This document discusses concepts related to the gas laws including:
1. Definitions of key terms like pressure, volume, temperature, moles, and the gas constant R.
2. Equations relating these variables like the ideal gas law PV=nRT and how pressure, volume, and temperature are directly proportional while temperature and moles are directly proportional.
3. Explanations of how the gas laws can be used to calculate heat, work, internal energy, and other thermodynamic properties of gases.
Solution manual for water resources engineering 3rd edition - david a. chinSalehkhanovic
Solution Manual for Water-Resources Engineering - 3rd Edition
Author(s) : David A. Chin
This solution manual include all problems (Chapters 1 to 17) of textbook. in second section of solution manual, Problems answered using mathcad software .
THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
2. – F ˆ F www.schoolDD.com 1
10
10.1 F
F ˈ ˂
F ˈ F F (Q) F ˈ (J)
- F 1 (= 4.186 J ) F F 1
1° C
10.1.1
ˈ F F
F F F F F
F F F
10.2.1 F F
F F ˈ F F F F F
F F F F F
F F F
1. (° C)
2. (K) ˈ F F F F F F F ( ˈ F
SI)
F
C =
R = F
F = F
K =
100
F F
0
° CK
373.16
273.16
K = C + 273
۱
=
܀
=
۴ି
ૢ
3. – F ˆ F www.schoolDD.com 2
10.1.2 F
1. F ( C ) F F
ˈ F F ˈ F (J/K)
2. F ( c ) F F 1 F
ˈ F F ˈ F (J/kg K)
F F F F F m ΔT F F
Q = F (J)
m = (kg)
c = F (J/kg K)
ΔT = (K ˚C)
- F ( C ) F F F C F C F
- F ( c ) F F ˈ
F c (J/kg K)
(-10˚C 0˚C)
4186
2100
900
450
390
140
130
m
∆Q
〉 ∆T
C =
ઢۿ
ઢ܂
m
∆Q
〉 ∆T
c =
ઢۿ
ܕઢ܂
Q = mc∆T
4. – F ˆ F www.schoolDD.com 3
F 1 F F 100 25˚C ( c = 390
J/kg K)
. ˈ 45 ˚C
. ˈ 15 ˚C
. F F F F F
Q = mc∆T
= 0.10x390x(45-25)
Q = 780 J Ans
. F F F
Q = mc∆T
= 0.10x390x(25-15)
Q = 390 J Ans
10.1.4 F
F F F F
F F F
F
- ˈ F
F F F F F F F
10.1.5 F
3
F F F F F
F F
F F F F F
F F F F F
F F F F F F F F F
F F ˂
s
5. – F ˆ F www.schoolDD.com 4
F F
F F m F F F
Q = F (J)
m = (kg)
L = F (J/kg)
F
Lm (J/kg)
F
ˈ Lv (J/kg)
333x103
2256x103
58.6x103
452x103
5.23x103
20.9x103
F 2 F F 200 -10˚ C ˈ
F ˈ F 190 ( c = 2100 J/kg K, c =
4186 J/kg K, Lm = 333x103
J/kg, Lv = 2256x103
J/kg )
“ F F ˈ
F F F F ˇ F F ”
F
F
F
F
Q = mL
200 g
-10° C
Q1
200 g
0° C
200 g
0° C
200 g
100° C
190 g + 10 g
100° C
Q2 Q3 Q4
6. – F ˆ F www.schoolDD.com 5
F F 200 g -10° C ˈ 0° C
Q1 = mc∆T
= 0.2x2100x(0-(-10))
Q1 = 4200 J
F F 200 g 0° C ˈ 0° C
Q2 = mL
= 0.2x333x103
Q2 = 66600 J
F F 200 g 0° C ˈ 100° C
Q3 = mc∆T
= 0.2x4186x(100-0)
Q3 = 83720 J
F F 10 g 100° C ˈ 10 g 100° C
Q4 = mL
= 0.01x2256x103
Q4 = 22560 J
F Q = Q1 + Q2 + Q3 + Q4
= 4200 + 66600 + 83720 + 22560
Q = 177080 J Ans
F 3
100 100˚ C F F F ˈ
90˚ C (c = 4186 J/kg K, Lv = 2256x103
J/kg)
F 100 g 100° C F ˈ 100 g 100° C
Q1 = mLv
= 0.1x2256x103
(L = L F )
Q1 = 225600 J
F 100 g 100° C ˈ 100 g 90° C
Q2 = mc∆T
= 0.1x4186x(100-90)
Q2 = 4186 J
F F Q = Q1 + Q2
= 225600 + 4186
Q = 229786 J Ans
100 g
100° C
100 g
100° C
Q1
100 g
90° C
Q2
“ F”
7. – F ˆ F www.schoolDD.com 6
F 4
F F 1 20 ˚C F ˈ -10 ˚C F
F F (c = 2100 J/kg K, c = 4186 J/kg K, Lm = 333x103
J/kg)
F 1 kg 20° C ˈ 1 kg 0° C
Q1 = mc∆T
= 1.0x4186x(20-0)
Q1 = 83720 J
F 1 kg 0° C ˈ 1 kg 0° C
Q2 = mLm
= 1.0x333x103
(L = L )
Q2 = 333000 J
F 1 kg 0° C ˈ 1 kg -10° C
Q3 = mc∆T
= 1.0x2100x(0-(-10))
Q3 = 21000 J
F F Q = Q1 + Q2 + Q3
= 83720 + 333000 + 21000
Q = 437720 J Ans
10.1.6 F
F F F F
F F F F
F F F F
F = F F
F 5
F 200 F F 300˚ C F 1 20
˚C F F ˈ F ( c = 500 J/kg K, c = 4200 J/kg )
1 kg
20° C
1 kg
0° C
Q1
1 kg
0° C
Q3
1 kg
-10° C
Q2
Q = Q Q = Q
“ F”
8. – F ˆ F www.schoolDD.com 7
Q = Q
(mc∆T) = (mc∆T)
F F ˈ t° C 20 < t ≤100
F F 0.2x500x(300- t) = 1.0x4200x(t-20)
30000 - 100 t = 4200t – 84000
114000 = 4300t
t = 26.5° C Ans ( )
F 6
F 5 F F ˈ 2 ˈ 0.5
F ˈ F
Q = Q
(mc∆T) = (mc∆T)
F F ˈ t° C 20 < t ≤100
F F 2.0x500x(300- t) = 0.5x4200x(t-20)
30000 - 100 t = 2100t – 42000
342000 = 3100t
t = 110.3° C > 100° C F ˈ F ˈ
F ˈ 100° C F F
1 kg
20° C Q
1 kg
t° CQ
0.2 kg
300° C
Q
0.2 kg
t° CQ t ≤ 100° C F ˈ
t = 300° C F
100° C ˈ F
0.5 kg
20° C Q
0.5 kg
t° CQ
2 kg
300° C
Q
2 kg
t° CQ t ≤ 100° C F ˈ
t = 300° C F
100° C ˈ F
0.5 kg
20° C Q 1
0.5 kg
100° C
Q
2 kg
300° C
Q
2 kg
100° CQ
+
100° CQ 2
9. – F ˆ F www.schoolDD.com 8
ˈ F F
Q = Q
(mc∆T) = (mc∆T) 1 + (mL) 2
F F 2.0x500x(300-100) = 0.5x4200x(100-20) + mx2256x103
32000 = 2256x103
m = 0.014 kg
ˈ 0.014 kg 100° C F F 0.5 0.014 = 0.486 kg 100° C Ans
F 7
˄ 1 2 20˚ C F F F 1
200 ˚C F ˈ F ( c = 1000 J/kg K, c
= 4200 J/kg c = 400 J/kg K )
Q = Q
(mc∆T) = (mc∆T) ˄ + (mc∆T)
F F ˈ t° C 20 < t ≤100
F F 1.0x400x(200- t) = 1.0x1000x(t-20) + 2.0x4200x(t-20)
80000 - 400 t = 1000t – 20000 + 8400 t - 168000
268000 = 9800t
t = 27.35° C Ans ( )
F 8
F 200 1 30 ˚C F 100
0 ˚C F ( c F = 800 J/kg K, c = 4200 J/kg K,
L = 333x103
J/kg )
2 kg
20° C Q
2 kg
t° C
Q
1kg
200° C
Q
1kg
t° CQ
20 < t ≤ 100° C F ˈ
˄ 1 kg
20° C
˄ 1 kg
t° CQ ˁ
10. – F ˆ F www.schoolDD.com 9
Q = Q
(mc∆T) + (mc∆T) F = (mL) + (mc∆T)
F F ˈ t° C 0 < t < 30
F F 1.0x4200x(30- t) + 0.2x800x(30- t) = 0.1x333x103
+ 0.1x4200x(t-0)
4360x(30- t) = 33300 + 420t
97500 = 4780t
t = 20.4° C Ans ( )
F 9
F 1 100 ˚C F 200 F
ˈ F ( c = 500 J/kg K, c = 4200 J/kg K, L = 333x103
J/kg )
Q = Q
(mc∆T) = (mL) + (mc∆T)
F F ˈ t° C 0 < t < 100
F F 1.0x500x(100- t) = 0.2x333x103
+ 0.2x4200x(t-0)
50000 - 500t = 66600 + 840t
-16600 = 1340t
1 kg
30° C Q
1 kg
t° C
Q
0.1 kg
0° C
Q
0.1 kg
0° C
Q 0 < t < 30° C
F 0.2 kg
30° C
F 0.2 kg
t° CQ F
Q
0.1 kg
t° C
1 kg
100° C Q
1 kg
t° C
Q
0.2 kg
0° C
Q
0.2 kg
0° C
Q
0 < t < 100° C
Q
0.2 kg
t° C
11. – F ˆ F www.schoolDD.com 10
t = -12.39° C F ˈ F F ˈ 0° C
ˈ F
F F
Q = Q
(mc∆T) = (mL)
F F 1.0x500x(100- 0) = mx333x103
50000 = 333x103
m
m = 0.15 kg = 150 g < 200 g OK
F F ˈ 0° C 0.15 kg Ans
10.1.7 F F
3
1. F
- F F F ˈ F F F
F F F
2. F
- F F ˈ F F F
F F F F F F F
F F F F F
3. F F
- F F F F F F F
F ˂
1 kg
100° C Q
1 kg
0° C
Q
0.2 kg
0° C
Q
+
0° C
Q
12. – F ˆ F www.schoolDD.com 11
10.2 F
- F F F F F F
F ˈ F
10.2.1 F
F ʽ F F
10.2.2 F
F ʽ F F
10.2.3 F
F F F
V ן
= F
F
V ן
۾
P
1
V
T
PV = F
V ן T
V
T
P
= F
۾܄
܂
=
۾܄
܂
F F F
1 2 (T F )
F F P, V F F = F F F F T
F ˈ K F
13. – F ˆ F www.schoolDD.com 12
F
ן n n = F =
୫
F
n =
ۼۯ
F 1 F 6.02x1023
F PV =
ۼۯ
RT
F F KB =
ୖ
ۼۯ
= F F F =
଼.ଷଵ
.ଶ୶ଵమయ
= 1.38x10-23
J/K
F PV = NKB T
PV = nRT PV = NKB T F F F F
F ˆ F F F
1. F PV = nRT
2. F F F P ן T, P ן n, V ן T, V ן n P ן
ଵ
F
3. F F F F F 1 2 F F F
F F
భభ
୬భభ
= R
మమ
୬మమ
= R
భభ
୬భభ
=
మమ
୬మమ
(P F ˈ P F )
F F
PV = nRT
ˈ F
R = F F = 8.31 J/mol K
. F
= 6.02 x 1023
F
1
۾܄
ܖ܂
=
۾܄
ܖ܂
F F F 1 2
F (T F )
14. – F ˆ F www.schoolDD.com 13
F 10
F 1 F 2 x 105
Pa 7˚ C F F F F
2 F F ˈ F
F PV = nRT
F F 2
భభ
୬భభ
=
మమ
୬మమ
P n
F
భ
భ
=
మ
మ
ଵ
ଶ଼
=
ଶ
మ
T2 = 560 K 560 273 = 287° C Ans
F 11
F F 105
Pa F 27˚ C ˈ -3˚ C ˈ
F
F PV = nRT
F F 2
భభ
୬భభ
=
మమ
୬మమ
V n
V1 = 1 m3
P1 = 2x105
Pa
T1 = 273+7 = 280 K
n1
V2 = 2 m3
P2 = P1
T2 = ?
n2 = n1
V1
P1 = 2x105
Pa
T1 = 273+27= 300 K
n1
V2 = V1
P2 = ?
T2 = 273+(-3) = 270 K
n2 = n1
15. – F ˆ F www.schoolDD.com 14
F
భ
భ
=
మ
మ
ଵఱ
ଷ
=
మ
ଶ
P2 = 0.9x105
Pa Ans
F 12
F F F 17˚ C F 2 x 105
Pa F
F ˈ 27˚ C F ˈ F (
=105
Pa)
F PV = nRT
F F 2
భభ
୬భభ
=
మమ
୬మమ
V n
F
భ
భ
=
మ
మ
ሺౝశ ౌబሻభ
భ
=
ሺౝశ ౌబሻమ
మ
F P F F ˈ P F F
ଶ୶ଵఱାଵఱ
ଶଽ
=
ౝమାଵఱ
ଷ
Pg 2 = 2.09x105
Pa Ans
F 13
F 10 27˚ C 105
Pa F
F
V1
Pg1 = 2x105
Pa
T1 = 273+17= 290 K
n1
V2 = V1
Pg2 = ?
T2 = 273+27 = 300 K
n2 = n1
16. – F ˆ F www.schoolDD.com 15
F PV = nRT
F F F F
F F 105
(10x10-3
) = n (8.31)(300) 1 = 1000 cc = 1000 cm3
= 1000(10-6
m3
) = 10-3
m3
n = 103
/ 2493 = 0.4 Ans
n =
୫
m = nM
= 0.4x2.0x10-3
m = 8.0x10-4
kg Ans
F 14
F 50 F 10 27˚ C
F F F F 5 17˚ C F F F
( R = 8.31 J/mol K, MN2 = 28 g/mol, 1 atm = 105
Pa )
. n1 F F P1 V1 = n1RT1
10x105
x50x10-3
= n1x8.31x300
n1 = 20
. n2 F F P2 V2 = n2RT2
5x105
x50x10-3
= n2x8.31x290
n2 = 10.4
F F F n1 n2 = 20 10.4 = 9.6 9.6x28x10-3
= 0.27 kg Ans
V = 10
P = 105
Pa
T = 273+27 = 300 K
n = ?
m = ?
V1 = 50x10-3
m3
P1 = 10 atm
T1 = 273+27 = 300 K
n1 = ?
V2 = 50x10-3
m3
P2 = 5 atm
T2 = 273+17 = 290 K
n2 = ?
17. – F ˆ F www.schoolDD.com 16
F 15
F 64 27˚ C 20 F F
F ( R = 8.31 J/mol K, MO2 = 28 g/mol )
P F F PV = nRT
Px20x10-3
=
ସ
ଷଶ
x8.31x300 n =
୫
P = 2.493x105
Pa Ans
F 16
F 1 1.3 0˚ C 1
13 10 27˚ C
F PV = nRT
F F 2
భభ
୬భభ
=
మమ
୬మమ
F n =
୫
M
F
భభ
୫భభ
=
మమ
୫మమ
ଵ୶ଵ
ଵ.ଷ୶ଶଷ
=
మ୶ଵ
ଵଷ୶ଷ
P2 = 1.10 atm Ans
m = 64 g
T = 273+27 = 300 K
V = 20x10-3
m3
P = ?
V1 = 1
m1 = 1.3 g
T1 = 273+0 = 273 K
P1 = 1 atm
V2 = 10
m2 = 13 g
T2 = 273+27 = 300 K
P2 = ?
18. – F ˆ F www.schoolDD.com 17
F 17
F F F F
ˈ F
F PV = nRT
F F 2
భభ
୬భభ
=
మమ
୬మమ
F V T
F
భ
୬భ
=
మ
୬మ
భ
୬భ
=
భ
మ
భ
୬మ
n2 = ½ n1 Ans
F 18
F F 10 kg/m3
27˚ C 2 F F
F 17˚ C 1 F F F
F PV = nRT
F F 2
భభ
୬భభ
=
మమ
୬మమ
F n =
୫
M
V1
P1
T1
n1
V2 = V1
P2 = ½ P1
T2 = T1
n2 = ?
V1
T1 = 273+27 = 300 K
P1 = 2 atm
ߩ1 = 10 kg/m3
V2 = V1
T2 = 273+17 = 290 K
P2 = 1 atm
ߩ2 = ?
19. – F ˆ F www.schoolDD.com 18
F
భభ
୫భభ
=
మమ
୫మమ
భ
ౣభ
భ
భ
=
మ
ౣమ
మ
మ
భ
ఘభభ
=
మ
ఘమమ
ଶ
ଵ୶ଷ
=
ଵ
ఘమ୶ଶଽ
ߩଶ = 5.17 kg/m3
Ans
10.3 F F
10.3.1 F
F
1. F F F ˈ
F F F
2. F F ˈ F
3. F ˈ F F F
10.3.2 F ( < EK > )
F F < EK > ˈ F F
1 F ˈ (J)
F F N F N< EK >
N< EK > =
ଷ
ଶ
NKB T
=
ଷ
ଶ
PV ( PV = NKB T )
=
ଷ
ଶ
nRT ( PV = nRT )
- < EK > F F F F F
< EK > =
KB T
20. – F ˆ F www.schoolDD.com 19
10.3.3 F
F F F vrms (vroot mean square )
F ˈ F (m/s)
- vrms F T M
- vrms F F (v) F F F
F 19
F 20 27˚ C ( R = 8.31 J/mol K, MH2 = 2 g/mol )
. F F
. F F
. vrms F
. < EK > = ?
< EK > =
ଷ
ଶ
KB T KB =
ୖ
ఽ
=
଼.ଷଵ
.ଶ୶ଵమయ
= 1.38x10-23
=
ଷ
ଶ
x 1.38x10-23
x300
< EK > = 6.21x10-25
J Ans
. N< EK > = ?
. N N = n NA
=
୫
=
ଶ
ଶ
x 6.02x1023
N = 6.02x1024
N< EK > = 6.02x1024
x 6.21x10-25
= 3.73 J Ans
vrms = ට
܂܀
ۻ
M = F 1 (kg)
m = 20 g
T = 273+27 = 300 K
21. – F ˆ F www.schoolDD.com 20
. vrms = ?
vrms = ට
ଷୖ
= ට
ଷ୶଼.ଷଵ୶ଷ
ଶ௫ଵషయ
= √3739500
vrms = 1933.78 m/s Ans
F 20
F F F 3 10 2 Pa
. N N = n NA = 3x6.02x1023
F F N< EK > =
ଷ
ଶ
NKBT =
ଷ
ଶ
PV ( PV = NKBT)
=
ଷ
ଶ
x2x10x10-3
N< EK > = 3x10-2
J Ans
F < EK > < EK > =
ଷ୶ଵషమ
=
ଷ୶ଵషమ
ଷ୶.ଶ୶ଵమయ
< EK > = 1.66x10-26
J Ans
F 21
F F 2x 1025
F F 105
Pa
F F
F < EK > < EK > =
ଷ
ଶ
KBT
F N< EK > = ଷ
ଶ
NKBT =
ଷ
ଶ
PV ( PV = NKBT)
< EK > = ଷ
ଶ
= ଷ
ଶ
x
ଵ୶ଵఱ
ଶ୶ଵమఱ
< EK > = 7.5x10-21
J Ans
n = 3
V = 10 = 10x10-3
m3
P = 2 Pa
N<EK> = ?
<EK> = ?
N/V = 2x1025
/m3
P = 1x105
Pa
<EK> = ?
22. – F ˆ F www.schoolDD.com 21
F 22
F
. F F ˈ 2 F F ˈ F
. F F ˈ 2 F F ˈ F
.
< EK > =
ଷ
ଶ
KBT
F < EK > ן T
ழாేభவ
ழாేమவ
=
భ
మ
=
భ
ଶభ
< EK2 > = 2< EK1 > Ans
.
< EK > =
ଷ
ଶ
KBT
N< EK > = ଷ
ଶ
NKBT =
ଷ
ଶ
PV
F < EK > ן P N V
ழாేభவ
ழாేమவ
=
భ
మ
=
భ
ଶభ
< EK2 > = 2< EK1 > Ans
F 23
F A 1 7˚ C F B 2 27˚ C
F F ˈ F ( R = 8.31 J/mol K )
T1
<EK1>
T2 = 2 T1
<EK2> = ?
V1
P1
N1
<EK1>
V2 = V1
P2 = 2 P1
N2 = N1
<EK2> = ?
A
nA = 1
TA = 273 + 7 = 280 K
<EKA>
B
nB = 2
TB = 273 + 27 = 300 K
<EKB>
+
23. – F ˆ F www.schoolDD.com 22
N< EK > N< EK > =
ଷ
ଶ
NKBT
=
ଷ
ଶ
nRT
(N< EK >)A + (N< EK >)B = (
ଷ
ଶ
nRT)A + (
ଷ
ଶ
nRT)B
=
ଷ
ଶ
R(nATA + nBTB)
=
ଷ
ଶ
x8.31(1x280 + 2x300)
F = 1.097x104
J Ans
F 24
F ˈ F F ( MH2 = 2 g/mol, MO2 =
32 g/mol)
vrms = ට
ଷୖ
F vrms ן
ଵ
√
T
୴౨ౣ౩ౄమ
୴౨ౣ౩ోమ
= ට
ోమ
ౄమ
= ට
ଷଶ
ଶ
= 4
vrmsH2 = 4 vrmsO2 Ans
F 25
F ʽ F F ˈ 4 F
vrms ˈ F
vrms = ට
ଷୖ
PV = nRT
F RT =
୬
vrms = ට
ଷ
୬
H2
vrmsH2 O2
vrmsO2
ߩଵ
vrms1
ߩଶ = 4ߩଵ
vrms2
24. – F ˆ F www.schoolDD.com 23
= ට
ଷ
ఘ
୬
=
୫
= ߩ
F vrms ן
ଵ
ඥఘ
P
୴౨ౣ౩భ
୴౨ౣ౩మ
= ට
ఘమ
ఘభ
= ට
ସఘభ
ఘభ
= 2
vrms2 = 2 vrms1 Ans
10.4
-
- F F F F F
F U F F
F F ˈ F F F
F F F F F F F
F F
F F F U =
ଷ
ଶ
NKBT
=
ଷ
ଶ
nRT
=
ଷ
ଶ
PV
10.4.1 F 1 F F
F F F F
U = N< EK >
〉 ∆Q
〉 ∆U
〉 ∆W
∆Q = ∆U + ∆W
ΔW = FΔs
= PAΔs
= PΔV
25. – F ˆ F www.schoolDD.com 24
∆Q
F F F +
F -
∆U
+
-
∆W
+
F -
F 26
F F F 1000 J F F F 200 J F
F F F
∆Q = ∆U + ∆W
1000 = 200 + ∆W
∆W = 800
F F = 800 J ( ∆W ˈ + ) Ans
F 27
F 1024
F F F F 1˚ C F F F F F F
(KB = 1.38x10-23
)
∆Q = ∆U + ∆W
=
ଷ
ଶ
NKB∆T + P∆V
=
ଷ
ଶ
x1024
x1.38x10-23
x1 + 0
∆Q = 20.7
F F F F F ∆Q = 20.7 J Ans (∆Q ˈ + )
〉 ∆Q = 1000 J
〉 ∆U = 200 J
∆W = ?
〉 ∆Q = ?
N = 1024
∆T = 1
∆V = 0
26. – F ˆ F www.schoolDD.com 25
F 28
100 N F 1 F 1 K
F F F F 20 cm. ( R = 8.31 J/mol K )
∆Q = ∆U + ∆W
=
ଷ
ଶ
nR∆T + (-F∆s) ( F ˈ )
=
ଷ
ଶ
x1x8.31x1 – 100x0.20
∆Q = -7.5 ( ˈ F )
F ∆Q = 7.5 J Ans
F 29
F F F F F F F
∆Q = ∆U + ∆W
=
ଷ
ଶ
NKB∆T + P∆V
=
ଷ
ଶ
P∆V + P∆V ( PV = NKBT)
∆Q =
ହ
ଶ
P∆V
F F F F F ∆Q = ହ
ଶ
P∆V J Ans
n = 1
∆T = 1 K
∆Q = ?
F = 100 N
0.20
〉 ∆Q = ?
P
∆V
∆W
∆U
27. – F ˆ F www.schoolDD.com 26
F 30
F F F 20 27˚ C 105
Pa F
ˈ 57˚ C F F F F F F
V2 F
భభ
୬భభ
=
మమ
୬మమ
P n
F
భ
భ
=
మ
మ
ଶ
ଷ
=
మ
ଷଷ
V2 = 22
∆Q = ∆U + ∆W
=
ଷ
ଶ
NKB∆T + P∆V
=
ଷ
ଶ
P∆V + P∆V ( PV = NKBT)
=
ହ
ଶ
P∆V =
ହ
ଶ
x105
x(22-2)x10-3
∆Q = 500
F F F F F ∆Q = 500 J Ans
〉 ∆Q = ?
V1 = 20
T1 = 273 + 27 = 300 K
P1 = 105
Pa
V2 = ?
T2 = 273 + 57 = 330 K
P2 = P1
∆W
∆U