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Casting Light on the Darkening of Colors in Historical Paintings

F. Da Pieve, C. Hogan, D. Lamoen, J. Verbeeck, F. Vanmeert, M. Radepont, M. Cotte, K. Janssens, X. Gonze, and G. Van Tendeloo
Phys. Rev. Lett. 111, 208302 – Published 15 November 2013
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Abstract

The degradation of colors in historical paintings affects our cultural heritage in both museums and archeological sites. Despite intensive experimental studies, the origin of darkening of one of the most ancient pigments known to humankind, vermilion (α-HgS), remains unexplained. Here, by combining many-body theoretical spectroscopy and high-resolution microscopic x-ray diffraction, we clarify the composition of the damaged paint work and demonstrate possible physicochemical processes, induced by illumination and exposure to humidity and air, that cause photoactivation of the original pigment and the degradation of the secondary minerals. The results suggest a new path for the darkening process which was never considered by previous studies and prompt a critical examination of their findings.

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  • Received 16 February 2013

DOI:https://doi.org/10.1103/PhysRevLett.111.208302

© 2013 American Physical Society

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Why Red Paint Darkens over the Centuries

Published 15 November 2013

Experiments and calculations reveal the chemical reactions that cause the brilliant red in ancient paintings to turn dark over time, as well as potential preservation measures.

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Authors & Affiliations

F. Da Pieve1,2,*, C. Hogan3,4, D. Lamoen2, J. Verbeeck2, F. Vanmeert5, M. Radepont5, M. Cotte6, K. Janssens5, X. Gonze7, and G. Van Tendeloo2

  • 1ALGC, Research Group General Chemistry, Vrije Universiteit Brussel (VUB), Pleinlaan 2, B-1050 Brussels, Belgium
  • 2EMAT, University of Antwerp, Groenenborgerlaan 171, B-2020 Antwerp, Belgium
  • 3Consiglio Nazionale delle Ricerche, Istituto di Struttura della Materia (CNR–ISM), via Fosso del Cavaliere 100, 00133 Rome, Italy
  • 4Department of Physics and European Theoretical Spectroscopy Facility (ETSF), Università di Roma “Tor Vergata,” Via della Ricerca Scientifica 1, 00133 Rome, Italy
  • 5Department of Chemistry, University of Antwerp, Groenenborgerlaan 171, B-2020 Antwerp, Belgium
  • 6European Synchrotron Radiation Facility, Beamline ID21, BP 220, 38043 Grenoble Cedex, France
  • 7Institute of Condensed Matter and Nanoscience, Université Catholique de Louvain, Chemin des étoiles 8, bte L7.03.01, B-1348 Louvain-la-Neuve, Belgium and European Theoretical Spectroscopy Facility (ETSF)

  • *Corresponding author. fabiana.dapieve@gmail.com

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Issue

Vol. 111, Iss. 20 — 15 November 2013

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