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New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

According to de-Broglie's hypothesis

λ = h m v p = m v = h λ K = p 2 2 m = h 2 2 m λ 2

Cut-off wavelength of emitted X-ray = h c K = h c * 2 m λ 2 h 2 = 2 m c λ 2 h

New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

Energy of electron in first existed state will be -3.4 eV.

So total energy difference will be (2.6 + 3.4) eV.

Wavelength ( λ ) = 1 2 4 2 e V n m 6 e V = 2 0 7 n m

F r e q u e n c y = c λ = 3 * 1 0 8 2 0 7 * 1 0 9 = 1 . 4 5 * 1 0 9 M H z

 

New answer posted

2 months ago

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A
alok kumar singh

Contributor-Level 10

No. of different wavelengths

= n * ( n 1 ) 2 = 6 * 5 2 = 1 5

New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

h f 1 = R ( 1 1 2 1 3 2 ) = R * 8 9

h f 2 = R ( 1 1 2 1 2 2 ) = R * 3 4

f 1 f 2 = 8 / 9 3 / 4 = 3 2 2 7

f2 = fx ( 2 7 3 2 )

= ( 2 . 9 2 * 1 0 1 5 ) * ( 2 7 3 2 )

= 2 . 4 6 * 1 0 1 5 H z

New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

  v z n

  v = k z n [K constant]

for 3rd orbit of He+

v H e + = k * 2 3 = 2 k 3  - (1)

v H = k * 1 3 = k 3  - (2)

v H e + v H = 2 : 1

New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

We know

Energy on any orbit is given by,

E n = 1 3 . 6 n 2 z 2

  E 1 = 1 3 . 6 1 2 * 9 [n1 = 1] (1)

For 3rd orbit

E 3 = 1 3 . 6 9 *   [n2 = 3]

E3 = 13.6ev

Δ E = E 3 E 1

= 13.6 – (13.6 * 9)

Δ E = 8 * 1 3 . 6 e v = p h o t o n e n e r g y

8 * 1 3 . 6 e v = h c λ

8 * 1 3 . 6 e v = 1 2 4 2 e v λ n m

λ = 1 1 . 4 1 5 * 1 0 9

= 114.15 * 1010m

New answer posted

2 months ago

0 Follower 2 Views

V
Vishal Baghel

Contributor-Level 10

Given absorb energy = 10.2 eV

E f = 1 3 . 6 n 2 = 3 . 4

n 2 = 4

n = 2

 

New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

mvr = n h 2 π

So momentum (mv) = n h 2 π r

New answer posted

2 months ago

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V
Vishal Baghel

Contributor-Level 10

According to Rutherford, e- revolves around in nucleus in circular orbit. Thus e- is always accelerating (centripetal acceleration). An accelerating change emits EM radiation and thus e- should loose energy and finally should collapse in the nucleus.

New answer posted

2 months ago

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P
Payal Gupta

Contributor-Level 10

ΔE=13.6 (112152)=13.6*2425eV

hcλ=13.6*2425eV.......... (1)

With the help of conservation of linear momentum, we can write

hλ=mHvHhcλ=cmHvHvH=hcλcmH=13.6*2425*1.6*10193*108*1.67*1027=4.17m/s

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