Skip to main content
Top
Published in:
Cover of the book

2013 | OriginalPaper | Chapter

1. Aspects of Physical Chemistry

Author : Ian W. M. Smith

Published in: Astrochemistry and Astrobiology

Publisher: Springer Berlin Heidelberg

Activate our intelligent search to find suitable subject content or patents.

search-config
loading …

Abstract

Some of those topics in physical chemistry that are especially relevant to astrochemistry and astrobiology are introduced in this chapter. I start with some discussion of the chemical elements: their relative abundances, their electronic structure, and how chemical bonds are formed in simple molecules. This leads to a discussion of how changes between energy levels lead to molecular spectra that can be used to identify molecules at a distance – even the vast distances from Earth to astronomical objects. Having considered forces within molecules, I then discuss the weaker forces between molecules, including hydrogen bonding. The next section focuses on chemical reactions from both the standpoint of thermodynamics and that of chemical kinetics. Finally, some consideration is given to surface processes, which can occur on the dust particles found in the interstellar medium, and enzyme kinetics, which is of great importance in biology.

Dont have a licence yet? Then find out more about our products and how to get one now:

Springer Professional "Wirtschaft+Technik"

Online-Abonnement

Mit Springer Professional "Wirtschaft+Technik" erhalten Sie Zugriff auf:

  • über 102.000 Bücher
  • über 537 Zeitschriften

aus folgenden Fachgebieten:

  • Automobil + Motoren
  • Bauwesen + Immobilien
  • Business IT + Informatik
  • Elektrotechnik + Elektronik
  • Energie + Nachhaltigkeit
  • Finance + Banking
  • Management + Führung
  • Marketing + Vertrieb
  • Maschinenbau + Werkstoffe
  • Versicherung + Risiko

Jetzt Wissensvorsprung sichern!

Springer Professional "Technik"

Online-Abonnement

Mit Springer Professional "Technik" erhalten Sie Zugriff auf:

  • über 67.000 Bücher
  • über 390 Zeitschriften

aus folgenden Fachgebieten:

  • Automobil + Motoren
  • Bauwesen + Immobilien
  • Business IT + Informatik
  • Elektrotechnik + Elektronik
  • Energie + Nachhaltigkeit
  • Maschinenbau + Werkstoffe




 

Jetzt Wissensvorsprung sichern!

Springer Professional "Wirtschaft"

Online-Abonnement

Mit Springer Professional "Wirtschaft" erhalten Sie Zugriff auf:

  • über 67.000 Bücher
  • über 340 Zeitschriften

aus folgenden Fachgebieten:

  • Bauwesen + Immobilien
  • Business IT + Informatik
  • Finance + Banking
  • Management + Führung
  • Marketing + Vertrieb
  • Versicherung + Risiko




Jetzt Wissensvorsprung sichern!

Footnotes
1
The notation 2 1H specifies the number of protons, 1, and the number of nucleons (protons + neutrons), 2. Any electrically neutral atom contains the same number of electrons and protons. To refer to an ion, a superscript after the chemical symbol is added. Thus a deuteron is signified by 2 1H1+. The number of protons in an elemental atom corresponds to its atomic number, Z.
 
2
These elements, heavier than lithium, are all referred to by astronomers as ‘metals’ – somewhat to the amusement, or bemusement, of those trained as chemists.
 
3
This total does not include the isotopomers of several species that have also been observed.
 
4
By convention, the ‘forward’ reaction is that proceeding from left to right in the chemical equation, and the ‘reverse’ reaction is that proceeding from right to left.
 
5
Associated with each vibration in a molecule, there is ‘zero-point energy’ corresponding approximately to ½hv where v is the frequency of the vibration. Consequently, as shown in Fig. 1.2, the lowest vibrational energy level with the quantum number v = 0, has an energy ½hv above the minimum of the potential energy curve.
 
6
A catalyst accelerates the rate of reaction without changing the position of equilibrium and without itself being changed during the course of reaction. As the equilibrium constant is not changed, it means that any catalyst must accelerate the rates of forward and reverse reactions in equal proportions. The changes in rate occur because the catalyst lowers the Gibbs energies of activation for the forward and reverse reactions.
 
Literature
1.
go back to reference Atkins PW, de Paula J (2010) Physical chemistry, 9th edn. Oxford University Press, Oxford Atkins PW, de Paula J (2010) Physical chemistry, 9th edn. Oxford University Press, Oxford
2.
go back to reference Chang R (2005) Physical chemistry for the biosciences. University Science, Sausalito Chang R (2005) Physical chemistry for the biosciences. University Science, Sausalito
3.
go back to reference Greenwood NN, Earnshaw A (1997) Chemistry of the elements, 2nd edn. Butteworth-Heinemann, Oxford, Chaps. 1 and 2 Greenwood NN, Earnshaw A (1997) Chemistry of the elements, 2nd edn. Butteworth-Heinemann, Oxford, Chaps.​ 1 and 2
4.
go back to reference Cameron AGW (1973) Abundances of elements in solar system. Space Sci Rev 15:121–146CrossRef Cameron AGW (1973) Abundances of elements in solar system. Space Sci Rev 15:121–146CrossRef
5.
go back to reference Newson HE (1995) Composition of the solar system, planets, meteorites, and major terrestrial reservoirs. In: Ahrens TJ (ed) Global earth physics: a handbook of physical constants. American Geophysical Union, Washington, DC Newson HE (1995) Composition of the solar system, planets, meteorites, and major terrestrial reservoirs. In: Ahrens TJ (ed) Global earth physics: a handbook of physical constants. American Geophysical Union, Washington, DC
6.
go back to reference Duncan DL, Harvie JL, McKean DC, Cradock S (1986) The ground state structures of disilane, methyl silane and the silyl halides, and an SiH bond length correlation with stretching frequency. J Mol Struct 145:225–242CrossRef Duncan DL, Harvie JL, McKean DC, Cradock S (1986) The ground state structures of disilane, methyl silane and the silyl halides, and an SiH bond length correlation with stretching frequency. J Mol Struct 145:225–242CrossRef
7.
go back to reference Harmony MD (1990) The equilibrium carbon-carbon single bond length in ethane. J Chem Phys 93:7522–7523CrossRef Harmony MD (1990) The equilibrium carbon-carbon single bond length in ethane. J Chem Phys 93:7522–7523CrossRef
8.
go back to reference Bernath PF (1995) Spectra of atoms and molecules. Oxford University Press, Oxford Bernath PF (1995) Spectra of atoms and molecules. Oxford University Press, Oxford
9.
go back to reference Herbig GH (1995) The diffuse interstellar bands. Annu Rev Astron Astrophys 33:19–73CrossRef Herbig GH (1995) The diffuse interstellar bands. Annu Rev Astron Astrophys 33:19–73CrossRef
10.
go back to reference Jenniskens P, Désert F-X (1994) A survey of the diffuse interstellar bands (3800–8680 Å). Astron Astrophys Suppl Ser 106:39–78 Jenniskens P, Désert F-X (1994) A survey of the diffuse interstellar bands (3800–8680 Å). Astron Astrophys Suppl Ser 106:39–78
11.
go back to reference Wayne RP (2000) Chemistry of atmospheres. Oxford University Press, Oxford Wayne RP (2000) Chemistry of atmospheres. Oxford University Press, Oxford
12.
go back to reference McKellar A (1940) Evidence for the molecular origin of some hitherto unidentified interstellar lines. Publ Astronom Soc Pac 52:187; (b) Adams WS (1941) Some results with the Coudé spectrograph of the Mount Wilson observatory. Astrophys J 93:11; (c) Douglas AE, Herzberg G (1941) CH+ in interstellar space and in the laboratory. Astrophys J 94:381 McKellar A (1940) Evidence for the molecular origin of some hitherto unidentified interstellar lines. Publ Astronom Soc Pac 52:187; (b) Adams WS (1941) Some results with the Coudé spectrograph of the Mount Wilson observatory. Astrophys J 93:11; (c) Douglas AE, Herzberg G (1941) CH+ in interstellar space and in the laboratory. Astrophys J 94:381
13.
go back to reference Burgh EB, France K, McCandliss SR (2007) Direct measurement of the ratio of carbon monoxide to molecular hydrogen in the diffuse interstellar medium. Astrophys J 658:446CrossRef Burgh EB, France K, McCandliss SR (2007) Direct measurement of the ratio of carbon monoxide to molecular hydrogen in the diffuse interstellar medium. Astrophys J 658:446CrossRef
14.
go back to reference Wakelam V, Smith IWM, Herbst E, Troe J, Geppert W, Linnartz H et al (2010) Reaction networks for interstellar chemical modelling: improvements and challenges. Space Sci Rev 156:13–72CrossRef Wakelam V, Smith IWM, Herbst E, Troe J, Geppert W, Linnartz H et al (2010) Reaction networks for interstellar chemical modelling: improvements and challenges. Space Sci Rev 156:13–72CrossRef
15.
go back to reference Balle TJ, Flygare WH (1981) Fabry-Perot cavity pulsed Fourier-transform microwave spectrometer with a pulsed nozzle particle source. Rev Sci Instrum 52:33–45CrossRef Balle TJ, Flygare WH (1981) Fabry-Perot cavity pulsed Fourier-transform microwave spectrometer with a pulsed nozzle particle source. Rev Sci Instrum 52:33–45CrossRef
16.
go back to reference Thaddeus P, McCarthy MC, Travers MJ, Gottleib CA, Chen W (1998) New carbon chains in the laboratory and in interstellar space. Faraday Discuss 109:121–135CrossRef Thaddeus P, McCarthy MC, Travers MJ, Gottleib CA, Chen W (1998) New carbon chains in the laboratory and in interstellar space. Faraday Discuss 109:121–135CrossRef
17.
go back to reference Herbst E, van Dishoeck EF (2009) Complex organic interstellar molecules. Ann Rev Astron Astrophys 47:427–480CrossRef Herbst E, van Dishoeck EF (2009) Complex organic interstellar molecules. Ann Rev Astron Astrophys 47:427–480CrossRef
18.
go back to reference Peeters E (2011) Astronomical observations of the PAH emission bands. In: Joblin C, Tielens AGGM (eds) PAHs in the universe. EAS Publication Series 46:13–27 Peeters E (2011) Astronomical observations of the PAH emission bands. In: Joblin C, Tielens AGGM (eds) PAHs in the universe. EAS Publication Series 46:13–27
19.
go back to reference Rigby M, Smith EB, Wakeham WA, Maitland GC (1986) The forces between molecules. Clarendon, Oxford Rigby M, Smith EB, Wakeham WA, Maitland GC (1986) The forces between molecules. Clarendon, Oxford
20.
go back to reference Buckingham AD, Del Bene JE, McDowell SAC (2008) The hydrogen bond. Chem Phys Lett 463:1–10CrossRef Buckingham AD, Del Bene JE, McDowell SAC (2008) The hydrogen bond. Chem Phys Lett 463:1–10CrossRef
21.
go back to reference Smith IWM (1980) Kinetics and dynamics of elementary gas reactions. Butterworths, London Smith IWM (1980) Kinetics and dynamics of elementary gas reactions. Butterworths, London
22.
go back to reference Pilling MJ, Seakins PW (1995) Reaction kinetics. Oxford University Press, Oxford Pilling MJ, Seakins PW (1995) Reaction kinetics. Oxford University Press, Oxford
23.
go back to reference Georgievskii Y, Klippenstein SJ (2005) Long-range transition state theory. J Chem Phys 122:194103-1–194103-17CrossRef Georgievskii Y, Klippenstein SJ (2005) Long-range transition state theory. J Chem Phys 122:194103-1–194103-17CrossRef
24.
go back to reference Legon AC, Millen DJ (1987) Directional character, strength, and nature of the hydrogen bond in gas-phase dimers. Acc Chem Res 20:39–46CrossRef Legon AC, Millen DJ (1987) Directional character, strength, and nature of the hydrogen bond in gas-phase dimers. Acc Chem Res 20:39–46CrossRef
25.
go back to reference (a) Miller RE (1990) Vibrationally induced dynamics in hydrogen-bonded complexes. Acc Chem Res 23:10–16. (b) Nesbitt DJ (1988) High-resolution infrared-laser spectroscopy of weakly bound molecular complexes. Chem Rev 45:843–870 (a) Miller RE (1990) Vibrationally induced dynamics in hydrogen-bonded complexes. Acc Chem Res 23:10–16. (b) Nesbitt DJ (1988) High-resolution infrared-laser spectroscopy of weakly bound molecular complexes. Chem Rev 45:843–870
26.
27.
28.
go back to reference Smith IWM (2007) The temperature-dependence of elementary reaction rates: beyond Arrhenius. Chem Soc Rev 36:1–15CrossRef Smith IWM (2007) The temperature-dependence of elementary reaction rates: beyond Arrhenius. Chem Soc Rev 36:1–15CrossRef
30.
go back to reference Baulch DL, Bowman CT, Cobos CJ, Cox RA, Just Th, Kerr JA et al (2005) Evaluated kinetic data for combustion modelling: supplement II. J Phys Chem Ref Data 34:757–1397CrossRef Baulch DL, Bowman CT, Cobos CJ, Cox RA, Just Th, Kerr JA et al (2005) Evaluated kinetic data for combustion modelling: supplement II. J Phys Chem Ref Data 34:757–1397CrossRef
31.
go back to reference Smith IWM, Sage AM, Donahue NM, Herbst E, Quan D (2006) The temperature-dependence of rapid low temperature reactions: experiment and prediction. Faraday Discuss 133:137–156CrossRef Smith IWM, Sage AM, Donahue NM, Herbst E, Quan D (2006) The temperature-dependence of rapid low temperature reactions: experiment and prediction. Faraday Discuss 133:137–156CrossRef
32.
go back to reference McClelland BJ (1973) Statistical thermodynamics. Chapman and Hall, London McClelland BJ (1973) Statistical thermodynamics. Chapman and Hall, London
33.
go back to reference Herbst E, Millar TJ (2008) The chemistry of cold interstellar cloud cores. In: Smith IWM (ed) Low temperatures and cold molecules. Imperial College Press, London, pp 1–54CrossRef Herbst E, Millar TJ (2008) The chemistry of cold interstellar cloud cores. In: Smith IWM (ed) Low temperatures and cold molecules. Imperial College Press, London, pp 1–54CrossRef
Metadata
Title
Aspects of Physical Chemistry
Author
Ian W. M. Smith
Copyright Year
2013
Publisher
Springer Berlin Heidelberg
DOI
https://doi.org/10.1007/978-3-642-31730-9_1

Premium Partners