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Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University

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Page 1: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Surfaces processes IIChemical routes

François Dulieu

LERMA

Paris Observatory and Cergy Pontoise University

Page 2: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

Molecules detected in 2002 in astrophysical environments

Surface processes I

Order of magnitudesStickingDesorptionComparison of methods (TPD, RAIRS, STM)

Surface processes IIChemical routes

Surface processes IIIDiffusion on surfaceDiffusion in bulkEnergetic aspects

Studied in lab.

Page 3: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

“Thermal cold surface Chemistry”, today

And H2O

2 ,

NH

2OH (?), CH

3NH

2 ...

Page 4: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

H CO O2

O O3

NO C2/3

H4/6

HCN H2

H H2

H2CO

CH3OH

H2O

2

H2O

+

OH+

H2O

2

H2O

+

NH2OH

NO2

CH2NH

CH3NH

2

O OH+

CO2

(?) (O2/O

3 ) C

2/3H

4/6O

OH HCOOHH

2CO

3

CO2

HNO3

+++

H2O

“Thermal cold surface (fast) chemistry”

No bulk chemistryNo irradiation (UV, electrons, Ions...)

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

Page 5: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

H CO O2

O NO C2/3

H4/6

HCN H2

H H2

H2CO

CH3OH

H2O

2

H2O

OH NH2OH

NO2

CH2NH

CH3NH

2

O OH CO2

(?) (O2/O

3 ) C

2/3H

4/6O

OH HCOOHH

2CO

3

CO2

HNO3

+++

H2O

“Thermal cold surface (fast) chemistry”

Num

ber

of m

olec

ule

s

Year

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

Page 6: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

H2 formation, a world in itself ! (Experiments only...)

On silicatesEfficiencies & process, see numerous Vidali and coworkers, (Cazaux et al)Energetic aspects, Lemaire et al 2010

On carbonaceous materialsEfficiencies & process : Vidali et al, Menella,

Zecho et al, Hornekaer et al …Energetic aspects, S. Price and coworkers

On water Ice :Efficiencies & process : Vidali et al, Amiaud et al 2007, Hornekaer et al 2003, Watanabe et al 2010.Energetic aspects : Hornekaer et al 2003, Congiu et al 2009,

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

Page 7: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

CO + H

CO + H HCO

tunnelling

Pirim et al, 2010, J. Phys. Chem. A

H2CO

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

CO H2 H

3 K

10 K

Page 8: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

CO + H

CO + H HCOtunnelling

Pirim et al, 2010, J. Phys. Chem. A

H2CO H

2COH CH

3OH

Fuchs et al, 2009, A&A

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

Page 9: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen II/III

CO + HCO + H HCO

tunnellingH

2CO H

2COH CH

3OH

tunnelling

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

Page 10: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Oxygen and Hydrogen experimentsO beam H beam

Ozone

About 20 reactions... + different experimental conditions and methods

Page 11: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Oxygen and Hydrogen experimentsO beam H beam

Water is easy to form experimentally !

O + H

O2 + H

O3 + H

Water is one of the compound easily formedon cold surfaces (10 - 50K)

Dulieu et al 2010, Vidali et al 2011

Miyauchi et al 2008, Ioppolo et al 2008Matar et al 2008, Oba et al 2009, Ioppolo et al 2010, Cuppen et al 2010

Mokrane et al 2009, Romanzin et al2011

Water formation rate >> CO + H ; CO+OH … > H + H

Water is amorphous and compact (Oba et al 2009, Accolla thesis)

Page 12: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Experimental agreement ?

3 itemsNo doubt

2 itemsstrong evidences

1 itemweak evidence

No item?

See Dulieu 2011IAU 280

Page 13: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Water formation (sub monolayer)

O2 + D → OD

O2D + D → D

2O

2

D2O

2+D → D

2O+OD

OD+ D → D2O

No barrier model. The probability of reaction is proportional to the surface concentration of reactants.

O2

HO2

H2O

2 OH

H2O

(D+D is small as longAs other product is present )

Page 14: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

O2 + D

O3+ D @ 10K

O3 + D @ 45 K

O3 +H → O2 + OHO2 desorb below 45 K

Signal O2

TPD, sub-monolayer regime

Water formation (sub monolayer)

Page 15: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

O2 + D → O2DO2D + D → D2O2D2O2+D → D2O+ODOD+ D → OD

Signal H2O2

Signal H2O

Signal H2O2

OH + H ?

H2O

2 is almost always < H

2O

O3+ H @ 10K

O3 + H @ 45 K

O2 + H

Water formation (sub monolayer)

Page 16: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Water formation “Multilayer”

Ioppolo et al PCCP 2010, IR spectroscopy, growing a O

2+ H layers (35 ML)

Much more H2O

2 than H

2O

Low H2O

2 comsuption

Probably H+H → H2

is the most active reaction !

H needs to penetrate through thesample

Page 17: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Water formation

Can explainMost of the signal,But chemical desorptionIs missing

Page 18: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Water formation O2

HO2

H2O

2 OH

H2O

Can explainMost of the signal,But chemical desorptionIs missing

Page 19: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Water formation

- Chemical desorption

- Substrate dependancy

Still to do :

Page 20: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

CO + OH reaction on cold surfaces

Photochemistry : CO + OH → CO2 + H

CO + OH on surfaces but “bulk or matrix” conditionsOba et al 2010, Ioppollo et al 2011, Zins et al 2011

© Noble et al 2011

No pure OH beam → in situ control of OH formation

Comparison of surfaces, coverage, temperature andChemical networks

Page 21: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

CO + OH reaction on cold surfacesH addition to CO/O2 mixtureOr CO/O3 mixture © Noble et al 2011

CO/O2 + H

Slow

HCO +HH

2CO

CO/HO2 + H

Slow

CO/H2O

2 + H

CO/OH / H2O

+ H

CO/ H2O / H

2O

CO2

+H

CO/O3 + H CO/OH + H

@ 50K

CO / H

2O

Page 22: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

CO + OH reaction on cold surfacesO2 and O3 pathways

© Noble et al 2011

CO2 is always a tiny compounds (max 4 %)No important substrate effectKinetics is different starting from O3 and O2

CO/O3 + H

CO/O2 + H

CO2

CO

Page 23: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

CO + OH reaction on cold surfacesH addition to CO/O2 mixture

© Noble et al 2011

CO2 is always a tiny compounds (max 4 %)No important substrate effectKinetics is different starting from O3 and O2

CO/O3 + H

CO/O2 + H

CO2

CO

Page 24: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

CO + OH reaction on cold surfacesH addition to CO/O2 mixture

© Noble et al 2011

CO2 is always a tiny compounds (max 4 %)No important substrate effectKinetics is different starting from O3 and O2

CO/O3 + H

CO/O2 + H

CO2

CO

Page 25: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

CO/O2 mixture + H (Ioppolo et al 2011) CO + OH mixture(Oba et al 2010)

From Goumans et al 2008

Page 26: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

© Congiu et al 2012, ApJ L et soumis a JCP

CO/O2 + H

- IR spectroscopy vs Mass spectroscopy

- Bulk chemistry vs surface chemistry

NH2OH synthesis via NO +H

Page 27: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

NH2OH synthesis via NO +H

© Congiu et al 2012, ApJ

NO (et éventuellement (NO)2) exposé à H ou D à 10 K disparait

CO/O2 + H

Page 28: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Synthèse de NH2OH via NO +H

© Congiu et al 2012, ApJ L et soumis a JCP

CO/O2 + H

Page 29: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

© Congiu et al 2012, ApJ

CO/O2 + H

NH2OH synthesis via NO +H

Page 30: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

© Congiu et al 2012, ApJ L and submitted to JCP© Fedoroseev et al 2012, submitted to JCP

- IR spectroscopy vs Mass spectroscopy

- Bulk chemistry vs surface chemistry

- "Fast” chemistry vs “slow” chemistry

Page 31: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

HCN + H

© Theulé et al 2011, A&A

Page 32: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

C2H4 + O → C2H4O

© Ward & Price 2011, ApJ

Page 33: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

C2H4 + O → C2H4O

© Ward & Price 2011, ApJ

==

Page 34: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

“Fast and slow chemistry”Surface and bulk chemistry

© Mispealer, 2012, A&A

Page 35: Surfaces processes II Chemical routes - Radboud Universiteit · Surfaces processes II Chemical routes François Dulieu LERMA Paris Observatory and Cergy Pontoise University. F- Dulieu

Review ofreactions

H+H

CO + H

Water formation

CO2 formation

HCOOH, H2CO3

C2H4O

NH2 -X

conclusion

F- Dulieu – LERMA – Chemistry and Infrared Spectroscopy of Interstellar Dust – June 2012, Nijmegen

Surface, dynamic matrix and bulk chemistry

More and more molecules …

Be carrefull when you compare results.

Surface: competition of fast process - stable products and fast reactions

Matrix dynamically grown : - radicals may survive- “secondary” reactions can happen- can be surface reactions if the reaction are faster than the growth

(T dependant)

Bulk chemistry- driven by slow reorganisation of the ice- in competition with desorption