![]() |
|
|---|
|
|
The metal hydrides |
|
THERMODYNAMICS It is known that some metals and alloys are able to absorb chemically hydrogen and then to reversibly release it [1-12]. The thermodynamic aspects of hydride formation from gaseous hydrogen are described by the PCI (pressure-composition isotherm) curves as shown in Fig. 1a. These curves are obtained in the following way. At a given temperature and with a low hydrogen pressure, the host metal begins to dissolve a small quantity of hydrogen in solid solution (α phase), after the dissociation of the H2 molecule into atomic hydrogen at the surface of the material. When the pressure increases, the hydrogen concentration in the metal undergoes small increments and then the local interactions between hydrogen atoms become more and more important up to the nucleation and growth of the hydride phase β. As long as the solid solution and the hydride coexist, the isotherm curves (hydrogen pressure at a given temperature as a function of hydrogen concentration in the material) present a plateau; the length of this plateau represents the hydrogen amount which can be reversibly stored at that temperature by small pressure changes. When the α→β transition is completed, the hydrogen pressure begins again to sharply increase with the concentration. The region of the diagram where the two phases coexist ends at a critical point Tc, over which the α→β transition is continuous. The equilibrium pressure (position of the plateau) strongly depends on temperature and is related to the enthalpy and entropy changes DH and DS, respectively, by the Van’t Hoff relation, reported analytically and graphically in Fig. 1b.
The
enthalpy changes related to the hydride formation or dissociation can
obtain experimentally from the slope of Van’t Hoff's plots. While the
enthalpy term depends on the metal-hydrogen bond stability, the entropy
term corresponds essentially to the transition from molecular hydrogen
to atomic hydrogen, necessary for the passage from gaseous to solid
phase and is similar for all the known hydrides. The working
temperature of a metal/hydride system is fixed by the thermodynamic
equilibrium pressure and by the overall reaction kinetics. In order to
make metal hydrides interesting for the use in hydrogen reservoirs, the
working pressure and temperature should be in the ranges 1-10 bar and
20-100 °C, respectively, corresponding to an enthalpy change between 15
and 24 kJ/molH. A further problem, already mentioned, concerns the
weight of the absorbing material, thus light metal hydrides containing
a high amount of hydrogen are preferable. Table 1 presents some
features of the main hydrides studied so far [1]. Besides the mentioned
thermodynamic aspects, also the hydrogen absorption and desorption
kinetics, i.e. the rate at which these processes occur, have a primary
importance for practical applications. However, none of the currently
studied hydrides presents at the same time all the required
characteristics for the practical functionality of a hydride-based
hydrogen reservoir.
COMMERCIAL HYDRIDES Hydrides of AB5 (e.g. LaNi5), AB (e.g. FeTi), AB2 (e.g. ZrV2) and A2B (e.g. Mg2Ni) types alloys are already commercially available and are supplied in special vessels. AB5 alloys absorb quickly and reversibly hydrogen at a pressure of few bars at room temperature or close to it. Moreover, they stand repeated cycles of absorption/desorption without loss of storage capacity [2]. Their weak point is the low weigh percent of stored hydrogen (less than 1.5), which makes the reservoir too heavy. Among the goals that, according to the U.S. DOE (Department of Energy), should be achieved within 2015 with the materials used for hydrogen storage, there are a hydrogen wt% of 5.5 (referred to the entire storage system), which is equivalent to 1.8 kWh/kg. The other 2015 targets are 40 g/L (1.3 kWh/L) and 3.3 min (1.5 kgH2/min) for the system volumetric density and the system fill time for 5-kg fill, respectively. Therefore, the AB5 alloys are not ideal for the use in a hydrogen reservoir, while they are more suitable as electrodes in a fuel cell [3]. The Fe-Ti alloy, studied since the 70’s and cheaper than the LaNi5 alloy, forms the hydrides FeTiH and FeTiH2 [4]. It allows absorption and desorption operations in thermodynamic favourable conditions, but requires a too high activation temperature and the weight percent of stored hydrogen (less than 2) also in this case is too low. AB2 alloys present, with respect AB5 alloys, a better reaction kinetics and a lower cost, but are more sensitive to contaminants. Mg2Ni alloy has a higher hydrogen capacity (up to 3.6 wt%), but the required working temperature for absorption and desorption reactions is higher than 200 °C.
LIGHT METALS BASED HYDRIDES A
high quantity of stored hydrogen can be achieved only by using light
elements like magnesium, which forms the hydride MgH2
with a theoretical hydrogen weight percent of 7.6 [5]. The use of
magnesium presents two main difficulties. First, due to the high
stability of Mg-H bond, the plateau pressure of the system is too low
in the temperature range of applicative interest (it is only 0.36
mbar at 100 °C). In order to get desorption pressures near
atmospheric, it is necessary to raise the temperature to about 300
°C. Moreover, even at 300 °C the hydrogenation and dehydrogenation
reactions are sluggish. It has been shown that the use of
nanostructured magnesium hydride produced by high energy milling is
more convenient than the massive material [6]: the presence of
sub-micrometric grains reduces the hydrogen diffusive path in solid
phase and the high concentration of defects and grain boundaries
offer preferential paths for gas escape and also nucleation sites for
metallic Mg. Good absorption and desorption kinetics were achieved
around 230 °C by milling metallic magnesium or its hydride with or
without the addition of catalysts [7-13].
REFERENCES 1. G. Sandrock, G. Thomas, IEA/DOC/SNL on-line hydride databases, Appl. Phys. A72 (2001) 153. 2. R.C. Bowman, C.H. Luo, C.C. Ahn, C.K. Witham, B. Fultz, J. Alloys Compd. 217 (1995) 185. 3. T. Sakai, M. Natsuoka, C. Iwakura, Handb. Phys. Chem. Rare Earths 21 (1995) 135. 4. J.J. Reilly, R.H. Wiswall, Inorg. Chem. 13 (1974) 218. 5. L. Schlapbach, A. Züttel, Nature 414 (2001) 353. 6. G. Liang, J. Huot, S. Boily, A. van Neste, R. Schulz, J. Alloys Compd. 292 (1999) 247. 7. R. Shulz, J. Huot, G. Liang, S. Boily, G. Lalande, M.C. Denis, J.P. Dodelet, Mater. Sci. Eng. A267 (1999) 240. 8. Zaluska, L. Zaluski, J.O. Stroem-Olsen, Appl. Phys. A72 (2001) 157. 9. R.C. Bowman, B. Fultz, MRS Bull. 27 (2002) 688. 10. B. Sakintuna,F. Lamari-Darkrim, M. Hirscher, Int. J. Hydrogen Energy 32 (2007) 1121. 11. Huot, M.-L. Tremblay, R. Schulz, J. Alloys Compd. 356-357 (2003) 603. 12. P. Palade, S. Sartori, A. Maddalena, G. Principi, S. Lo Russo, M. Lazarescu, G. Schinteie, V. Kuncser, G. Filoti, J. Alloys Compd. 415 (2006) 170. 13. A. Maddalena, M. Petris, P. Palade, S. Sartori, G. Principi, E. Settimo, B. Molinas, S. Lo Russo, Int. J. Hydrogen Energy 31 (2006) 2097. 14. A. Züttel, Materials Today, vol. 6 September (2003) 24. 15. W. Luo, J. Alloys Compd. 381 (2004) 284. 16. S. Orimo, Y. Nakamori, G. Kitahara, K. Miwa, N. Ohba, S. Towata, A. Züttel, J. Alloys Compd. 404–406 (2005) 427. 17. J.J. Vajo and G.L. Olson, Scr. Mater. 56 (2007) 829. 18. F. Agresti, A. Khandelwal, G. Capurso, S. Lo Russo, A. Maddalena, G. Principi, Nanotechnology 21 (2010) 065707.
|
||||||||||||||||||||||||||||