57 research outputs found

    The future problem solving program international: an intervention to promote creative skills in portuguese adolescents

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    The Future Problem Solving Program International (FPSPI) is an internationally applied educational program that involves young people. Its theoretical foundation is both the Creative Problem Solving Model and the Futurist Thinking. It aims to promote creative and critical thinking through a futurist approach to problems. This study intended to analyze the effects of the program on creative skills evaluated by the Torrance Tests of Creative Thinking (Figural Version). The participants’ perceptions of the efficacy of the program were also assessed. This intervention was carried out with 131 adolescents over a period of 7 months in an extra-curricular context. The evaluation of the program takes into account periods both before and after interventions, using similar experimental and control groups. The results showed significant statistical differences for the all skills studied and very positive perceptions of the efficacy of FPSPI. Two significant gender differences in creative performance were also found. The results are described and discussed in order to promote awareness for future research concerning this program(undefined)info:eu-repo/semantics/publishedVersio

    Diversifying Experiences

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    Diversifying experiences

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    In the current chapter diversifying experiences - unusual and unexpected events or situations that push people outside of the realm of normality - and their influence on creativity are discussed. Three different types of diversifying experiences are considered. Most of this chapter is dedicated to schema-violations. Different types of schema violations are discussed, varying in intensity, valence, and level of engagement. An explanation is offered for why they can influence creativity. Next, the focus shifts to mental and developmental adversity and multicultural experience and on how they may act as diversifying experience and hereby influence creativity

    Cultural diversity and creativity

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    Cultural diversity refers to the extent of cultural differences that exist between people. The first part of our chapter discusses the influence that diversity has on creative processes. Historiometric, cross-sectional and experimental work supports the idea that, under the right circumstances, individual experiences of diversity can increase creative potential. Studies on group and team creativity paint a more complex picture, suggesting that group diversity can sometimes help and sometimes hinder creative performance. We also discuss the issue of cross-cultural differences in creativity and suggest that further work is needed to better understand what aspects of creativity are shared, and what aspects of creativity are different across cultures

    Herschel/PACS OH Spectroscopy of Seyfert, LINER, and Starburst Galaxies

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    We investigated the 65, 71, 79, 84, 119, and 163 μm OH doublets of 178 local (0 < z < 0.35) galaxies. They were observed using the Herschel/Photoconductor Array Camera and Spectrometer, including Seyfert galaxies, low-ionization nuclear emission-line regions, and star-forming galaxies. We observe these doublets exclusively in absorption (OH71), primarily in absorption (OH65, OH84), mostly in emission (OH79), only in emission (OH163), and an approximately even mix of the both (OH119). In 19 galaxies we find P Cygni or reverse P Cygni line profiles in the OH doublets. We use several galaxy observables to probe spectral classification, brightness of a central active galactic nucleus (AGN)/starburst component, and radiation field strength. We find that OH79, OH119, and OH163 are more likely to display strong emission for bright, unobscured AGNs. For less luminous, obscured AGNs and nonactive galaxies, we find populations of strong absorption (OH119), weaker emission (OH163), and a mix of weak emission and weak absorption (OH79). For OH65, OH71, and OH84, we do not find significant correlations with the observables listed above. For OH79 and OH119, we find relationships with both the 9.7 μm silicate feature and Balmer decrement dust extinction tracers in which more dust leads to weaker emission/stronger absorption. The origin of emission for the observed OH doublets, whether from collisional excitation or from radiative pumping by infrared photons, is discussed.With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737
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