Enantiopure Crystallization From Achiral Building Blocks Under Supercooled Conditions
Source abstract
Abstract
Abstract The emergence of homochirality in the absence of external chiral influences remains a fundamental challenge in studies of abiogenesis and asymmetric materials synthesis. Here it is shown that both the conglomerate polymorph of the supramolecular salt (BTBA)FeCl 4 (BTBA = benzyl(tributyl)ammonium) ( 1 , a racemic mixture of 1 ‐ P 3 1 and 1 ‐ P 3 2 ), and its achiral polymorph ( 2 , P 2 1 / c ) exclusively convert into 100% 1 ‐ P 3 1 or 100% 1 ‐ P 3 2 upon melt crystallization at a cooling rate of 3600 K h −1 . Differential scanning calorimetry (DSC) reveals that, prior to this transformation, racemic mixtures of 1 convert into 3 ( P 2 1 / c ), an achiral polymorph distinct from both 1 and 2 , whereas 2 crystallizes directly without intermediates. Nucleation experiments conducted at varying degrees of supercooling show that deeper supercooling effectively impedes molecular reorganization into stable crystal nuclei and, in particular, suppresses secondary nucleation by restricting molecular diffusion, thereby enabling a single chiral nucleus to dominate crystal growth. These results establish melt supercooling as a solvent‐ and template‐free strategy for accessing homochiral materials and reveal how the balance between thermodynamic and kinetic factors governs spontaneous mirror‐symmetry breaking (SMSB).
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Origins and Evolution of Life · Crystallography and molecular interactions · Crystallization and Solubility Studies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
State Key Laboratory of Physical Chemistry of Solid Surfaces and Department of Chemistry College of Chemistry and Chemical Engineering Xiamen University Xiamen 361005 China
Funding
National Natural Science Foundation of China
References (28)
Show source-provided references
1. 10.1038/374594a010.1038/374594a0 ↗
2. 10.1007/BF0158158110.1007/BF01581581 ↗
3. 10.1126/science.ado932510.1126/science.ado9325 ↗
4. 10.1038/3505742110.1038/35057421 ↗
5. 10.1002/anie.20241433210.1002/anie.202414332 ↗
6. 10.1002/anie.20220633210.1002/anie.202206332 ↗
7. 10.1038/ncomms654310.1038/ncomms6543 ↗
8. 10.1002/(SICI)1521-3773(19991203)38:23<3418::AID-ANIE3418>3.0.CO;2-V10.1002/(SICI)1521-3773(19991203)38:23<3418::AID-ANIE3418>3.0.CO;2-V ↗
9. 10.1002/anie.20201388510.1002/anie.202013885 ↗
10. 10.1038/378767a010.1038/378767a0 ↗
11. 10.1021/acs.chemrev.9b0055710.1021/acs.chemrev.9b00557 ↗
12. 10.1021/ja807450610.1021/ja8074506 ↗
13. 10.1002/anie.20090723110.1002/anie.200907231 ↗
14. 10.1021/cg060698d10.1021/cg060698d ↗
15. 10.1021/cg050183710.1021/cg0501837 ↗
16. 10.1021/cg400927m10.1021/cg400927m ↗
17. 10.1002/anie.20100720910.1002/anie.201007209 ↗
18. 10.1002/anie.20220126810.1002/anie.202201268 ↗
19. 10.1126/science.250.4983.97510.1126/science.250.4983.975 ↗
20. 10.1021/acs.cgd.4c0023310.1021/acs.cgd.4c00233 ↗
21. 10.1002/anie.20210780410.1002/anie.202107804 ↗
22. Kashchiev D. · 2000
23. 10.1038/3506570410.1038/35065704 ↗
24. 10.1103/PhysRevLett.93.03550210.1103/PhysRevLett.93.035502 ↗
25. 10.1073/pnas.160493811310.1073/pnas.1604938113 ↗
26. Kelton K. F. · 2010
27. 10.1007/s11426-024-2542-310.1007/s11426-024-2542-3 ↗
28. 10.1021/j150668a00210.1021/j150668a002 ↗