Verify the three Q values reported for the reactions given in Fig. 43-11.The needed atomic and particle masses are

H1e1.007825uH4e4.002603uH22.014102ue±0.0005486uH3e3.016029u

(Hint: Distinguish carefully between atomic and nuclear masses, and take the positrons properly into account.)

Short Answer

Expert verified

All the energy values are verified.

Step by step solution

01

Describe the expression for energy

The expression for energy is given by,

Q=-mc2

Here, Qis the energy released in a reaction, mis the mass difference between the parent nuclei and the daughter nuclei, and is the velocity of light.

02

Verify the three Q values reported for the reactions

Consider the first reaction.

H1+H12H+e++v

The energy equation can be written as follows.

Q1=2mp-md-me+c2

Here,mp is the mass of the proton,md is the mass of deuteron, andme+ is the mass of positron.

Rewrite the equation as follows.

role="math" localid="1661923054546" Q1=2m1H-me+-m2H-me+-me+c2=2m1H-m2H-2me+c2......1

Substitute all the known values in equation (1).

Q1=21.007825u-2.014102u-20.0005486u931.5MeV/u=0.41984568MeV0.42MeV

Therefore, the energy released is 0.42MeV.

Consider the second reaction.

H2+H13He+y

The energy equation can be written as follows.

Q2=m2H+m1H-m3Hec2.....2

Substitute all the known values in equation (2).

Q2=2.014102u+1.007825u-3.016029u931.5MeV/u=5.493987MeV5.49MeV

Therefore, the energy released is5.49MeV .

Consider the third reaction.

H3e+H3e4He+=+1H+1H

The energy equation can be written as follows.

Q3=2m3He-m4He-2m1Hc2......3

Substitute all the known values in equation (3).

Q3=23.016029u-4.002603u-1.007825u931.5MeV/u=12.8593575MeV12.86MeV

Therefore, the energy released is 12.86MeV.

Therefore, all the energy values are verified.

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Most popular questions from this chapter

Calculate and compare the energy released by (a) the fusion of1.0 kg of hydrogen deep within the Sun and (b) the fission of 1.0 kgofU235in a fission reactor.

At the center of the Sun, the density of the gas is1.5×105kg/m3 and the composition is essentially 35% hydrogen by mass and 65% helium by mass. (a) What is the number density of protons there? (b) What is the ratio of that proton density to the density of particles in an ideal gas at standard temperature (0°C) and pressure(1.01×105Pa) ?

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In Fig. 43-10, the equation for n(K), the number density per unit energy for particles, n(K)=1.13nK1/2(kT)3/2e-KkTiswhere nis the total particle number density. At the center of the Sun, the temperature is1.50×107Kand the average proton energyKavgis 1.94 keV. Find the ratio of the proton number density at 5.00keVto the number density at the average proton energy.

Question: In a particular fission event in which U235is fissioned by slow neutrons, no neutron is emitted and one of the primary fission fragments is Ge83. (a) What is the other fragment? The disintegration energy is Q = 170 MeV. How much of this energy goes to (b) the Ge83fragment and (c) the other fragment? Just after the fission, what is the speed of (d) the Ge83fragment and (e) the other fragment?

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