scholarly journals Damage in domains and interfaces: a coupled predictive theory

2006 ◽  
Vol 1 (7) ◽  
pp. 1205-1233 ◽  
Author(s):  
Francesco Freddi ◽  
Michel Frémond
Keyword(s):  
2009 ◽  
Vol 13 (9) ◽  
pp. 1141-1151
Author(s):  
Karim Benzarti ◽  
Pierre Argoul ◽  
Francesco Freddi ◽  
Michel Frémont ◽  
Thi Hoa Tam Nguyen

2005 ◽  
Vol 109 (21) ◽  
pp. 4646-4656 ◽  
Author(s):  
Lawrence B. Harding ◽  
Yuri Georgievskii ◽  
Stephen J. Klippenstein

1995 ◽  
Vol 33 (3) ◽  
pp. 427-440 ◽  
Author(s):  
KEVIN B. GRIER ◽  
MICHAEL MCDONALD ◽  
ROBERT D. TOLLISON

Cell Systems ◽  
2018 ◽  
Vol 6 (4) ◽  
pp. 456-469.e10 ◽  
Author(s):  
Manuel Razo-Mejia ◽  
Stephanie L. Barnes ◽  
Nathan M. Belliveau ◽  
Griffin Chure ◽  
Tal Einav ◽  
...  

2019 ◽  
Vol 15 (S352) ◽  
pp. 350-352
Author(s):  
Kathryn Grasha ◽  
Daniela Calzetti

AbstractStar formation provides insight into the physical processes that govern the transformation of gas into stars. A key missing piece in a predictive theory of star formation is the link between scales of individual stars and star clusters up to entire galaxies. LEGUS is now providing the information to test the overall organization and spatial evolution of star formation. We present our latest findings of using star clusters from LEGUS combined with ALMA CO observations to investigate the transition from molecular gas to star formation in local galaxies. This work paves the way for future JWST observations of the embedded phase of star formation, the last missing ingredient to connect young star clusters and their relation with gas reservoirs. Multi-wavelength studies of local galaxies and their stellar and gas components will help shed light on early phases of galaxy evolution and properties of the ISM at high-z.


2014 ◽  
Vol 90 (6) ◽  
Author(s):  
Guillaume Hupin ◽  
Sofia Quaglioni ◽  
Petr Navrátil

2010 ◽  
Vol 7 (3) ◽  
pp. 317-343 ◽  
Author(s):  
ELINOR OSTROM ◽  
XAVIER BASURTO

Abstract:Most powerful analytical tools used in the social sciences are well suited for studying static situations. Static and mechanistic analysis, however, is not adequate to understand the changing world in which we live. In order to adequately address the most pressing social and environmental challenges looming ahead, we need to develop analytical tools for analyzing dynamic situations – particularly institutional change. In this paper, we develop an analytical tool to study institutional change, more specifically, the evolution of rules and norms. We believe that in order for such an analytical tool to be useful to develop a general theory of institutional change, it needs to enable the analyst to concisely record the processes of change in multiple specific settings so that lessons from such settings can eventually be integrated into a more general predictive theory of change.


2015 ◽  
Vol 10 (S314) ◽  
pp. 290-294
Author(s):  
Michael C. Liu

AbstractI present a highly biased and skewed summary of IAU Symposium 314, “Young Stars and Planets Near the Sun,” held in May 2015. This summary includes some takeaway thoughts about the rapidly evolving state of the field, as well as some crowd-sourced predictions for progress over the next ~10 years. We predict the elimination of 1–2 of the currently recognized young moving groups, the addition of 3 or more new moving groups within 100 pc, the continued lack of a predictive theory of stellar mass, robust measurements of the gas and dust content of circumstellar disks, and an ongoing struggle to achieve a consensus definition for a planet.


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