Q.The Q value of a nuclear reaction A+b→C+d is defined by Q=[mA+mb−mC−md]c2 where the masses refer to the respective nuclei. Determine from the given data the Q-value of the following reactions and state whether the reactions are exothermic or endothermic.
Atomic masses are given to be
m(12H)=2.014102 u,
m(13H)=3.016049 u,
m(612C)=12.000000 u,
m(1020Ne)=19.992439 u.
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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Nuclear Reaction Balancing
Nuclear Reaction Balancing: The Intuition
Think of a nuclear reaction like a game of atomic Lego. You start with a certain set of blocks (the reactants), and after the reaction, you end up with a different set of blocks (the products). The fundamental rule is: you cannot lose or gain any Lego pieces. You can rearrange them, break some apart, or fuse them together, but the total number of each type of piece must stay the same.
In the atomic world, the "pieces" are:
- Protons (positive charge, found in the nucleus)
- Neutrons (neutral charge, also in the nucleus)
- Energy (which can appear or disappear, but that's a separate story)
The nucleus of an atom is made of protons and neutrons. When a nuclear reaction happens, the nuclei change. But the total number of protons and the total number of neutrons must be conserved — they cannot be created or destroyed.
This is different from chemical reactions, where atoms themselves are conserved. In nuclear reactions, atoms can change into different elements, but the nucleons (protons + neutrons) are conserved.
The Precise Statement
A nuclear reaction is balanced when two quantities are equal on both sides of the reaction arrow:
- Mass number (A) — the total number of nucleons (protons + neutrons). This is the superscript number.
- Atomic number (Z) — the total number of protons. This is the subscript number.
For any nuclear reaction:
Reactant1+Reactant2→Product1+Product2+…
The balancing conditions are:
∑Areactants=∑Aproducts
∑Zreactants=∑Zproducts
Nuclear Reaction Balancing Rules
Total mass number (A) on left=Total mass number (A) on right
Total atomic number (Z) on left=Total atomic number (Z) on right
How to Write a Nuclear Equation
Every nuclear particle is written as:
ZAX
Where:
- X = chemical symbol of the element
- A = mass number (top left)
- Z = atomic number (bottom left)
Common particles you'll encounter:
| Particle | Symbol | A | Z |
|---|---|---|---|
| Alpha particle | α or 24He | 4 | 2 |
| Beta particle | β− or −10e | 0 | -1 |
| Gamma ray | γ or 00γ | 0 | 0 |
| Neutron | n or 01n | 1 | 0 |
| Proton | p or 11p | 1 | 1 |
| Positron | β+ or +10e | 0 | +1 |
A common mistake: forgetting that beta particles have Z=−1 (for β−) or Z=+1 (for β+). This is because a neutron turns into a proton (or vice versa), and the beta particle carries away the "missing" charge.
Worked Example
Problem: Balance the following alpha decay reaction:
92238U→90234Th+?
Step 1: Identify what's missing. We have an unknown particle on the right.
Step 2: Balance mass numbers (A).
Left: A=238
Right: A=234+Aunknown
So 238=234+Aunknown⟹Aunknown=4
Step 3: Balance atomic numbers (Z).
Left: Z=92
Right: Z=90+Zunknown …
Why this formula?
Why Nuclear Reaction Balancing Works
Nuclear reaction balancing rests on a single, non-negotiable principle: conservation laws are absolute. In every nuclear reaction — whether natural decay, artificial transmutation, or fission/fusion — two quantities never change:
- Total mass number (A) — the sum of protons + neutrons
- Total atomic number (Z) — the sum of protons
These aren't arbitrary rules. They follow from deeper physics: baryon number conservation (protons and neutrons are baryons, and their total count is fixed) and charge conservation (electric charge cannot be created or destroyed). A nuclear reaction is just a rearrangement of nucleons; the number of nucleons stays constant, and the total charge stays constant.
For a reaction Z1A1X+Z2A2Y→Z3A3W+Z4A4Z:
A1+A2=A3+A4
Z1+Z2=Z3+Z4
The Reasoning Behind Each Conservation Law
Mass number conservation (A conserved):
A nucleon (proton or neutron) can change identity — a neutron can beta-decay into a proton, or a proton can capture an electron and become a neutron — but it cannot vanish or appear from nothing. The total count of nucleons before the reaction equals the total count after. This is why, for example, in alpha decay:
92238U→90234Th+24He
The left side has A=238; the right side has 234+4=238. The alpha particle carries away exactly 4 nucleons.
Atomic number conservation (Z conserved):
Charge is strictly conserved. The total positive charge (proton count) before equals the total after. In the same alpha decay, Z goes from 92 to 90+2=92. If charge weren't conserved, atoms would spontaneously change their chemical identity — which never happens in a closed system.
A common mistake is to think mass number conservation means mass is conserved. It does not. Mass-energy is conserved, but the rest mass can change (and usually does, releasing energy). The mass number A is a count of nucleons, not a measure of mass in kilograms.
How to Apply It: A Worked Example
Suppose you see: 92235U+01n→56141Ba+??Kr+301n
You know the total A on the left: 235+1=236.
On the right, you have 141+AKr+3(1)=144+AKr. …
Concept: Nuclear Reaction Balancing — the Q-value tells us whether energy is released (exothermic, Q>0) or absorbed (endothermic, Q<0).
Step 1 – Reaction (i):
11H+13H→12H+12H
Mass of 11H is 1.007825 u (proton mass, standard value).
Q=[1.007825+3.016049−2×2.014102]c2
=[4.023874−4.028204]c2=(−0.004330 u)c2
Using 1 u=931.5 MeV/c2,
Q=−0.004330×931.5≈−4.03 MeV.
Step 2 – Reaction (ii):
612C+612C→1020Ne+24He …
- Q=−4.03 MeV — endothermic;
- Q=+4.62 MeV — exothermic.
For each reaction, Q=[∑mreactants−∑mproducts]×931.5 MeV. A positive Q means energy is released (exothermic); a negative Q means energy is absorbed (endothermic). Besides the masses listed in the question, the two standard atomic masses m(11H)=1.007825 u and m(24He)=4.002603 u are used.
(i) 11H+13H→12H+12H
Δm=[m(11H)+m(13H)]−2m(12H)
Δm=(1.007825+3.016049)−2(2.014102)=4.023874−4.028204=−0.004330 u.
Q=(−0.004330)(931.5)=−4.03 MeV.
Since Q<0, the reaction is endothermic.
(ii) 612C+612C→1020Ne+24He
Δm=2m(612C)−[m(1020Ne)+m(24He)] …
Method: Mass-Energy Balance (Q-value calculation using atomic masses)
The Q-value tells you how much energy is released or absorbed in a nuclear reaction. The sign of Q decides whether the reaction is exothermic (energy released, Q > 0) or endothermic (energy absorbed, Q < 0).
Steps for any reaction:
- Write the reaction in the form A+b→C+d.
- Identify the masses of all reactants and products from the given data. If a mass is not directly given, check if it can be inferred (here all are given).
- Compute the mass difference: Δm=(mA+mb)−(mC+md).
- Multiply by c2 to get Q. In atomic mass units, 1 u⋅c2=931.5 MeV.
- If Q > 0, the reaction is exothermic. If Q < 0, it is endothermic.
(i) 11H+13H→12H+12H
Masses:
- m(11H) is not directly given. But note: 11H is a proton. Its mass is not the same as the atomic mass of hydrogen-1 (which includes one electron). However, in nuclear reaction balancing using atomic masses, the electron masses cancel if the number of electrons is the same on both sides. Let’s check: Left side: 1 electron (from H-1) + 1 electron (from H-3) = 2 electrons. Right side: 1 electron (from H-2) + 1 electron (from H-2) = 2 electrons. So electron masses cancel. We can use the given atomic masses directly.
But we still need m(11H). It is the atomic mass of hydrogen-1, which is 1.007825 u (standard value). Since the problem does not provide it, we must use the standard value. (If the problem expected you to compute without it, they would have given it — but here it's missing. We proceed with the known value.)
m(11H)=1.007825 u
m(13H)=3.016049 u
m(12H)=2.014102 u (each)
Mass of reactants: 1.007825+3.016049=4.023874 u
Mass of products: 2×2.014102=4.028204 u
Mass difference: Δm=4.023874−4.028204=−0.004330 u
Q = Δm⋅c2=−0.004330×931.5 MeV≈−4.03 MeV
Since Q < 0, the reaction is endothermic. …
Common Mistakes in Nuclear Reaction Q-Value Problems
Mistake 1: Using nuclear masses when only atomic masses are given
The formula uses nuclear masses, but the data gives atomic masses (which include electrons). For reactions where the number of electrons is conserved, atomic masses can be used directly — but students often forget to check this.
How to avoid: Count the electrons on each side. In reaction (i):
Left side: 1 electron (from 11H) + 1 electron (from 13H) = 2 electrons
Right side: 1 electron (from 12H) + 1 electron (from 12H) = 2 electrons
Electron count is balanced, so atomic masses work directly.
For reaction (ii):
Left: 6 + 6 = 12 electrons
Right: 10 + 2 = 12 electrons
Again balanced. So no correction needed here — but always verify.
If the electron count is not balanced, you must subtract the electron masses from the atomic masses to get nuclear masses, or add/subtract the appropriate number of electron masses to the Q-value.
Mistake 2: Forgetting to convert atomic mass units (u) to energy
The Q-value formula gives mass difference in u. To get energy in MeV, you must multiply by 931.5 MeV/c2 (or equivalently, c2=931.5 MeV/u).
How to avoid: Always write the conversion explicitly:
Q=(Δm in u)×931.5 MeV/u
Mistake 3: Sign error in the Q-value formula
Students sometimes write Q=[mC+md−mA−mb]c2 (reversed sign). This flips exothermic/endothermic classification.
How to avoid: Remember:
Q>0 means exothermic (energy released) — the products have less mass than the reactants.
Q<0 means endothermic (energy absorbed) — products have more mass.
The given formula Q=[mA+mb−mC−md]c2 is correct: reactants minus products.
Mistake 4: Arithmetic errors with precise mass values
The masses are given to 6 decimal places. A small subtraction error changes the sign or magnitude significantly.
How to avoid: Work systematically. For reaction (i):
Reactants: m(11H)+m(13H)
We need m(11H) — it's not given directly! This is a trap.
The mass of 11H (protium) is approximately 1.007825 u (standard value). But since it's not in the given data, you must use the standard value or note that the problem expects you to know it.
Using standard values:
m(11H)=1.007825 u
m(13H)=3.016049 u
Sum = 4.023874 u …
- AP EAPCET 2026Set eng-2026-05-13-FN1 markMCQQ.Binding energy per nucleon of deuteron and Helium nuclei are 1.1 MeV and 7 MeV respectively. If a single Helium nucleus was formed by adding two Deuterons, the energy released is (A) 23.6 MeV (B) 32.4 MeV (C) 28.6 MeV (D) 13.6 MeV
›Reveal solutionSolution
This tests fusion energetics via total binding energy (not BE per nucleon directly). Two deuterons fusing to helium release 23.6 MeV — this is exactly the classic D-D fusion energy release figure.
Concept and Intuition
Binding energy per nucleon measures how tightly bound, on average, each nucleon is. To get the total binding energy of a nucleus you must multiply by the mass number A (the total nucleon count), because binding energy is an extensive (whole-nucleus) quantity while BE/nucleon is an intensive (per-particle) one. When lighter nuclei fuse into a more tightly-bound heavier nucleus, the difference in total binding energy is released as energy (mass converts to energy per E=mc2, already baked into the BE values).
Step-by-Step Solution
- Deuteron (12H) has mass number A=2 and BE/nucleon =1.1 MeV. Total BE of one deuteron =2×1.1=2.2 MeV.
- Two deuterons together carry total BE =2×2.2=4.4 MeV.
- Helium (24He) has mass number A=4 and BE/nucleon =7 MeV. …
- AP EAPCET 2026Set eng-2026-05-15-AN1 markMCQQ.During the decay of an unstable nucleus, if its neutron number and mass number decrease by 5 and 12 respectively, then the particles released in the decay are (A) One alpha particle and six positrons (B) One alpha particle and six electrons (C) Three alpha particles and one positron (D) Three alpha particles and one electron
›Reveal solutionSolution
Matching the mass-number and neutron-number decreases uniquely picks three α particles plus one positron.
Concept and Intuition
An α particle (24He) removes 2 protons and 2 neutrons, so it always changes A by −4, Z by −2, N by −2. A β− (electron) emission converts a neutron to a proton: Z by +1, N by −1, A unchanged. A β+ (positron) emission does the reverse: Z by −1, N by +1, A unchanged. We're told the overall changes are N down by 5 and A down by 12, so ΔZdecrease=ΔA−ΔN=12−5=7.
Step-by-Step Solution
- Only α particles change A, each by −4. To get a total A decrease of 12 we need exactly 3 α particles.
- Three α particles alone give a Z decrease of 6 and an N decrease of 6.
- We still need one more unit of Z-decrease (to reach 7) while N's decrease must come back up from 6 to 5 (i.e., N needs +1 relative to the 3-alpha result).
- A positron emission does exactly that: Z decreases by 1 more (reaching 7 total) and N increases by 1 (bringing the N-decrease from 6 down to 5). …
- AP EAPCET 2025Set ap-2025-05-19-FN1 markMCQQ.The equation for 10Ne23 nucleus which decays by β-emission is (A) 10Ne23β-decay10Ne22+νˉ+e+ (B) 10Ne23β-decay10Ne23+ν+e− (C) 10Ne23β-decay11Na22+e−+νˉ (D) 10Ne23β-decay11Na23+e−+νˉ
›Reveal solutionSolution
This tests the mass/charge bookkeeping of β−-decay. In β−-decay a neutron becomes a proton, so Z increases by 1 while A is unchanged; the correct daughter is 11Na23.
Concept and Intuition
In β− (negatron) decay, one neutron inside the nucleus transforms into a proton, emitting an electron (e−) and an electron-antineutrino (νˉ):
n→p+e−+νˉ
Since a neutron is replaced by a proton, the mass number A stays the same but the atomic number Z increases by 1. The daughter nucleus therefore sits one place to the right in the periodic table.
Step-by-Step Solution
- Parent nucleus: 10Ne23 (Z = 10, A = 23).
- β−-decay converts one neutron to a proton: Z→Z+1=11, A unchanged =23.
- Element with Z = 11 is sodium (Na). So the daughter is 11Na23.
- Conservation of charge and lepton number requires the emitted particles to be e− and νˉ (not a positron, which would occur in β+-decay and would decrease Z).
- Full equation: 10Ne23→11Na23+e−+νˉ.
Common Mistakes …
- AP EAPCET 2025Set eng-2025-05-27-FN1 markMCQQ.If the binding energy per nucleon of deuteron (1H2) is 1.15 MeV and an α-particle has a binding energy of 7.1 MeV per nucleon, then the energy released per nucleon in the given reaction is 1H2+1H2→2He4+Q (A) 23.8 MeV (B) 26.1 MeV (C) 5.95 MeV (D) 28.9 MeV
›Reveal solutionSolution
This tests binding-energy bookkeeping for a fusion reaction; the total Q is 23.8 MeV, which works out to 5.95 MeV per nucleon.
Concept and Intuition
In any nuclear reaction, the energy released equals the increase in total binding energy: reactants with less total binding energy fuse into a product with more total binding energy, and the difference is released as Q. Binding energy per nucleon must first be converted to total binding energy (multiply by mass number) before adding/subtracting, since binding energy is an extensive (additive) quantity, not per-nucleon directly comparable across different nuclei.
Step-by-Step Solution
- Each deuteron 1H2 has mass number 2 and BE/nucleon =1.15MeV, so total BE per deuteron =2×1.15=2.3MeV.
- Two deuterons together: total initial BE =2×2.3=4.6MeV.
- The product 2He4 has mass number 4 and BE/nucleon =7.1MeV, so total BE =4×7.1=28.4MeV. …
- AP EAPCET 2023Set ap-2023-05-22-AN1 markMCQQ.Among the following the possible nuclear reaction is (A) 510B+24He→713N+11H (B) 1124Na+01n→1020Ne+24He (C) 93239Np→94239Pu+e−+υˉ (D) 711N+11H→612C+e−+υˉ
›Reveal solutionSolution
A nuclear reaction is physically possible only if both mass number and atomic number balance on both sides; checking each option, only the Np-239 → Pu-239 beta decay balances.
Concept and Intuition
Every nuclear reaction must independently conserve total mass number A (nucleon count) and total charge/atomic number Z on both sides of the arrow (along with energy/momentum, but those aren't testable from the symbolic equation alone). This is a quick, purely bookkeeping check that instantly rules out fabricated-looking reactions.
Step-by-Step Solution
- Option (A): A: 10+4=14, 13+1=14 — matches. Z: 5+2=7, but 7+1=8 — mismatch. Not possible as written (correct version would emit a neutron, not a proton).
- Option (B): A: 24+1=25 vs 20+4=24 — mismatch. Not possible.
- Option (C): A: 239 vs 239+0+0=239 — matches. Z: 93 vs 94+(−1)+0=93 — matches. This is the well-known genuine β− decay 93239Np→94239Pu+e−+υˉ. …
- AP EAPCET 2023Set eng-2023-05-18-FN1 markMCQQ.A radioactive decay forms an isotope of the original nucleus with the emission of the following particles (A) one α- and four β- particles (B) one α- and one β- particles (C) one α- and two β- particles (D) four α- and one β- particles
›Reveal solutionSolution
Restoring the original atomic number (needed for an isotope) after one α decay requires exactly two β− decays to compensate.
Concept and Intuition
An isotope of the original nucleus has the same atomic number Z (same element) but generally a different mass number A. In radioactive decay: an α particle emission reduces Z by 2 and A by 4; a β− particle emission (electron emission, a neutron converting to a proton) increases Z by 1 while leaving A unchanged.
Step-by-Step Solution
- Let the decay chain involve nα alpha particles and nβ beta particles.
- Net change in atomic number: ΔZ=−2nα+nβ.
- For the final nucleus to be an isotope (same Z, so ΔZ=0, but with A reduced due to the alpha decays, so genuinely a different isotope, not the identical nuclide): nβ=2nα. …
- AP EAPCET 2022Set ap-2022-07-11-AN1 markMCQQ.Consider a radioactive isotope 92U238 decays into 82Pb206 in a series by emission of nα number of alpha particles and nβ number of beta particles. Then the values of nα and nβ? (A) nα=8, nβ=8 (B) nα=6, nβ=6 (C) nα=8, nβ=6 (D) nα=6, nβ=8
›Reveal solutionSolution
This tests radioactive-decay-series bookkeeping: the mass-number drop fixes the alpha count, and the atomic-number drop (after accounting for the alphas) fixes the beta count. Answer: nα=8, nβ=6.
Concept and Intuition
In a decay series, mass number (A) changes only because of α-emission — each α is a 24He nucleus, so it reduces A by 4. β−-emission (an electron ejected when a neutron converts to a proton inside the nucleus) changes Z but leaves A unchanged. So the total mass-number drop alone tells us how many alphas were emitted; once that is known, the atomic-number drop tells us how many betas were needed to make the numbers balance.
Step-by-Step Solution
- Mass-number change: 238−206=32. Since each α reduces A by 4: nα=32/4=8.
- Atomic-number change: 92−82=10 (a net decrease of 10 over the whole series). …
- AP EAPCET 2022Set eng-2022-07-07-FN1 markMCQQ.The correct statement of the following is (A) The Q – value of a nuclear process is the difference between final and initial kinetic energies. (B) The nuclear mass is always higher than the total mass of its constituents (C) Nuclides with same number of neutrons in the nucleus are known as isotopes. (D) In nuclear fusion, a heavy nucleus breaks into two smaller fragments.
›Reveal solutionSolution
This tests precise nuclear-physics vocabulary: Q-value, mass defect, isotopes/isotones, and fission vs fusion. Only the Q-value statement (A) is accurate.
Concept and Intuition
Nuclear reactions release or absorb energy according to the mass difference between reactants and products (Q=Δmc2). Equivalently, since total energy is conserved, this same Q shows up as the difference between the total kinetic energy carried away by the products and the total kinetic energy the reactants had — this equivalence is exactly what statement (A) states. The other statements test whether you can distinguish related-but-different ideas: mass defect (binding energy) vs. constituent mass, isotopes vs. isotones, and fission vs. fusion.
Step-by-Step Solution
- (A) By definition, Q=(KE of products)−(KE of reactants), which equals [∑mreactants−∑mproducts]c2. This is the standard textbook definition — true.
- (B) Because of the mass defect (binding energy), a nucleus's mass is always less than the sum of the masses of its free constituent nucleons, not higher — false.
- (C) Nuclides with the same number of protons (atomic number Z) are isotopes; nuclides with the same number of neutrons are isotones. The statement swaps these — false. …
- AP EAPCET 2021Set ap-2021-09-03-FN1 markMCQQ.The binding energy per nucleon of 3Li7 and 2He4 nuclei are 5.60 MeV and 7.06 MeV, respectively. Then, in the nuclear reaction 3Li7+1H1⟶2He4+2He4+Q, the value of Q, the energy released, is (A) 19.6 MeV (B) −2.4 MeV (C) 8.4 MeV (D) 17.3 MeV
›Reveal solutionSolution
This tests computing the Q-value of a nuclear reaction from binding energies per nucleon, using Q=(total BE of products)−(total BE of reactants). The answer is 17.3 MeV.
Concept and Intuition
In a nuclear reaction, the energy released, Q, equals the increase in total binding energy going from reactants to products — because a more tightly bound (higher total BE) final configuration corresponds to a lower rest-mass total, and that mass difference is released as kinetic energy/radiation by E=mc2. So instead of tracking individual masses, we can directly use Q=∑(BE)products−∑(BE)reactants, taking care to multiply each binding energy per nucleon by the number of nucleons in that nucleus to get the total binding energy.
Step-by-Step Solution
- Reaction: 3Li7+1H1→2He4+2He4+Q.
- Total BE of 3Li7 (7 nucleons, 5.60 MeV/nucleon): 7×5.60=39.2 MeV.
- Total BE of 1H1: a single proton has no binding energy (there's nothing to bind to itself), so BE =0. …
- AP EAPCET 2021Set eng-2021-08-20-AN1 markMCQQ.Which of the following nuclear reactions is possible? (A) 5B10+2He4⟶7N13+1H1 (B) 11Na24+1H1⟶10Ne20+2He4 (C) 93Np239⟶94Pu239+β−+γ− (D) 7N11+1H1⟶6C12+β−+γ−
›Reveal solutionSolution
A real nuclear reaction must conserve both mass number (A) and charge/atomic number (Z) on both sides; only option (C) does.
Concept and Intuition
In any nuclear reaction (or decay), the total mass number A (nucleons) and the total charge Z (protons, counting β− as charge −1 and mass number 0, and γ as carrying neither charge nor mass number) must each be conserved separately. Checking these two simple bookkeeping sums is the fastest way to spot an impossible reaction.
Step-by-Step Solution
- (A) 5B10+2He4→7N13+1H1: mass numbers 10+4=14=13+1 ✓, but charges 5+2=7 on the left vs 7+1=8 on the right ✗ — charge not conserved, impossible as written (the real reaction actually produces a neutron, 7N13+0n1).
- (B) 11Na24+1H1→10Ne20+2He4: charges 11+1=12=10+2 ✓, but mass numbers 24+1=25=20+4=24 ✗ — mass number not conserved, impossible. …
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