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6 months ago

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V
Vishal Baghel

Contributor-Level 10

4.24

(a) Despite being a scalar quantity, energy is not conserved in elastic collisions. False

(b) Despite being a scalar quantity, the temperature can take negative values. False

(c) The total path length is a scalar quantity. Yet it has the dimension of length. False

(d) A scalar quantity such as gravitational potential can vary from one point to another point in space. False

(e) The value of a scalar does not vary for observers with different orientation of axis. True

New answer posted

6 months ago

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V
Vishal Baghel

Contributor-Level 10

4.23

(a) For any arbitrary motion of a particle average velocity cannot be expressed by this equation. False

 

(b) The arbitrary motion of the particle can be represented by this equation, True

 

(c) For arbitrary motion of the particle, the acceleration may also be non uniform. False

 

(d) The motion of the particle is arbitrary, acceleration of the particle may also be non-uniform, so can not represent the motion of the particle in space. False

 

(e) The arbitrary motion of the particle can be represented by the given equation. True

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Payal Gupta

Contributor-Level 10

13.14 Let the atomic mass of a substance be = M and the density of the substance be = ?

Avogadro's number, N = 6.023 *1023

Volume of N number of molecules =43? r3N ……. (i)

Volume of one mole of a substance =M?  …… (ii)

Equating (i) and (ii), we get

43? r3N=M?

New answer posted

6 months ago

13.13 A gas in equilibrium has uniform density and pressure throughout its volume. This is strictly true only if there are no external influences. A gas column under gravity, for example, does not have uniform density (and pressure). As you might expect, its density decreases with height. The precise dependence is given by the so-called law of atmospheres

n2 = n1 exp [ -mg (h2h1)/ kBT]

where n2, n1 refer to number density at heights h2 and h1 respectively. Use this relation to derive the equation for sedimentation equilibrium of a suspension in a liquid column:

n2 = n1 exp [ -mg NA ( ρ - ρ' ) (h2h1)/ ( ρ RT)]

where ρ is

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Payal Gupta

Contributor-Level 10

13.13 According to law of atmospheres, we have

n2 = n1 exp [ -mg (h2h1)/ kBT] ….(i)

where n1 is the number of density at height  h1and n2 is the number of density at height h2

mg is the weight of the particle suspended in the gas column

Density of the medium = ?

Density of the suspended particle = ?'

Mass of one suspended particle = m'

Mass of medium displaced = m

Volume of the suspended particle = V

According to Archimedes's principle for a particle suspended in a liquid column, the effective weight of the suspended particle is given as:

Weight of the medium displaced – weight of the suspended particle = mg – m'g

= mg- V ?'g = mg –

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6 months ago

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P
Payal Gupta

Contributor-Level 10

13.12 Rate of diffusion of hydrogen, R1= 28.7 cm3 s–1

Rate of diffusion of another gas, R2 = 7.2 cm3 s–1

According to Graham's law of diffusion, we have:

 R1R2= M2M1, where M1= molecular mass of hydrogen = 2.02 g and M2 is the molecular mass of the unknown gas

M2=M1* (R1R2)2= 2.02* (28.77.2)2= 32.09 = Molecular mass of Oxygen

Hence, the unknown gas is Oxygen.

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6 months ago

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Payal Gupta

Contributor-Level 10

13.11 Length of the narrow bore, L = 1 m = 100 cm

Length of the mercury thread, l = 76 cm

Length of the air column between mercury and the closed end, lo  = 15 cm

Since the bore is held vertically in air with the open end at the bottom, the mercury length that occupies the air space is 100 – (76 + 15) = 9 cm

Hence, total length of the air column = 15 + 9 = 24 cm

Let h cm of mercury flow out as a result of atmospheric pressure.

Length of the air column in the bore = 24 + h cm

Length of the mercury column = 76 – h cm

Initial pressure,  P1 = 76 cm of mercury

Initial volume, V1= 15 cm3

Final pressure, P2 = 76 – (76 – h) = h cm

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Payal Gupta

Contributor-Level 10

13.10 Pressure inside the cylinder containing nitrogen, P = 2.0 atm = 2 *1.013*105 Pa

Temperature inside the cylinder, T = 17 ?=290K

Radius of nitrogen molecule, r = 1.0 Å = 1 *10-10 m

Diameter of nitrogen molecule, d = 2 *10-10 m

Molecular mass of nitrogen molecule, M = 28 u = 28 g (assume) = 28 *10-3 kg

The root means square speed of nitrogen is given by the relation

R is the universal gas constant = 8.314 J/mole/K

Hence 

The mean free path l is given by

l ?=kT?2?d2P where k = Boltzmann constant = 1.38*10-23 kg-m2s-2K-1 

l?=1.38*10-23*290?2?(2*10-10)2*2*1.013*105= 1.11*10-7  m

Collision frequency = Vrmsl? = 508.261.11*10-7= 4.57 109 /s

Collision time, T = dVrms  =2*10-10508.26S= 3.93 *10-13 s

T

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Payal Gupta

Contributor-Level 10

13.9 Temperature of the helium atom, THe = – 20 °C = 253 K and temperature of argon atom be = TAr

Atomic mass of helium, MHe = 4.0 u

Atomic mass of Argon, MAr = 39.9 u

Let VrmsAr be the rms speed of Argon and VrmsHe be the rms speed of Helium

From the relation of Vrms=3kTM we get

rms speed of Argon, VrmsAr=3kTArMAr

rms speed of Helium, VrmsHe=3kTHeMHe

Since both the speeds are equal, we get

3kTArMAr = 3kTHeMHe or TArMAr = THeMHe or TAr = THe*MArMHe = 253*39.94 = 2523.675 K = 2.523 *103 K

New answer posted

6 months ago

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P
Payal Gupta

Contributor-Level 10

13.8  (a) According to Avogadro's law, the three vessels will contain an equal number of the respective molecules. This number is equal to Avogadro's number, N = 6.023 *1023

(b) The root mean square speed ( Vrms) of a gas of mass m and temperature T is given by the relation Vrms=3kTm . Where k is Boltzmann constant. For the given gases, k and T are constants. Hence Vrms depends only on the mass of the atoms

Therefore, the root mean square speed of the molecules in the three cases is not the same. Among Neon, Chlorine and Uranium hexafluoride, the mass of the neon is the smallest, so Neon will have the highest root mean square sp

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6 months ago

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P
Payal Gupta

Contributor-Level 10

13.7 (i) At room temperature, T = 27 ? = 300 K

kB is Boltzmann constant = 1.38 *10-23 m2kgs-2K-1

Average thermal energy = 32kBT = 3*1.38*10-23*3002 = 6.21 *10-21 J

Hence, the average thermal energy of a helium atom at room temperature is 6.21 *10-21 J

(ii) On the surface of the Sun, T = 6000 K

Hence average thermal energy = 32kBT = 3*1.38*10-23*60002 = 1.242 *10-19 J

Hence, the average thermal energy of a helium atom on the surface of the Sun is 1.242 *10-19 J

(iii) Inside the core of a star, T = 107 K

Hence average thermal energy = 32kBT = 3*1.38*10-23*1072 = 2.07 *10-16 J

Hence, the average thermal energy of a helium atom

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