We know,
where R = Rydberg constant, Z = atomic number Here, n 1 = 1, n 2 = 5
=
According to conservation of linear momentum, we get Momentum of photon = Momentum of atom
= mv v =
=
=
We know,
where R = Rydberg constant, Z = atomic number Here, n 1 = 1, n 2 = 5
=
According to conservation of linear momentum, we get Momentum of photon = Momentum of atom
= mv v =
=
=
Nuclear radius, R = R 0 A 1/3 where R 0 is a constant and A is the mass number
=
R Cu =
=
= 4.8 fermi
In first case, n 1 = 3 and n 2 = 4
=
In second case, n 1 = 2 and n 2 = 3
=
=
=
KE max = 10eV = 2.75 eV Total incident energy E = + KE max = 12.75 eV Energy is released when electron jumps from the excited state n to the ground state.
E 4 – E 1 = {– 0.85 – (–13.6) ev} = 12.75eV value of n = 4
Initially P = 4N 0 Q = N 0 Half life T P = 1 min.
T Q = 2 min.
Let after time t number of nuclei of P and Q are equal, that is N P = N Q
=
t = 4 min After 4 minutes, both P and Q have equal number of nuclei. Number of nuclei of R =
+
=
E n =
E 1 = –13.6 eV E 2 = –3.4 eV E 3 = –1.5 eV E 4 = –0.85 eV E 3 – E 2 = –1.5 – (–3.4) = 1.9 eV E 4 – E 3 = –0.85 – (–1.5) = 0.65 eV Obviously, difference of 11.1 eV is not possible.
Extremely high temperature needed for fusion make kinetic energy large enough to overcome coulomb repulsion between nuclei.
-particle is 2 He 4 In emission, the neutron gets converted to proton and electron n X m
n - 2 Y m - 4
n Z m - 4
Momentum Mu =
Recoil energy :
=
=
=
From Einstein relation, E = mc 2 Rearranging, m =
We see that mass decay per second :
=
×
=
Now mass decay of U 235 per hour, =
60 60 =
3600 = 4 × 10 –8 kg = 40 microgram