Pervasive nanoscale deformation twinning as a catalyst for efficient energy dissipation in a bioceramic armour

2014 ◽  
Vol 13 (5) ◽  
pp. 501-507 ◽  
Author(s):  
Ling Li ◽  
Christine Ortiz
2007 ◽  
Vol 38 (12) ◽  
pp. 2916-2927 ◽  
Author(s):  
H.A. Padilla ◽  
C.D. Smith ◽  
J. Lambros ◽  
A.J. Beaudoin ◽  
I.M. Robertson

1999 ◽  
Vol 64 (10) ◽  
pp. 3757-3762 ◽  
Author(s):  
Satoshi Shinoda ◽  
Hiroshi Tsukube ◽  
Yoshinobu Nishimura ◽  
Iwao Yamazaki ◽  
Atsuhiro Osuka

2010 ◽  
Vol 136 (1) ◽  
pp. 1-5 ◽  
Author(s):  
A. D. Ghare ◽  
R. N. Ingle ◽  
P. D. Porey ◽  
S. S. Gokhale

2015 ◽  
Vol 3 (18) ◽  
pp. 3654-3676 ◽  
Author(s):  
Qiang Chen ◽  
Hong Chen ◽  
Lin Zhu ◽  
Jie Zheng

Double network (DN) hydrogels as promising soft-and-tough materials intrinsically possess extraordinary mechanical strength and toughness due to their unique contrasting network structures, strong interpenetrating network entanglement, and efficient energy dissipation.


2019 ◽  
Vol 14 (S351) ◽  
pp. 430-433
Author(s):  
Giacomo Fragione

AbstractWith the hundreds of merging binary black holes (BHs) expected to be detected by LIGO, LISA, and other upcoming instruments, the modelling of astrophysical channels that lead to the formation of compact BH binaries has become of crucial importance. BHs of any size can form bound systems in every astrophysical environment, from the field to galactic nuclei. If a binary is too wide, it needs a catalysis process to harden and merge, as in the case a third objects orbiting the BH binary on a distant orbit. In this case, Kozai-Lidov cycles can pump up the binary eccentricity, thus driving it to a merger thanks to efficient energy dissipation at the pericenter. Some remarkable scenarios where the Kozai-Lidov mechanism operates are in triple and quadruple systems of stellar BHs, and in intermediate-mass BH-stellar BH binaries in orbit around a central supermassive BH in galactic nuclei.


2018 ◽  
Vol 20 (3) ◽  
pp. 1794-1799 ◽  
Author(s):  
Sanha Lee ◽  
Gøran Brekke-Svaland ◽  
Fernando Bresme

Deformation twinning provides a mechanism for energy dissipation in crystalline structures, with important implications on the mechanical response of carbonate biogenic materials.


2016 ◽  
Vol 113 (12) ◽  
pp. E1655-E1662 ◽  
Author(s):  
Dvir Harris ◽  
Ofir Tal ◽  
Denis Jallet ◽  
Adjélé Wilson ◽  
Diana Kirilovsky ◽  
...  

In cyanobacteria, photoprotection from overexcitation of photochemical centers can be obtained by excitation energy dissipation at the level of the phycobilisome (PBS), the cyanobacterial antenna, induced by the orange carotenoid protein (OCP). A single photoactivated OCP bound to the core of the PBS affords almost total energy dissipation. The precise mechanism of OCP energy dissipation is yet to be fully determined, and one question is how the carotenoid can approach any core phycocyanobilin chromophore at a distance that can promote efficient energy quenching. We have performed intersubunit cross-linking using glutaraldehyde of the OCP and PBS followed by liquid chromatography coupled to tandem mass spectrometry (LC/MS-MS) to identify cross-linked residues. The only residues of the OCP that cross-link with the PBS are situated in the linker region, between the N- and C-terminal domains and a single C-terminal residue. These links have enabled us to construct a model of the site of OCP binding that differs from previous models. We suggest that the N-terminal domain of the OCP burrows tightly into the PBS while leaving the OCP C-terminal domain on the exterior of the complex. Further analysis shows that the position of the small core linker protein ApcC is shifted within the cylinder cavity, serving to stabilize the interaction between the OCP and the PBS. This is confirmed by a ΔApcC mutant. Penetration of the N-terminal domain can bring the OCP carotenoid to within 5–10 Å of core chromophores; however, alteration of the core structure may be the actual source of energy dissipation.


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