Pub Date : 2021-10-01DOI: 10.1088/978-0-7503-3527-0ch12
P. Alam
This study was conducted to determine the phenotypic characteristics of the angut pigeon breed, which is native to Şanlıurfa, where pigeon breeding has been done traditionally for a long time and is also one of the domestication centers. In this study, we adopted 146 angut pigeons comprising 72 males and 74 females. Additionally, four different colour variations were determined: yellow angut (41.1%, n = 60), red angut (35.6%, n = 52), white angut (13.7%, n = 20) and black angut (9.6%, n = 14). All the colour variants had a peak crest (upright feathers) costume structure, which was at the back of the head, starting from the end of the neck and extending from ear to ear. Among the gender groups from the measurements obtained in this study; wing length, wingspan, tail length and head width (P < 0.001); shank length and head length (P < 0.01). Differences in beak length and beak width were also significant (P < 0.05). Moreover, the differences in beak length and beak width were significant (P < 0.05). Today, although anguts are morphologically similar to the Demkeş breed in Turkey, they do not have trumpeting sound ability. The trumpeter breeds of fancy pigeons are so named because of their unique vocalizations, which sound vaguely like low laughter. The data obtained on the morphological features of angut pigeons support the hypothesis that angut pigeons are a form pigeon and should be defined as a different breed.
{"title":"‘L’","authors":"P. Alam","doi":"10.1088/978-0-7503-3527-0ch12","DOIUrl":"https://doi.org/10.1088/978-0-7503-3527-0ch12","url":null,"abstract":"This study was conducted to determine the phenotypic characteristics of the angut pigeon breed, which is native to Şanlıurfa, where pigeon breeding has been done traditionally for a long time and is also one of the domestication centers. In this study, we adopted 146 angut pigeons comprising 72 males and 74 females. Additionally, four different colour variations were determined: yellow angut (41.1%, n = 60), red angut (35.6%, n = 52), white angut (13.7%, n = 20) and black angut (9.6%, n = 14). All the colour variants had a peak crest (upright feathers) costume structure, which was at the back of the head, starting from the end of the neck and extending from ear to ear. Among the gender groups from the measurements obtained in this study; wing length, wingspan, tail length and head width (P < 0.001); shank length and head length (P < 0.01). Differences in beak length and beak width were also significant (P < 0.05). Moreover, the differences in beak length and beak width were significant (P < 0.05). Today, although anguts are morphologically similar to the Demkeş breed in Turkey, they do not have trumpeting sound ability. The trumpeter breeds of fancy pigeons are so named because of their unique vocalizations, which sound vaguely like low laughter. The data obtained on the morphological features of angut pigeons support the hypothesis that angut pigeons are a form pigeon and should be defined as a different breed.","PeriodicalId":10614,"journal":{"name":"Composites Engineering: An A–Z Guide","volume":"132 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2021-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"79648992","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2021-10-01DOI: 10.1088/978-0-7503-3527-0ch15
P. Alam
The field of gastronomy, according to research funding agencies in Brazil, is classified in the large area of health sciences. However, despite this official classification, it can be said that gastronomy is crossed by a series of theoretical and methodological issues, of an interdisciplinary nature, which expands it beyond its disciplinary boundaries. In this sense, this article aims to discuss the French philosophy of Michel Foucault, especially from the genealogical phase of the thinker, when the main characteristics of disciplinary power and biopower were addressed. In addition to this initial approach, a film analysis of the cinematographic work called “Gosto se discussed” was presented, in which excerpts were highlighted that showed the full operationalization of body training technologies inside the kitchen of a traditional restaurant in São Paulo. It is expected that the present work will collaborate to enhance, more and more, the use of cinematographic works as a didactic and pedagogical resource in the educational field.
根据巴西研究资助机构的说法，烹饪领域属于健康科学的大领域。然而，尽管有这种官方分类，但可以说，美食学是由一系列跨学科性质的理论和方法问题交叉的，这使它超出了学科界限。在这个意义上，本文旨在讨论米歇尔·福柯的法国哲学，特别是从思想家的谱系阶段，当纪律权力和生命权力的主要特征被解决。除了这种最初的方法之外，还展示了对电影作品“Gosto se discussed”的电影分析，其中突出显示了圣保罗一家传统餐厅厨房内身体训练技术的全面运作。预期目前的工作将有助于越来越多地加强使用电影作品作为教育领域的教学和教学资源。
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Pub Date : 2021-10-01DOI: 10.1088/978-0-7503-3527-0ch3
P. Alam
We study a class of early dark energy (EDE) models, in which, unlike in standard dark energy models, a substantial amount of dark energy exists in the matter-dominated era. We self-consistently include dark energy perturbations, and show that these models may be successfully constrained using future observations of galaxy clusters, in particular the redshift abundance, and the Sunyaev–Zel’dovich (SZ) power spectrum. We make predictions for EDE models, as well as ΛCDM for incoming X-ray (eROSITA) and microwave (South Pole Telescope) observations. We show that galaxy clusters’ mass function and the SZ power spectrum will put strong constraints both on the equation of state of dark energy today and the redshift at which EDE transits to present-day ΛCDM-like behavior for these models, thus providing complementary information to the geometric probes of dark energy. Not including perturbations in EDE models leads to those models being practically indistinguishable from ΛCDM. An MCMC analysis of future galaxy cluster surveys provides constraints for EDE parameters that are competitive with and complementary to background expansion observations such as supernovae.
{"title":"‘C’","authors":"P. Alam","doi":"10.1088/978-0-7503-3527-0ch3","DOIUrl":"https://doi.org/10.1088/978-0-7503-3527-0ch3","url":null,"abstract":"We study a class of early dark energy (EDE) models, in which, unlike in standard dark energy models, a substantial amount of dark energy exists in the matter-dominated era. We self-consistently include dark energy perturbations, and show that these models may be successfully constrained using future observations of galaxy clusters, in particular the redshift abundance, and the Sunyaev–Zel’dovich (SZ) power spectrum. We make predictions for EDE models, as well as ΛCDM for incoming X-ray (eROSITA) and microwave (South Pole Telescope) observations. We show that galaxy clusters’ mass function and the SZ power spectrum will put strong constraints both on the equation of state of dark energy today and the redshift at which EDE transits to present-day ΛCDM-like behavior for these models, thus providing complementary information to the geometric probes of dark energy. Not including perturbations in EDE models leads to those models being practically indistinguishable from ΛCDM. An MCMC analysis of future galaxy cluster surveys provides constraints for EDE parameters that are competitive with and complementary to background expansion observations such as supernovae.","PeriodicalId":10614,"journal":{"name":"Composites Engineering: An A–Z Guide","volume":"11 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2021-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"77755304","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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