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A 12.5 eV electron beam is used to bombard gaseous hydrogen at room temperature. What series of wavelengths will be emitted?

In ground state, energy of gaseous hydrogen at room temperature = – 13.6 eV.

Energy of electron beam used to bombard the gaseous hydrogen = 12.5 eV 

Therefore, after bombardment,
Energy of gaseous hydrogen = –13.6 + 12.6
                                           = – 1.1 eV.

Since, En = -13.6n2       
 So,          n2 = -13.6-1.1 = 12.3        n  = 3 

That is, the electron would jump from n = 1 to n = 3, where E3 = -13.632 = -1.5 eV. 
On de-excitation, the electron may jump from n = 3 to n = 2 giving rise to Balmer series.

It may also jump from n = 3 to n = 1, giving rise to Lyman series. 


So, number of spectral line is,

= n(n-1)2 = 3(3-1)2 = 3 

Thus, three spectral lines appear.

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In accordance with the Bohr's model, find the quantum number that characterises the earth's revolution around the sun in an orbit of radius 1.5 × 1011 m with orbital speed 3 × 104m/s. (Mass of earth = 6.0 × 1024 kg.)

Given, 
Radius of the orbit, r = 1.5 × 1011 m 
Orbital speed, v = 3 × 104m/s. 
Mass of the earth, m = 6.0 × 1024 kg

Now, according to Bohr's theory
                   mvr = nh2π 

or,                   n= 2π mvrh 
                    

                       
                         = 2.56 × 1074.
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A hydrogen atom initially in the ground level absorbs a photon, which excites it to the n = 4 level. Determine the wavelength and frequency of photon.


Initially, hydrogen is in the ground state. 
After absorption of photon Hydrogen atom excited to level, n=4.

Energy of an electron in n
th orbit of H atom is, 

                                  En = -13.6n2eVwhen n=1;           E1 = -13.6 eV 

Energy in 4th (n = 4) level 

                  E4 = -13.642 = -0.85
             E = E4-E1

                                                       E = -0.85 - (-13.6) eV                                             = -0.85 + 13.6                                 E =12.75 eV  Now, energy of a photon = hνTherefore,                                     hv  = 12.75 eV                                 hv = 12.75 × 1.6 × 10-19J                                   v = 12.75×1.6×10-196.6 ×10-34i.e.,                                v = 3.078 ×1015 Hz, is the required frequency of the photon.Now, wavelength of photon is ,                                       λ = cλ = 3 × 1083.078 × 1015i.e.,                               λ = 974.4 Å
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(a) Using the Bohr's model calculate the speed of the electron in a hydrogen atom in the n = 1, 2, and 3 levels. (b) Calculate the orbital period in each of these levels.

(a) From the relation, 

v = cnα,      where   α = 2π Ke2ch = 0.0073

Therefore, the speed of electron in hydrogen atom in n=1, 2 and 3 is given by, 
                    v1 = 3×1081×0.0073 = 2.19×106 m/sv2 = 3×1082×0.0073 = 1.095 ×106 m/sv3 =3×1083×0.0073 =7.3×105 m/s.

(b) Orbital period in each of the level is given by, 

T = 2πrv  As  r1 = 0.53×10-10m  

T1 = 2π×0.53×10-102.19×106= 1.52×10-16s ' 

As,  r2 = 4 r1    and   v2  = 12v1 

         T2 =  8 T1      = 8 × 1.52 × 10-16s      = 1.216 × 10-15s 

Also as, r3 = 9 r1   and  v3 = 13v1 
 T3 = 27 T1 = 27 × 1.52 × 10-16s                      = 4.1 × 10-15 s. 

T1, T2 and T3 are respectively the orbital time period for n1, nand n3

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Answer the following questions, which help you understand the difference between Thomson's model and Rutherford's model better.
Is the average angle of deflection of α-particles by a thin gold foil predicted by Thomson's model much less, about the same, or much greater than that predicted by Rutherford's model?

The average angle of deflection of α-particles by a thin gold foil predicted by Thomson's model is about the same as predicted by Rutherford. 
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