Abstract

Here we report the chemoselective synthesis of several important, climate relevant isoprene nitrates using silver nitrate to mediate a ’halide for nitrate’ substitution. Employing readily available starting materials, reagents and Horner–Wadsworth–Emmons chemistry the synthesis of easily separable, synthetically versatile ‘key building blocks’ (E)- and (Z)-3-methyl-4-chlorobut-2-en-1-ol as well as (E)- and (Z)-1-((2-methyl-4-bromobut-2-enyloxy)methyl)-4-methoxybenzene has been achieved using cheap, ’off the shelf’ materials. Exploiting their reactivity we have studied their ability to undergo an ‘allylic halide for allylic nitrate’ substitution reaction which we demonstrate generates (E)- and (Z)-3-methyl-4-hydroxybut-2-enyl nitrate, and (E)- and (Z)-2-methyl-4-hydroxybut-2-enyl nitrates (‘isoprene nitrates’) in 66–80% overall yields. Using NOESY experiments the elucidation of the carbon–carbon double bond configuration within the purified isoprene nitrates has been established. Further exemplifying our ‘halide for nitrate’ substitution chemistry we outline the straightforward transformation of (1R,2S)-(−)-myrtenol bromide into the previously unknown monoterpene nitrate (1R,2S)-(−)-myrtenol nitrate.

Highlights

  • Understanding the chemistry of the biosphere and its interaction with the atmosphere is fundamental to Earth System science

  • We considered the development of efficient synthesis routes to small organic nitrates to have broader benefits to the general synthesis community

  • Exploring the potential of isoprene as a starting material we considered it to have several advantages: it is cheap, commercially available, handled and has the prerequisite C5-skeleton that ensures it is a highly desirable and amenable starting material for its chemical transformation into isoprene nitrates (IPNs)

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Summary

Introduction

Understanding the chemistry of the biosphere and its interaction with the atmosphere is fundamental to Earth System science. Subjecting rac-17 to O-nitration with in situ generated 22 resulted, as judged by 1H NMR, in a very poor yield (

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