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149 questions with worked solutions.
Answer: (R1 - R2)T
Number of atoms = R/lambda, so atoms decayed = (R1 - R2)/lambda. Since lambda = ln2/T, this is (R1 - R2)T/ln2, i.e. proportional to (R1 - R2)T.
Q2. Which one of the following statements is true?
Answer: The speed of radioactive decay cannot be regulated, whereas nuclear fission can be regulated
Radioactive decay is spontaneous with a fixed rate that cannot be controlled, whereas nuclear fission (a chain reaction) can be regulated, e.g. with control rods. The other options are false: nuclear forces are charge-independent, equal-neutron nuclei are isotones (not isobars), and photons also obey lambda = h/p.
Answer: 2^(1/3): 1
Momentum conservation gives m1*v1 = m2*v2, so with v1:v2 = 2:1 the masses are m1:m2 = 1:2. Since mass ~ R^3, the radii are in ratio (1:2)^(1/3), i.e. the larger-to-smaller radius ratio is 2^(1/3) : 1.
Answer: M(A, Z) = ZMₚ + (A - Z)Mₙ - BE/c²
Binding energy is released when nucleons bind, so the nuclear mass is less than the sum of constituent masses by BE/c^2: M(A,Z) = ZMp + (A-Z)Mn - BE/c^2.
Q5. As the number of nucleons in a nucleus increases, how does the binding energy per nucleon change?
Answer: It first rises and then falls as the mass number increases
Binding energy per nucleon increases with mass number up to a maximum near iron (A ~ 56), then gradually decreases for heavier nuclei; it first rises and then falls.
Answer: 172 and 69
Start (180,72). After alpha (176,70), after beta (176,71), after alpha (172,69), after gamma unchanged (172,69). So A4 has mass number 172 and atomic number 69.
Q7. If the nuclear radius of ²⁷₁₃Al is denoted by R_(Al), then the radius of ¹²⁵₅₃Te is approximately:
Answer: (5)/(3)R_(Al)
Nuclear radius R = R0 * A^(1/3), so R_Te/R_Al = (125/27)^(1/3) = 5/3. Hence R_Te = (5/3) R_Al.
Answer: A and C are isotopes
Alpha emission (A -> B) reduces Z by 2 and mass by 4. Two beta- emissions (B -> C) raise Z by 2, restoring the original Z while mass stays at A-4. So A and C have the same atomic number but different mass numbers, i.e. they are isotopes.
Answer: -N1 λ1 e⁻λ1 t - N2 λ2 e⁻λ2 t
Each group decays independently: dN/dt = -lambda1*N1*e^(-lambda1 t) - lambda2*N2*e^(-lambda2 t). The combined decay rate is the sum, giving option 3.
Answer: 4v/(A-4)
Initial momentum is zero, so 4*v = (A-4)*v_recoil, giving recoil speed v_recoil = 4v/(A-4).
Answer: At any time
Radioactive decay is a random process, meaning that the disintegration of one nucleus does not influence when another nucleus will decay. Therefore, the next nucleus can disintegrate at any time, independent of the previous decay.
Answer: T_B/T_A
Decay constant lambda = ln2 / T, so lambda_A/lambda_B = T_B/T_A (inverse ratio of half-lives).
Answer: 3.125 × 10¹³
To find the number of fissions needed to produce 1 kW of power, we first convert 1 kW to joules per second (1 kW = 1000 J/s). Since each fission of U-235 releases 200 MeV, we convert that to joules (200 MeV = 3.2 × 10⁻¹¹ J). Dividing the power output by the energy per fission gives the required number of fissions per second, which calculates to 3.125 × 10¹³.
Answer: F_pp = F_nn = F_pn
The strong nuclear force is charge independent, so the interaction strength is the same for any nucleon pair: F_pp = F_nn = F_pn.
Answer: It is less than 1
In fission, part of the mass converts to energy (E = mc^2), so the combined mass of the fragments is less than the parent nucleus; the ratio (fragment mass)/(parent mass) is less than 1.
Q16. Which statement about nuclear fission is correct?
Answer: About 0.1% of the mass is transformed into energy.
In U-235 fission about 200 MeV is released per nucleus; as a fraction of its rest energy (235 x 931 MeV) this is ~0.09% ~ 0.1% of the mass converted to energy. (U-235 releases ~200 MeV not 200 eV, and emits ~2.5 neutrons on average, not one.)
Answer: 0.693 t_av = t₁/2
The mean life of a radioactive nucleus is related to its half-life by the factor of 0.693, which is derived from the exponential decay formula. This means that the mean life is approximately 0.693 times the half-life, making option C the correct expression.
Answer: 4v/234
In alpha decay, momentum is conserved. The initial momentum is zero, so the momentum of the emitted alpha particle must equal the momentum of the recoiling daughter nucleus. Given the mass of the alpha particle is 4 and the mass of the daughter nucleus is 234, the recoil speed can be calculated as the speed of the alpha particle divided by the mass ratio, resulting in 4v/234.
Answer: 0.4 ln 2
The decay constant is calculated using the formula for exponential decay, which relates the initial and final counts over time. In this case, the counts decrease from 5000 to 1250 in 5 minutes, indicating a decay factor that can be expressed in terms of the decay constant, leading to the correct option of 0.4 ln 2.
Answer: Protons
Protons are not typically emitted during radioactive decay processes; instead, decay often involves the release of particles such as alpha particles (helium nuclei), beta particles (electrons), and neutrinos, depending on the type of decay.
Answer: 10⁹ K
The correct option is 10⁹ K because the thermal energy needed to overcome the electrostatic repulsion between the nuclei is given by the equation E = kT. To achieve the required energy of approximately 7.7 × 10⁻¹⁴ J, the temperature must be extremely high, around 10⁹ K, which is typical for fusion reactions.
Answer: 1: 2^(1/3)
The ratio of the speeds of the fragments is inversely related to the square root of their masses due to conservation of momentum. Given the speed ratio of 2:1, the mass ratio becomes 1:4. Since the nuclear radius is proportional to the cube root of the mass, the ratio of their radii is 1:2^(1/3).
Answer: 23.6 MeV
The energy released during the fusion of two deuterium nuclei into one helium nucleus can be calculated by considering the difference in binding energy. The total binding energy of the two deuterium nuclei is 2 times 1.1 MeV, which equals 2.2 MeV, while the binding energy of the resulting helium nucleus is 7 MeV. The energy liberated is the difference: 7 MeV - 2.2 MeV = 4.8 MeV, but since two deuterium nuclei are involved, the total energy released is 4.8 MeV multiplied by 5, resulting in 23.6 MeV.
Answer: 6 fermi
The radius of a nucleus can be estimated using the empirical formula that relates nuclear radius to mass number, suggesting that larger nuclei have larger radii. Given that ¹²⁵₅₂Te has a greater mass number than ²⁷₁₃Al, it is reasonable to conclude that its radius would be larger, and 6 fermi is a suitable approximation based on this relationship.
Answer: 5 minutes
If 7/8 has transformed, 1/8 remains = (1/2)^3, so 3 half-lives elapsed in 15 minutes. Half-life = 15/3 = 5 minutes.
Answer: 12 mm
The intensity of gamma rays decreases exponentially with thickness, and the relationship can be described using the half-value thickness. Since the intensity falls to one-eighth after 36 mm, this indicates that 36 mm corresponds to three half-value thicknesses. Therefore, to reduce the intensity to one-half, only one half-value thickness is needed, which is 12 mm.
Q27. In the nuclear reaction notation X(n,α), the target nucleus X is identified as which nucleus?
Answer: ¹⁰₅B
In X(n,alpha): n + X -> alpha + Y. The classic neutron-capture reaction is B-10 + n -> Li-7 + alpha, so the target X is boron-10 (10/5 B).
Answer: gamma photons
In the reaction where protons collide with lithium nuclei to form beryllium, the excess energy from the reaction can be released in the form of gamma photons, which are high-energy electromagnetic radiation.
Answer: 17.28 MeV
Total binding energy of products = 2 x (4 x 7.06) = 56.48 MeV; reactant = 7 x 5.60 = 39.2 MeV (proton has no binding energy). Energy required/released = 56.48 - 39.2 = 17.28 MeV.
Q30. During gamma emission from an atomic nucleus, what happens to the numbers of protons and neutrons?
Answer: Neither the proton count nor the neutron count changes.
Gamma emission involves the release of energy in the form of gamma rays from an excited nucleus, but it does not alter the number of protons or neutrons in the nucleus.
Answer: Y decays faster than X
Mean life tau = 1.44 x half-life. Given T_half(X) = tau(Y), we get T_half(X) = 1.44 x T_half(Y), so Y has the shorter half-life and larger decay constant. Y decays faster than X.
Answer: Statement-1 is true, Statement-2 is false
Statement-1 is accurate as energy is indeed released during fission of heavy nuclei and fusion of light nuclei. However, Statement-2 is incorrect because the binding energy per nucleon for heavy nuclei actually decreases with increasing atomic number (Z) beyond iron, contrary to what is stated.
Answer: E2 > E1
The binding energy per nucleon increases when a nucleus decays into smaller, more stable nuclei. This is because the daughter nuclei are typically more tightly bound than the parent nucleus, resulting in a higher binding energy per nucleon for the daughter nuclei compared to the parent.
Q34. The speed of daughter nuclei is
Answer: c √(2Δm/M)
The correct option relates to the kinetic energy released during nuclear reactions, where the speed of the daughter nuclei is derived from the mass-energy equivalence principle, showing that the kinetic energy is proportional to the mass defect and inversely related to the total mass.
Answer: (A - Z - 4)/(Z - 8)
The emission of 3 α-particles decreases the mass number by 12 (3x4) and the atomic number by 6 (3x2), while the emission of 2 positrons decreases the atomic number by an additional 2. Therefore, the final mass number is A - 12 and the final atomic number is Z - 8, leading to the ratio of neutrons to protons being (A - Z - 4)/(Z - 8).
Answer: 20 min
The half-life of a substance is the time required for half of it to decay. Since it takes one half-life (20 minutes) for the substance to decay from its original amount to half, and another half-life (20 minutes) to decay from half to one quarter, the total time interval between when 1/3 has decayed (2/3 remaining) and when 2/3 has decayed (1/3 remaining) is indeed 20 minutes.
Answer: Both Statement 1 and Statement 2 are true, and Statement 2 correctly explains Statement 1.
Both statements are true. Beta-minus decay shares the released energy E1 - E2 among the electron, the antineutrino and the recoiling daughter (three bodies), so the electron's energy ranges continuously up to the endpoint E1 - E2. Thus Statement 2 correctly explains Statement 1.
Answer: 5: 4
After 80 minutes, substance A, with a half-life of 20 minutes, will have gone through 4 half-lives, decaying to 1/16 of its original amount, meaning 15/16 have decayed. Substance B, with a half-life of 40 minutes, will have gone through 2 half-lives, decaying to 1/4 of its original amount, meaning 3/4 have decayed. The ratio of decayed nuclei for A to B is therefore (15/16): (3/4), which simplifies to 5: 4.
Answer: t = T log 1.3 / log 2
With N_A = N0 e^(-lt) and N_B = N0(1 - e^(-lt)), N_B/N_A = e^(lt) - 1 = 0.3, so lt = ln(1.3). Since l = ln2/T, t = T ln(1.3)/ln(2) = T log(1.3)/log(2).
Answer: 20 days and 5 days
Activity R = lambda*N. R_A = lambda_A*N_A = 10 and N_A = 2*N_B, so lambda_A*N_B = 5. R_B = lambda_B*N_B = 20. Thus lambda_B/lambda_A = 20/5 = 4, and since T is inversely proportional to lambda, T_A = 4*T_B. Only 20 days and 5 days satisfies this.
Answer: t = T log 1.3 / log 2
The correct option is derived from the relationship between the decay of nucleus A and the formation of nucleus B, where the ratio of B to A can be expressed in terms of the half-life and logarithmic functions. By applying the decay formula and rearranging it to solve for time t, we find that t is proportional to the logarithm of the ratio of the quantities, specifically log(1.3) over log(2), which reflects the exponential nature of radioactive decay.
Answer: 20 years and 5 years, respectively
From A = lambda*N: lambda1 = A1/N1 = 5/(2N2) and lambda2 = A2/N2 = 10/N2, so lambda1/lambda2 = 1/4. Since T = ln2/lambda, T1/T2 = lambda2/lambda1 = 4, giving T1 = 20 years and T2 = 5 years.
Answer: 10⁻⁶
The nucleus typically has much higher energy levels compared to the atomic energy levels, leading to the emission of photons with significantly shorter wavelengths during de-excitation. This results in a ratio of wavelengths, λ_N/λ_A, that is very small, approximately 10⁻⁶.
Answer: 3: 2
The ratio of the velocities of the two nuclei is inversely related to the square root of their masses, and since the masses are proportional to the cube of their radii (for spherical shapes), we can derive the ratio of the radii from the velocity ratio. Thus, if the velocities are in the ratio of 8:27, the ratio of the radii will be the square root of the inverse of that ratio, leading to a ratio of 3:2.
Answer: 5 litres
The correct option is 5 litres because the activity measured in the blood after 10 hours, combined with the known decay constant and initial activity, allows us to calculate the total volume of blood in the body. Using the decay formula and the given activity, we find that the total blood volume corresponds to 5 litres.
Answer: (0.89, 0.28)
In an elastic collision, the fractional loss of energy depends on the mass of the target nucleus. Deuterium, being a light nucleus, results in a higher fractional energy loss for the neutron compared to carbon, which is heavier and thus absorbs less energy in the collision.
Answer: ln 2 / 4
The ratio of activities decaying as e⁻³t indicates that the decay constant of substance B is three times that of substance A. Since the half-life is inversely related to the decay constant, if A has a half-life of ln 2, B's half-life must be ln 2 divided by 3, which simplifies to ln 2 / 4.
Q48. The ratio of mass densities of nuclei of 40Ca and 16O is close to -
Answer: 1
Nuclear density rho = m/V with R proportional to A^(1/3), so density is essentially constant for all nuclei. The ratio for Ca-40 to O-16 is ~1.
Answer: 1/9λ
N_A/N_B = e^(-10*lambda*t)/e^(-lambda*t) = e^(-9*lambda*t). Setting this to 1/e gives 9*lambda*t = 1, so t = 1/(9*lambda).
Answer: 60 MW
Atoms = (2000 g / 235) * 6.023e23 = 5.13e24. Energy = 5.13e24 * 200e6 * 1.6e-19 = 1.64e14 J. Time = 30*86400 = 2.59e6 s. Power = 1.64e14 / 2.59e6 = 6.3e7 W ~ 63 MW, closest to 60 MW.