuclear force

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8
Q

do seperate nucleons have more or less mass than the nucleus

A

MORE

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9
Q

to dismantle a nucleus

A

work done against strong nuclear force

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10
Q

why does seperated nucleons have more mass

A

. work done against nuclear force to seperate nucleons
. each nucleon in deep potential well
. each nucleon has more potential energy
. this energy transferred to mass

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11
Q

einstein’s mass energy equation

A

<>E = <>mc²
E = c²<>m
E = mc²

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12
Q

accordingto einstein’s equation

A

. mass of system increases when energy is SUPPLIED
. mass of system decreases when energy is RELEASED

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13
Q

proton rest mass

A

1.672 623 * 10 ^-27

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14
Q

neutron rest mass

A

1.674 929 * 10 ^-27

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15
Q

12, 6 C nucleus rest mass

A
  1. 926 483 * 10 ^-27
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16
Q

mass defect

A

the difference between the total mass of the individual seperate nucleons and the mass of the nucleus

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17
Q

E = mc² applies to all energy changes

A

. includes chemical reactions
. not just nuclear processes

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18
Q

atomic mass unit

A

1/12 of the mass of a neutral atom or carbon-12

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19
Q

u to kg

A

1.66 * 10^ - 27

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20
Q

if negative change in mass

A

energy is lost

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21
Q

binding energy

A

the minimum external energy required to completely seperate all the neutrons and protons of a nucleus to infinity

22
Q

binding energy is EXTERNAL, NOT stored in nucleus

23
Q

findinf binding energy per nucleon

A

. determine mass defect for nucleus
. use E = mc² for binding energy of nucleus
. divide the nucleus binding energy by number of nucleons

24
Q

higher bindig energy

25
nucleus with highest binding energy / most stable isotope in nature
56, 26 Fe
26
stable nuclei
. 12, 6 C . 16, 8 O . 4, 2 He
27
for nuclides with A > 20
. not much variation in binding energy per nucleon
28
fission
the process in which a massive nucleus
29
induced fission
. split nucleus by firing a slow moving neutron at it
30
induced fission reaction
1,0 neutron + 235, 92 U => 236, 92 U => 142, 56 Ba + 92, 36 Kr + 2 1,0 neutron
31
uranium - 236
highly unstable
32
in the induced fission uranium reaction
. energy released . two fast moving electrons released . two product fragments have more binding energy
33
fusion
the process in which two light nuclei join together to form a heavier nucleus
34
which fusion reaction takes place in the core of many stars
2,1 H + 1,1 proton => 3, 2 He
35
Geiger Muller (GM) tube
. detects radiation from weak source . each count is reresents detection of alpha/beta particle of gamma ray photon . counter beeps in random, irregular manner
36
ratemeter
. measures faster rates of radiation . fluctuating needle . has control for setting the time constant . fluctuations more smooth on 5s setting
37
spontaneous decaying
. radioactive decay occurs for unstable nucleus . cannot be predicted
38
for radioactive substance, number of undecayed nuclei
gradually decreases
39
radioactive decay is
. spontaneous . random
40
radioactive decay is spontaneous
. decay of particular nucleus is not affected by other nuclei . not affected by chemical reactions or external factors like temperature and pressure
41
radioactive decay is random
. can't predict when a particluar nucleus will decay . each nucleus has same chance of decaying per unit time
42
decay constant, lambda
the probability that an individual nucleus will decay per unit time interval units = s-1, min -1, h -1, y -1
43
activity, A
the rate of decay of nuclei of a radioactive source unit = becquerel, Bq
44
formula for activity
A = - rate constant * N minus sign means number of decayed nuclei decreases with time
45
more the decay constant
greater the activity of sample
46
count rate, R
the number of particles or gamma photons detected per unit time by a GM tube always a fraction of the activity of a sample
47
corrected count rate
count rate - background radiation
48
exponential decay
the decrease of a quanitiy where the rate of decrease is proportional to the value of the quantity
49
half life
the half life of an isotope is the mean time taken for half of the active nuclei in a sample to decay
50
equations for radioactive decay
N = No e^-lambda*t A = Ao e^-lambda*t R = Ro e^-lambda*t X = Xo e^-lambda*t Xo is that at time = 0
51
relating decay constant and half life
lambda = ln2/ (t1/2) lambda = 0.693/ half life
52
lambda = ln2/ (t1/2) equation derivation
x = ln y N = No * e^ -lambda* t N/No = e^ (-lambda* t1/2) = 1/2 e^ (lambda* t1/2) = 2 lambda* t1/2 = ln2 lambda = ln2/ (t1/2)