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Could dark matter or neutrinos discriminate between the enantiomers of a chiral molecule?

dc.contributor.authorDobado González, Antonio
dc.contributor.authorBargueño, P.
dc.contributor.authorGonzalo Fonrodona, Isabel
dc.date.accessioned2023-06-20T10:35:04Z
dc.date.available2023-06-20T10:35:04Z
dc.date.issued2008-04
dc.descriptionThis work is supported by the DGICYT (Spain) project BPA2005-02327, by the Universidad Complutense/CAM projects 910309 and CCG06-UCM/ESP-137, and by the MEC (Spain) projects CTQ2005-09185-C02-02 and FIS2004-03267. The work of PB was supported by the FPI grant BES-2006-11976 from the Spanish MEC. The authors would like to thank A. L. Maroto and R. Pérez de Tudela for useful discussions.
dc.description.abstractWe examine the effect of cold dark matter on the discrimination between the two enantiomers of a chiral molecule. We estimate the energy difference between the two enantiomers due to the interaction between fermionic WIMPs (weak interacting massive particles) and molecular electrons on the basis that electrons have opposite helicities in opposite enantiomers. It is found that this energy difference is completely negligible. Dark matter could then be discarded as an inductor of chiroselection between enantiomers and then of biological homochirality. However, the effect of cosmological neutrinos, revisited with the currently accepted neutrino density, would reach, in the most favorable case, an upper bound of the same order of magnitude as the energy difference obtained from the well-known electroweak electron-nucleus interaction in some molecules.
dc.description.departmentDepto. de Óptica
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipDGICYT (Spain)
dc.description.sponsorshipUniversidad Complutense/CAM
dc.description.sponsorshipMEC (Spain)
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/21466
dc.identifier.doi10.1209/0295-5075/82/13002
dc.identifier.issn0295-5075
dc.identifier.officialurlhttp://iopscience.iop.org/0295-5075/82/1/13002
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.relatedurlhttp://arxiv.org/abs/0802.2164
dc.identifier.urihttps://hdl.handle.net/20.500.14352/50654
dc.issue.number1
dc.journal.titleEurophysics Letters
dc.language.isoeng
dc.publisherEPL Association, European Physical Society
dc.relation.projectIDBPA2005-02327
dc.relation.projectID910309
dc.relation.projectIDCCG06-UCM/ESP-137
dc.relation.projectIDCTQ2005-09185-C02-02
dc.relation.projectIDFIS2004-03267
dc.relation.projectIDBES-2006-11976
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.cdu535
dc.subject.keywordRacemic Amino-Acids
dc.subject.keywordParity Violation
dc.subject.keywordBiomolecular Homochirality
dc.subject.keywordEnergy Difference
dc.subject.keywordOrigin
dc.subject.keywordRadiation
dc.subject.keywordLight
dc.subject.ucmFísica (Física)
dc.subject.ucmÓptica (Física)
dc.subject.unesco22 Física
dc.subject.unesco2209.19 Óptica Física
dc.titleCould dark matter or neutrinos discriminate between the enantiomers of a chiral molecule?
dc.typejournal article
dc.volume.number82
dcterms.references[1] Bonner W. A., Orig. Life Evol. Biosph., 21 (1991) 59. [2] Jorissen A. and Cerf C., Orig. Life Evol. Biosph., 32 (2002) 129. [3] Cline D. B. (Editor), The Physical Origin of Homochirality in Life, AIP Conf. Proc., 379 (1996). [4] Hegstrom R. A., Rich A. and Van House J., Nature, 313 (1985) 391. [5] Bailey J., Chrysostomou A. and Hough J. H. et al. Science, 281 (1998) 672. [6] Bailey J., Orig. Life Evol. Biosph., 31 (2001) 167. [7] Buschermhle M., Whittet D. C. B., Chrysostomou A. et al., Astrophys. J., 624 (2005) 821. [8] Rikken G. L. J. A. and Raupach E., Nature, 405 (2000) 932. [9] Ruchon T., Vallet M., Chauvat D. et al., J. Chem. Phys., 125 (2006) 084104. [10] Engel M. H. and Macko S. A., Nature, 389 (1997) 265. [11] Pizzarello S. and Cronin J. R., Geochim. Cosmochim. Acta, 64 (2000) 329. [12] Bonner W. A., Orig. Life Evol. Biosph., 22 (1992) 407. [13] Bouchiat A. M. and Bouchiat C. C., Rep. Prog. Phys.,60 (1997) 1351. [14] Letokhov V. S., Phys. Lett. A, 53 (1975) 275. [15] Rein D. W., Hegstrom R. A. and Sandars P. G. H., J. Chem. Phys., 73 (1980) 2329. [16] Zanasi R., Lazzeretti A. and Soncini A., Phys. Rev. E, 59 (1999) 3382. [17] Laerdahl J. K. and Schwerdtfeger P., Phys. Rev. Lett., 84 (2000) 3811. [18] Soulard P. et al., Phys. Chem. Chem. Phys., 8 (2006) 79. [19] Crassous J. et al., Org. Biomol. Chem., 3 (2005) 2218. [20] Kondepudi D. K. and Nelson G. M., Nature, 314 (1985) 438. [21] Plasson R., Kondepudi D. K., Bersini H., Commeyras A. and Asakura K., Chirality, 19 (2007) 589. [22] Salam A., J. Mol. Evol., 33 (1991) 105. [23] Avalos M., Babiano R., Cintas P., Jim´enez J. L. and Palacios J. C., Tetrahedron Asymmetry, 11 (2000) 2845. [24] Chandrasekhar S., Chirality, 20 (2008) 84. [25] Bargueño P. and Gonzalo I., Orig. Life Evol. Biosph., 36 (2006) 171. [26] Bargueño P. and Pérez de Tudela R., Orig. Life Evol. Biosph., 37 (2007) 253. [27] Muñoz C., Int. J. Mod. Phys. A, 19 (2004) 3093. [28] Sadoulet B., Rev. Mod. Phys., 71 (1999) 197. [29] Gelmini G. B., Phys. Scr., T121 (2005) 131. [30] Stodolsky L., Phys. Rev. Lett., 34 (1975) 110. [31] Pérez-Díaz J. L., Pérez-García V. M. and Gonzalo I., Phys. Lett. A, 160 (1991) 453. [32] Duda G., Gelmini G. and Nussinov S., Phys. Rev. D, 64 (2001) 122001. [33] Dolgov A. D. et al., Nucl. Phys. B, 632 (2002) 363. [34] Binetruy P., Supersymmetry: Theory Experiment and Cosmology (Oxford University Press) 2006. [35] Dark Matter Tools Workgroup Home Page: http:// dmtools.berkeley.edu.
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relation.isAuthorOfPublication.latestForDiscovery16523fad-99a9-422c-9a8e-c949ccffadec

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