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What is the binding energy per nucleon of the europium isotope E63152u? Here are some atomic masses and the neutron mass.

Eu63152151.921742uH11.007825un1.008665u

Short Answer

Expert verified

The binding energy per nucleon of the europium isotope is 8.23 MeV.

Step by step solution

01

Given data

The given isotope americium isE63152u .

The atomic mass unit of the isotope europium,MEu=151.921742u

The atomic mass of the hydrogen,MH=1.007825u

The atomic mass unit of neutron,Mn=1.008665u

02

Understanding the concept of binding energy  

The binding energy of an element is defined as the amount of energy required to separate a particle from a system of particles or to disperse all the particles of the system. It can simply also be stated as the product of mass defect with the square of the speed of light. This relation will give the required binding energy of the isotope europium. Now, using this value and dividing it by the number of nucleons of the isotope, we can get the binding energy per nucleon of the europium isotope.

Formulae:

The binding energy of an atom, โˆ†Ebe=ZMH+A-ZMn-Matomc2orโˆ†mc2ยทยทยทยทยทยทยทยท1

Where, Zis the atomic number (number of protons), Ais the mass number (number of nucleons), MHis the mass of a hydrogen atom, Mnis the mass of a neutron, and Matomis the mass of an atom. In principle, nuclear masses should be used, but the mass of the Zelectrons included in ZMHis canceled by the mass of the Zelectrons included in Matom, so the result is the same.

The binding energy per nucleon of an atom, โˆ†Ebe/nucleon=โˆ†Ebe/A.........(2)

03

Calculation of the binding energy per nucleon of europium

At first we can calculate the mass excess or the mass defect for the europium isotope with z = 63 using equation (1) as follows:

โˆ†m=631.007825u+152-631.008665u-151.921742u=1.342418u

Now, the binding energy can be calculated by converting the amu value of mass defect into as MeV considering equation (1) follows:

โˆ†Ebe=1.342418u931.5MeV/u=1250.454MeV

Thus, according to the concept the binding energy per nucleon of europium isotope with nucleon number A =152 as can be calculated using equation (2) as follows:

โˆ†Ebe/nucleon=1250.454MeV/152=8.23MeV

Hence, the required value of energy is 8.23 MeV.

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Most popular questions from this chapter

a. Show that the massMof an atom is given approximately by Mapp=Amp, whereAis the mass number and is the proton mass. For (b) 1H, (c)31P,(d)120Sn, (e) 197Au, and (f) 239Pu, use Table 42-1 to find the percentage deviation between Mappand M:

role="math" localid="1662047222746" percentagedeviation=Mapp-MMร—100

(g) Is a value ofMappaccurate enough to be used in a calculation of a nuclear binding energy?

At t=0, a sample of radionuclide Ahas the same decay rate as a sample of radionuclide Bhas at. The disintegration constants areฮปAandฮปB, withฮปA<ฮปB. Will the two samples ever have (simultaneously) the same decay rate? (Hint:Sketch a graph of their activities.)

The radionuclide32Pdecays toS32as described by Eq. 42-24. In a particular decay event, an1.71 MeVelectron is emitted, the maximum possible value. What is the kinetic energy of the recoilingS32atom in this event? (Hint:For the electron it is necessary to use the relativistic expressions for kinetic energy and linear momentum. TheS32atom is non-relativistic.)

If the unit for atomic mass were defined so that the mass of 1Hwere exactly 1.000 000 u, what would be the mass of(a) localid="1661600852143" 12C(actual mass 12. 000 000 u ) localid="1661600855467" 238Uand (b) (actual mass 238.050 785 u)?

The radionuclide C11decays according to

C11โ†’B11+e++v,T1/2=20.3

The maximum energy of the emitted positrons is 0.960 MeV. (a) Show that the disintegration energy Qfor this process is given by

role="math" localid="1661759171201" Q=(mC-mB-2me)c2

WheremCandmBare the atomic masses ofC11andB11, respectively, andmeis the mass of a positron. (b) Given the mass valuesmC=11.011434u,mB=11.009305uandme=0.0005486u, calculate Qand compare it with the maximum energy of the emitted positron given above. (Hint:LetmC andmBbe the nuclear masses and then add in enough electrons to use the atomic masses.)

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