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|1.6 Photocatalyzed Reactions|<br />

an average power of approximately 100 terawatts of sunlight, natural photosynthesis directly and<br />

indirectly provides the basis for nearly all life on earth. G. Ciamician, an important pioneer<br />

of photochemistry research, realized the relevance of that fact (see figure 11). Although his<br />

understanding was certainly basic, he found out that the use of solar energy would help to:<br />

[21, 22]<br />

(1) carry out reactions under mild conditions,<br />

(2) look for activation conditions that allow for more direct reactions and thus improve<br />

atom economy,<br />

(3) increase the use of renewable materials or reagents (using directly light rather than<br />

fossil solar energy) and<br />

(4) minimize the use of energy.<br />

Figure 11: Photochemistry pioneer GIACOMO CIAMICIAN, as he watches his reactions, driven by solar<br />

irradiation in flasks on the balcony on top of his laboratory at the University of Bologna, Italy, circa<br />

1910. [4]<br />

Today, these statements are incorporated into the "12 principles" of green chemistry as formulated<br />

by Anastas and Warner. [23]<br />

According to Turro, today it is known that photochemical reactions differ from thermal reactions<br />

in three important respects: [24] |14|

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