cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Posterior mediastinal mass representing with disfagia and chest pain: Calcified leiomyoma located in distal part of esophagus.
Creators: name: Erkoc, Mustafa Fatih
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Anatomy
subject: Thorax
subject: CT
subject: Fluoroscopy
subject: PACS
subject: Percutaneous
subject: Barium enema
subject: Biopsy
subject: Education
subject: Neoplasia

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 46 years
description: Clinical History: A 46 year old woman presented with retrosternal chest pain and dysphagia aggravating the previous 3 months. Physical examination and basic blood investigation did not reveal any abnormality. She had no previous surgery or any past medical history. Final Diagnosis: Esophageal leiomyoma
Weyl collineations that are not curvature collineations
Creators: name: Hussain, Ibrar
name: Qadir, Asghar
name: Saifullah, K.
Publisher: name: arXiv
Year: 2008
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Though the Weyl tensor is a linear combination of the curvature tensor, Ricci tensor and Ricci scalar, it does not have all and only the Lie symmetries of these tensors since it is possible, in principle, that "asymmetries cancel". Here we investigate if, when and how the symmetries can be different. It is found that we can obtain a metric with a finite dimensional Lie algebra of Weyl symmetries that properly contains the Lie algebra of curvature symmetries. There is no example found for the converse requirement. It is speculated that there may be a fundamental reason for this lack of "duality".
description: 9 pages
An aortic prosthesis infection
Creators: name: Salvan-Schaschl, Carmen
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Abdomen
subject: Arteries / Aorta
subject: Absorptiometry / Bone densiometry
subject: CT
subject: CT-Angiography
subject: Ablation procedures
subject: Diagnostic procedure
subject: Abscess
subject: Aneurysms
subject: Arteriosclerosis
subject: Infection
subject: Prostheses

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 69 years
description: Clinical History: The patient was presenting with recently onset of diffuse abdominal pain. He claimed lower extremity pain starting months ago. For 20 years he had an aortobiiliacal prosthesis surgery. And he was known with renal insufficiency with dialysis. Final Diagnosis: An aortic prosthesis infection
SVC\'s ostium obstruction causes a right-to-left shunt : unusual acquired systemic to-pulmonary venous collateral pathway
Creators: name: HO-MOUYE, Fabien
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Cardiovascular system
subject: CT
subject: Contrast agent-intravenous
subject: Haemodynamics / Flow dynamics

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 63 years
description: Clinical History: A 63-year-old woman was referred to CT-scan for suspicion of pulmonary embolism. She had history of Ebstein disease and tricuspid valves replacement decades ago, no pulmonary disease nor anemia. A recent echocardiography showed normal right and left contr... Final Diagnosis: Systemic-to-Pulmonary veinous acquired shunt as collateral pathway.
Bayesian analysis of spatially distorted cosmic signals from Poissonian data
Creators: name: Weig, Cornelius
name: Ensslin, Torsten
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: Reconstructing the matter density field from galaxy counts is a problem frequently addressed in current literature. Two main sources of error are shot noise from galaxy counts and insufficient knowledge of the correct galaxy position caused by peculiar velocities and redshift measurement uncertainty. Here we address the reconstruction problem of a Poissonian sampled log-normal density field with velocity distortions in a Bayesian way via a maximum a posteriory method. We test our algorithm on a 1D toy case and find significant improvement compared to simple data inversion. In particular, we address the following problems: photometric redshifts, mapping of extended sources in coded mask systems, real space reconstruction from redshift space galaxy distribution and combined analysis of data with different point spread functions.
description: 19 pages, 10 figures, accepted
Osteogenesis Imperfecta : a typical case
Creators: name: HO-MOUYE, Fabien
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Bones
subject: Plain radiographic studies
subject: Diagnostic procedure
subject: Congenital
subject: Demineralisation-Bone

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: male, 7 years
description: Clinical History: A 7 year-old boy, with growth retardation (<2.5 SD , wieght 24 lbs, <95th percentile, in accordance with growth) and motor development delay such as inability to walk, was referred to our hospital for management and counseling. Final Diagnosis: Osteogenesis imperfecta
title: Ð¤Ð¸Ð»Ð¾ÑÐ¾ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸: Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÐµ ÑÐµÑÐ¸ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¸
Creators: name: ÐÐ»ÑÐ³Ð¸Ð½, Ð¡ÐµÑÐ³ÐµÐ¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ñ
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ñ

description: Ð ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ð¸ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² ÐºÐ½Ð¸Ð³Ð¸ ÑÐ°ÑÐºÑÑÐ²Ð°ÐµÑÑÑ Ð¼Ð½Ð¾Ð³Ð¾Ð°ÑÐ¿ÐµÐºÑÐ½Ð°Ñ Ð¾Ð½ÑÐ¾Ð»Ð¾Ð³Ð¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸, Ð²ÑÐ´ÐµÐ»ÑÐµÑÑÑ ÐºÐ»ÑÑÐµÐ²Ð°Ñ ÑÐ¾Ð»Ñ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐµÑÐµÐ¹ Ð² Ð¾ÑÐ¼ÑÑÐ»ÐµÐ½Ð¸Ð¸ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐ°ÐºÑÐ¸Ðº Ð² Ð¸ÑÑÐ¾ÑÐ¸Ð¸ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾ÑÑÐ¸. ÐÐ¾Ð´ÑÐµÑÐºÐ½ÑÑÐ° Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ Ð·Ð½Ð°ÑÐ¸Ð¼Ð¾ÑÑÑ ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ð¸ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸ Ð´Ð»Ñ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÐ¼ÑÑÐ»Ð¾Ð²Ð¾Ð³Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÑÐµÑÐ°Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÑÑÐ²Ð°. ÐÐ½Ð°Ð»Ð¸Ð·Ð¸ÑÑÐµÑÑÑ ÑÐ¾Ð»Ñ Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÑ ÑÐµÑÐµÐ¹ Ð² ÑÑÐ°Ð½ÑÐ»ÑÑÐ¸Ð¸ Ð¸ Ð»ÐµÐ³Ð¸ÑÐ¸Ð¼Ð°ÑÐ¸Ð¸ ÑÐµÐ½Ð½Ð¾ÑÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼, Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾ÑÐµÑÐ¸Ð²Ð¾ Ð¿ÑÐ¾ÑÐ²Ð»ÑÑÑÐ¸ÑÑÑ Ð² ÑÐµÐ°Ð»Ð¸ÑÑ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÑÑÐ²Ð°. ÐÐ±ÑÑÐ¶Ð´ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð½ÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÑÐµÑÑÑ Ð¾Ð±ÑÐµÐ¹ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ¾Ð¹: Â«Ð¤Ð¸Ð»Ð¾ÑÐ¾ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸ - ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸ÑÂ», - Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð² ÑÐ²ÑÐ·Ð¸ Ñ Ð¾Ð±Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐµÐ½Ð½Ð¾ÑÑÐµÐ¹ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÐ¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¾ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² ÐÑÑÐ³Ð»Ð¾Ð³Ð¾ ÑÑÐ¾Ð»Ð° Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼: Â«Ð¤Ð¸Ð»Ð¾ÑÐ¾ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸: Ð¸Ð½ÑÐµÐ»Ð»ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÐµ ÑÐµÑÐ¸ Ð¸ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð² Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¸Â», Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð½Ð¾Ð³Ð¾ 16 Ð½Ð¾ÑÐ±ÑÑ 2012 Ñ. Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ¾ÑÑÐ¼Ð° Â«ÐÐ½Ð¸ ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð¹ ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ð¸: ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ñ Ð¸ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¼ Ð¼Ð¸ÑÐµÂ». ÐÐ´ÑÐµÑÐ¾Ð²Ð°Ð½Ð¾ ÑÐ¸ÑÐ¾ÐºÐ¾Ð¼Ñ ÐºÑÑÐ³Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÐµÐ»ÐµÐ¹ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ¸Ð»Ð¾ÑÐ¾ÑÐ¸Ð¸, ÐºÑÐ»ÑÑÑÑÐ¾Ð»Ð¾Ð³Ð¸Ð¸, ÑÐ¾ÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð´ÑÑÐ³Ð¸Ñ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÐ°ÑÐ½Ð¾Ð³Ð¾ Ð·Ð½Ð°Ð½Ð¸Ñ.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÐÑÑÐ¾ Ð ÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ "Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ðµ ÑÐ¸Ð»Ð¾ÑÐ¾ÑÑÐºÐ¾Ðµ Ð¾Ð±ÑÐµÑÑÐ²Ð¾"
Electroweak scale neutrinos and decaying dark matter
Creators: name: Aranda, Alfredo
name: de Anda, Francisco J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We explore the scalar phenomenology of a model of electroweak scale neutrinos that incorporates the presence of a lepton number violating singlet scalar. An analysis of the pseudoscalar-Majoron field associated to this singlet field is carried out in order to verify the viability of the model and to restrict its parameter space. In particular we study the Majoron decay $J \to νν$ and use the bounds on the Majoron mass and width obtained in a modified Majoron Decaying Dark Matter scenario.
description: 8 pages, 6 figures. A discussion on the invisible Higgs decay mode present in the model and some references were added . Version to appear in PLB
MPEC 2024-C81 : 2024 CM1
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2024
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2024 CM1

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹ Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÑÐ¸Ð¿Ð¾Ð², ÐÐ½Ð°ÑÐ¾Ð»Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»Ð¸Ð·Ð°ÑÐ¸Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹
Ð¼Ð½Ð¾Ð³Ð¾ÑÐ´ÐµÑÐ½Ð¾ÑÑÑ
Ð²ÐµÐºÑÐ¾ÑÐ¸Ð·Ð°ÑÐ¸Ñ

description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÑÐµÐ¹ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ. Ð ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ, Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½Ð¾Ð¹ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼. ÐÑÐ½Ð¾Ð²Ð½Ð°Ñ Ð·Ð°Ð´Ð°ÑÐ° - Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð¿Ð¾Ð´ÑÐ¾Ð´Ñ ÑÐ°ÑÐ¿Ð°ÑÐ°Ð»Ð»ÐµÐ»Ð¸Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÐ¸ÑÐ»ÐµÐ½Ð¸Ð¹; Ð¸Ð·ÑÑÐ¸ÑÑ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹, Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¸ Ð´Ð»Ñ Ð¿Ð°ÑÐ°Ð»Ð»ÐµÐ»ÑÐ½Ð¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð² Ð²ÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ´ÑÐ°Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð°, Ð¿Ð¾ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐµ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ð¹.
title: ÐÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¨ÑÑÑÐ¿Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸Ñ
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð²ÑÑÑÐµÐ³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ 050400 Â«ÐÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¾Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸ÐµÂ». Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÐºÐ¾-Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹, ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¸ ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ±Ð¾ÑÐ°, Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¼Ð¿Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð´Ð°Ð½Ð½ÑÑ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¾Ð² Ð¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Â«Ð¡Ð¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÂ» Ð¸ Â«Ð¡Ð¾ÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸Ñ Ð² Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ð¸Â».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
No Neutron Star Companion To The Lowest Mass SDSS White Dwarf
Creators: name: Agueros, Marcel
name: Heinke, Craig
name: Camilo, Fernando
name: Kilic, Mukremin
name: Anderson, Scott
name: Freire, Paulo
name: Kleinman, Scot
name: Liebert, James
name: Silvestri, Nicole
Publisher: name: arXiv
Year: 2009
Subjects: subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: SDSS J091709.55+463821.8 (hereafter J0917+4638) is the lowest surface gravity white dwarf (WD) currently known, with log g = 5.55 +/- 0.05 (M ~ 0.17 M_sun; Kilic et al. 2007a,b). Such low-mass white dwarfs (LMWDs) are believed to originate in binaries that evolve into WD/WD or WD/neutron star (NS) systems. An optical search for J0917+4638's companion showed that it must be a compact object with a mass >= 0.28 M_sun (Kilic 2007b). Here we report on Green Bank Telescope 820 MHz and XMM-Newton X-ray observations of J0917+4638 intended to uncover a potential NS companion to the LMWD. No convincing pulsar signal is detected in our radio data. Our X-ray observation also failed to detect X-ray emission from J0917+4638's companion, while we would have detected any of the millisecond radio pulsars in 47 Tuc. We conclude that the companion is almost certainly another WD.
description: 4 pages, 1 table; to appear in the Astrophysical Journal Letters
Planar electric trap for neutral particles
Creators: name: Morinaga, Makoto
name: Kishimoto, Tetsuo
Publisher: name: arXiv
Year: 2009
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: FOS: Physical sciences

description: A new geometry to trap neutral particles with an ac electric field using a simple electrodes structure is described. In this geometry, all electrodes are placed on a single chip plane, while particles are levitated above the chip. This provides an easy construction of the trap and a good optical access to the trap.
description: 10 pages, 13 figures
Granger causality and the inverse Ising problem
Creators: name: Pellicoro, Mario
name: Stramaglia, Sebastiano
Publisher: name: arXiv
Year: 2010
Subjects: subject: Neurons and Cognition (q-bio.NC)
subject: Disordered Systems and Neural Networks (cond-mat.dis-nn)
subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Biological sciences
subject: FOS: Physical sciences

description: We study Ising models for describing data and show that autoregressive methods may be used to learn their connections, also in the case of asymmetric connections and for multi-spin interactions. For each link the linear Granger causality is two times the corresponding transfer entropy (i.e. the information flow on that link) in the weak coupling limit. For sparse connections and a low number of samples, the L1 regularized least squares method is used to detect the interacting pairs of spins. Nonlinear Granger causality is related to multispin interactions.
description: 6 pages and 8 figures. Revised version in press on Physica A
Confirming a Population of Hot-Dust Dominated, Star Forming Ultraluminous Galaxies at High-Redshift
Creators: name: Casey, C. M.
name: Chapman, S. C.
name: Beswick, R. J.
name: Biggs, A. D.
name: Blain, A. W.
name: Hainline, L. J.
name: Ivison, R. J.
name: Muxlow, T.
name: Smail, I.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We identify eight z>1 radio sources undetected at 850um but robustly detected at 70um, confirming that they represent ultraluminous infrared galaxies (ULIRGs) with hotter dust temperatures (T_dust=52+-10 K) than Submillimetre Galaxies (SMGs) at similar luminosities and redshifts. These galaxies share many properties with SMGs: ultra-violet (UV) spectra consistent with starbursts, high stellar masses and radio luminosities. We can attribute their radio emission to star formation since high-resolution MERLIN radio maps show extended emission regions (with half light radii of 2-3kpc), which are unlikely to be generated by AGN activity. These observations provide the first direct confirmation of hot, dusty ULIRGs which are missed by current submillimetre surveys. They have significant implications for future observations from the Herschel Space Observatory and SCUBA2, which will select high redshift luminous galaxies with less selection biases.
description: 9 pages, 6 figures; accepted for publication in MNRAS
title: ÐÑÐ¾ÐµÐºÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð´Ð¸Ð¾Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»Ð¾ÑÑ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ, ÐºÐ°Ðº Ð¡ÐÐÐ Ð´Ð»Ñ Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÐµÐ¹ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ ÑÑÐµÐ´ÑÑÐ²
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¦Ð¾Ð»Ð°Ð½, ÐÐ¼Ð¸ÑÑÐ¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ°Ð´Ð¸Ð¾Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð°
ÑÐ´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð»Ð¾ÑÑ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ
ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Ðµ ÑÑÐµÐ´ÑÑÐ²Ð¾
ÑÐ°Ð´Ð°Ñ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¾Ð¿Ð¸ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ Ð¿Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð´Ð¸Ð¾Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¿Ð¾Ð»Ð¾ÑÑ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð¾Ð±Ð·Ð¾Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ Ð¿Ð¾Ð¼Ð¾ÑÐ¸ Ð²Ð¾Ð´Ð¸ÑÐµÐ»Ñ Ð¿ÑÐ¸ ÑÐ´ÐµÑÐ¶Ð°Ð½Ð¸Ð¸ Ð¿Ð¾Ð»Ð¾ÑÑ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÐºÐ¾Ð½ÐºÑÑÐµÐ½ÑÐ½ÑÐµ Ð¿ÑÐµÐ¸Ð¼ÑÑÐµÑÑÐ²Ð° ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð³ÑÐ°ÑÐ¸Ðº ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ ÑÐµÑÑÑÑÑ Ð´Ð»Ñ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¾Ð¿ÑÑÐ½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·ÑÐ°. ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½ Ð»Ð¾Ð³Ð¸ÐºÐ¾-ÑÑÑÑÐºÑÑÑÐ½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ð´Ð»Ñ Ð»ÑÑÑÐµÐ³Ð¾ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ ÑÐµÐ»ÐµÐ¹ Ð¸ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼. Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð¼ ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð¾ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¿Ð°ÐºÐµÑÐ° Microsoft Project.
Fluctuations of Quantum Fields in a Classical Background and Reheating
Creators: name: Kaya, Ali
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We consider the particle creation process associated with a quantum field χin a time-dependent, homogeneous and isotropic, classical background. It is shown that the field square χ^2, the energy density and the pressure of the created particles have large fluctuations comparable to their vacuum expectation values. Possible effects of these fluctuations on the reheating process after inflation are discussed. After determining the correlation length of the fluctuations in two different models, corresponding to the decay in the parametric resonance regime and in the perturbation theory, it is found that these fluctuations should be taken into account in the final thermalization process, in the back-reaction effects and when the formation of primordial black holes is considered. In both models, by comparing quantum and thermal fluctuations with each other it is observed that very quick thermalization after the complete inflaton decay is not always possible even when the interaction rates are large. On the other hand, when the back-reaction effects are included during the preheating stage, the coherence of the inflaton oscillations is shown to be lost because of the fluctuations in χ^2. Finally, we note that a large fluctuation in the energy density may cause a black hole to form and we determine the fraction of total energy density that goes into such primordial black holes in the model of preheating we consider.
description: 14 pages, 1 figure, revtex4; v3:references added, a minor correction, to appear in Phys. Rev. D
Dynamics of entanglement via propagating microwave photons
Creators: name: Sabin, C.
name: Garcia-Ripoll, J. J.
name: Solano, E.
name: Leon, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We propose a simple circuit quantum electrodynamics (QED) experiment to test the generation of entanglement between two superconducting qubits. Instead of the usual cavity QED picture, we study qubits which are coupled to an open transmission line and get entangled by the exchange of propagating photons. We compute their dynamics using a full quantum field theory beyond the rotating-wave approximation and explore a variety of regimes which go from a weak coupling to the recently introduced ultrastrong coupling regime. Due to the existence of single photons traveling along the line with finite speed, our theory shows a light cone dividing the spacetime in two different regions. In one region, entanglement may only arise due to correlated vacuum fluctuations, while in the other the contribution from exchanged photons shows up.
description: v2: New version. 6 pages, 3 figures. Accepted in Phys. Rev. B.
Reversible MRI changes in a paediatric case of scurvy
Creators: name: Barros D'Sa, Ian
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Anatomy
subject: Paediatric
subject: Conventional radiography
subject: Image manipulation / Reconstruction
subject: MR
subject: Comparative studies
subject: Defecography
subject: Diagnostic procedure
subject: Biological effects

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 8 years
description: Clinical History: 8yr old girl with a history of eating disorder,(height 1.29m,50thcentile,weight 17.8kg, 0.4thcentile). Admitted for nasogastric feeding/psychiatry input. New right knee pain and difficulty walking. Iron deficiency anaemia on bloods. Pathological fracture/... Final Diagnosis: Scurvy
Melorheostosis
Creators: name: Oliveira, Maria
Publisher: name: EURORAD
Year: 2014
Subjects: subject: Bones
subject: CT
subject: Conventional radiography
subject: Diagnostic procedure
subject: Dysplasias

description: Clinical History Image Findings Discussion Find Diagnosis Differential Diagnosis
description: female, 80 years
description: Clinical History: The patient, an 80-year-old female, presented to the emergency department for respiratory distress. A chest x-ray and a CT scan were performed. The patient had clinical history of osteoarthritis. Final Diagnosis: Polyostotic Melorheostosis
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ½ÐµÑÐ³Ð¾ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸
Creators: name: Ð¯Ð´ÑÐºÐ¸Ð½, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: Ð­Ð½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¸
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿ÑÐµÐ´ÑÑÐ²Ð»ÑÐµÐ¼ÑÐµ Ðº ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÐ¼ ÐºÐ°Ðº Ðº ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¸ÑÑÐµÐ¼Ð°Ð¼, Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÑÑ ÑÑÐµÑ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐºÑÐ°, ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°. ÐÐ¾ÑÑÐ¾Ð¼Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ½ÐµÑÐ³Ð¾ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÑ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð´Ð»Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð² Ð½Ð° Ð¾Ð±Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ¾Ð½Ð´Ð¾Ð² Ñ ÑÑÐµÑÐ¾Ð¼ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ ÑÐ½ÐµÑÐ³Ð¾ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð½ÑÐ¹ Ð°Ð²ÑÐ¾ÑÐ¾Ð¼ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ½ÐµÑÐ³Ð¾ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÑ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¿Ð¾ÑÐ¾ÐºÐ¾Ð² Ð² Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¿ÑÐ¸ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ð¸ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾Ð³Ð¾ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐµÐºÑÐ°, Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ð¸ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¸ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð² Ð¼Ð°ÑÑÑÐ°Ð±Ðµ ÑÐµÐ³Ð¸Ð¾Ð½Ð°. Ð Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð°Ð²ÑÐ¾ÑÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¼Ð¸ Ð¿Ð¾ÑÐ¾ÐºÐ°Ð¼Ð¸ Ð½Ð° ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ ÑÐ½ÐµÑÐ³Ð¾ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ»ÐµÐºÑÑÐ¾ÑÐµÑÐµÐ²ÑÑ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¹ (Ð Ð¡Ð). Ð Ð°ÑÐºÑÑÑÑ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¿Ð¾ÑÐ¾ÐºÐ° ÐºÐ°Ð¿Ð¸ÑÐ°Ð»ÑÐ½ÑÑ Ð²Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹ Ð¸ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ° ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÐºÐ°Ð¿Ð¸ÑÐ°Ð»ÑÐ½ÑÑ Ð²Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ½ÐµÑÐ³Ð¾ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð Ð¡Ð.
Measurement of $B \to D_s^{(*)} Kπ$ branching fractions
Creators: name: The Belle Collaboration
name: Wiechczynski, J.
name: Lesiak, T.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: We report a measurement of the exclusive $B^+$ meson decay to the $D_s^{(*)-} K^+π^+$ final state using $657 \times 10^{6} B\overline{B}$ pairs collected at the $Υ(4S)$ resonance with the Belle detector at the KEKB asymmetric-energy $e^+e^-$ collider. We use $D_s^{*-}\to D_s^-γ$ and the $D_s^-\to ϕπ^-$, $\overline{K^{*}}(892)^0 K^-$ and $K^0_S K^-$ decay modes for $D_s^{(*)}$ reconstruction and measure the following branching fractions: ${\cal B}(B^+\to D_s^-K^+π^+)= (1.94^{+0.09}_{-0.08} ({\mathrm stat})^{+0.20}_{-0.20} {\mathrm (syst)} \pm 0.17 {\cal(B)})\times 10^{-4}$ and ${\cal B}(B^+\to D_s^{*-}K^+π^+)= (1.47^{+0.15}_{-0.14} ({\mathrm stat})^{+0.19}_{-0.19} ({\mathrm syst}) \pm 0.13 {\cal(B)})\times 10^{-4}$. The uncertainties are due to statistics, experimental systematic errors and uncertainties of intermediate branching fractions, respectively.
description: 10 pages, 4 figures, submitted to PRD
Fidelity and superconductivity in two-dimensional t-J models
Creators: name: Rigol, Marcos
name: Shastry, B. Sriram
name: Haas, Stephan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We compute the ground-state fidelity and various correlations to gauge the competition between different orders in two-dimensional t-J-type models. Using exact numerical diagonalization techniques, these quantities are examined for (i) the plain t-J and t-t'-J models, (ii) for the t-J model perturbed by infinite-range d-wave or extended-s-wave superconductivity inducing terms, and (iii) the t-J model, plain and with a d-wave perturbation, in the presence of non-magnetic quenched disorder. Various properties at low hole doping are contrasted with those at low electron filling. In the clean case, our results are consistent with previous work that concluded that the plain t-J model supports d-wave superconductivity. As a consequence of the strong correlations present in the low hole doping regime, we find that the magnitude of the d-wave condensate occupation is small even in the presence of large d-wave superconductivity inducing terms. In the dirty case, we show the robustness of the ground state in the strongly correlated regime against disorder.
description: 11 pages, 12 figures, as published
The role of noise and advection in absorbing state phase transitions
Creators: name: Barrett-Freeman, C.
name: Evans, M. R.
name: Marenduzzo, D.
name: Tailleur, J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study the effect of advection and noise on the field theory for directed percolation (DP). We show that even a very small advective velocity is enough to change the universality class of the dynamic phase transition. When the noise is taken to be proportional to the square root of the population density, we find an additional nonequilibrium 'spinodal' line separating a region where an exponentially decreasing density is metastable, from another one in which it is unstable. If the noise is instead linear in the density, the phase diagram changes dramatically both quantitatively and qualitatively, and the spinodal line becomes a true phase boundary. We briefly discuss possible applications of our results to microbial sedimentation and population dynamics in rivers.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Ð¿ÑÐ¸ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐµ Ð½Ð° 90 Ð¼ÐµÑÑ Ð² ÐÑÐ¸Ð¼Ð¾ÑÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ¾Ð½ÑÑÐµÐ², Ð Ð¾Ð¼Ð°Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ
ÑÐµÑÑÐ¾ÑÐ°Ð½
Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ°
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° Ð¿ÑÐ¸ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐµ Ð½Ð° 90 Ð¼ÐµÑÑ Ð² ÐÑÐ¸Ð¼Ð¾ÑÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Antiferromagnetic ordering induced by paramagnetic depairing in unconventional superconductors
Creators: name: Ikeda, Ryusuke
name: Hatakeyama, Yuhki
name: Aoyama, Kazushi
Publisher: name: arXiv
Year: 2010
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Antiferromagnetic (AFM) (or spin-density wave) quantum critical fluctuation enhanced just below H_c2(0) have been often observed in d-wave superconductors with a strong Pauli paramagnetic depairing (PD) including CeCoIn_5. It is shown here that such a tendency of field-induced AFM ordering is a consequence of strong PD and should appear particularly in superconductors with a gap node along the AFM modulation. Two phenomena seen in CeCoIn_5, the anomalous vortex lattice form factor and the AFM order in the Fulde-Ferrell-Larkin-Ovchinnikov state, are explained based on this peculiar PD effect.
description: 4 pages, 3 figures Title and text were changed. References are added. Resubmitted version
3q29_Bionano_SupplementaryFiles
Creators: name: Yilmaz, Feyza
Publisher: name: figshare
Year: 2021
Subjects: subject: 60408 Genomics
subject: FOS: Biological sciences
subject: 60102 Bioinformatics
subject: FOS: Computer and information sciences

description: 3q29 bionano genomics optical mapping molecule support for each haplotype and coordinates of haplotype segments.
PEMIKIRAN SØREN KIERKEGAARD TENTANG HAKIKAT AGAMA
Creators: name: Phangiano, Ricky
Publisher: name: figshare
Year: 2021
Subjects: subject: 60308 Life Histories
subject: FOS: Biological sciences

description: PEMIKIRAN SØREN KIERKEGAARD TENTANG HAKIKAT AGAMA
Replication of Carretero-Navarro et al (2019)
Creators: name: Murphy, Jennifer
name: Coyle, Taylor
name: Warne, Joe
Publisher: name: Open Science Framework
Year: 2023
Subjects: subject: sports science
subject: sports and exercise science
subject: replication
subject: kinesiology
subject: open science

description: Replication of the study titled "Effect of different loading conditions on running mechanics at different velocities" as part of the large replication project in the Sports Science Replication Centre
title: ÐÑÐ¾ÑÐµÑÑÑ Ð´ÐµÑÐ¾ÐºÑÐ¸ÐºÐ°ÑÐ¸Ð¸ Ð¿ÑÐ¸ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¸ Ñ Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð²ÐµÑÐµÑÑÐ² Ð½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð¼
Creators: name: Ð ÐµÐ¼Ð±Ð¾Ð²ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ¾Ð³Ð¸Ð»ÐµÐ½ÐºÐ¾Ð²Ð°, ÐÑÐ±Ð¾Ð²Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2017
Subjects: Ð¥Ð¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð²ÐµÑÐµÑÑÐ²Ð°
ÐÐ¼Ð¼ÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ
Ð´ÐµÑÐ¾ÐºÑÐ¸ÐºÐ°ÑÐ¸Ñ
ÐºÑÐµÐ½Ð¾Ð±Ð¸Ð¾ÑÐ¸ÐºÐ¸

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ Ð¼Ð¾Ð½Ð¾Ð³ÑÐ°ÑÐ¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾Ð± Ð¾Ð±ÐµÐ·Ð²ÑÐµÐ¶Ð¸Ð²Ð°Ð½Ð¸Ð¸
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ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¾ÑÐ³Ð°Ð½Ð¾Ð² (Ð¼ÐµÐ¶ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ Ð¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ), ÑÐµÐ½ÑÑÐ¾Ð² Ð³Ð¸Ð³Ð¸ÐµÐ½Ñ Ð¸ ÑÐ¿Ð¸Ð´ÐµÐ¼Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¤ÐÐÐ Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ Ð´ÑÑÐ³Ð¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ¾Ð², Ð¾ÑÑÑÐµÑÑÐ²Ð»ÑÑÑÐ¸Ñ Ð¼ÐµÐ´Ð¸ÐºÐ¾-Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ðµ ÑÐ¾Ð¿ÑÐ¾Ð²Ð¾Ð¶Ð´ÐµÐ½Ð¸Ðµ ÑÐ°Ð±Ð¾Ñ Ð½Ð° Ð¾Ð¿Ð°ÑÐ½ÑÑ ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ Ð¸ Ð´Ñ.
title: Ð¡Ð¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ðµ ÑÑÐ´ÐµÐ¹ÑÑÐ²Ð¾ ÐºÐ°Ðº ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸
title: Sports refereeing as a component of sports training
Creators: name: ÐÐµÑÐµÐ²Ð¸ÑÐºÐ¸Ð¹, ÐÐ²Ð°Ð½
name: Ð¢Ð°Ð¼Ð±Ð¾Ð²ÑÐºÐ¸Ð¹, ÐÐ½Ð°ÑÐ¾Ð»Ð¸Ð¹
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ðµ ÑÑÐ´ÐµÐ¹ÑÑÐ²Ð¾
ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐ¾ÑÑÑÐ·Ð°Ð½Ð¸Ðµ
ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ðµ ÑÐ¾ÑÐµÐ²Ð½Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð°Ñ ÑÑÐµÐ½Ð¸ÑÐ¾Ð²ÐºÐ°
ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ°
sports refereeing
sports competition
sports training

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸Ð½ÑÑÐ° Ð¿Ð¾Ð¿ÑÑÐºÐ° ÐºÐ¾Ð½ÐºÑÐµÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð² ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ð¼ÐµÑÑÐ° ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÑÐ´ÐµÐ¹ÑÑÐ²Ð°, Ð² ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ð² ÑÑÐ°ÑÑÐµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ðµ ÑÑÐ´ÐµÐ¹ÑÑÐ²Ð¾ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¾ ÐºÐ°Ðº ÑÐµÐ»Ð¾ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸.
description: In this paper, an attempt is made to concretize the place of sports refereeing in sports training, because the development of the model presented in the article, sports refereeing is justified as an integral component of sports training.
Angular Energy Distribution of Collapsar-Jets
Creators: name: Mizuta, Akira
name: Aloy, Miguel A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Collapsars are fast-spinning, massive stars, whose core collapse liberates an energy, that can be channeled in the form of ultrarelativistic jets. These jets transport the energy from the collapsed core to large distances, where it is dissipated in the form of long-duration gamma-ray bursts. In this paper we study the dynamics of ultrarelativistic jets produced in collapsars. Also we extrapolate our results to infer the angular energy distribution of the produced outflows in the afterglow phase. Our main focus is to look for global energetical properties which can be imprinted by the different structure of different progenitor stars. Thus, we employ a number of pre-supernova, stellar models (with distinct masses and metallicities), and inject in all of them jets with fixed initial conditions. We assume that at the injection nozzle, the jet is mildly relativistic (Lorentz factor $\sim 5$), has a finite half-opening angle ($5^\circ$), and carries a power of $10^{51} $erg s$^{-1}$. These jets arrive intact to the stellar surface and break out of it. A large Lorentz factor region $Γ\simmore 100$ develops well before the jet reaches the surface of the star, in the unshocked part of the beam, located between the injection nozzle and the first recollimation shock. These high values of $Γ$ are possible because the finite opening angle of the jet allows for free expansion towards the radial direction. We find a strong correlation between the angular energy distribution of the jet, after its eruption from the progenitor surface, and the mass of the progenitors. The angular energy distribution of the jets from light progenitor models is steeper than that of the jets injected in more massive progenitor stars. This trend is also imprinted in the angular distribution of isotropic equivalent energy.
description: 16 pages, 18 figures, accepted for publication in ApJ, high resolution figures are available at http://www.cfs.chiba-u.ac.jp/~mizuta/ms15.pdf
Negative human-crocodile interactions in Kariba, Zimbabwe: data to support potential mitigation strategies
Creators: name: MATANZIMA, Joshua
name: Marowa, I
name: Nhiwatiwa, T
Publisher: name: La Trobe
Year: 2024
Subjects: classificationCode: 4104
subject: Environmental management
classificationCode: 3103
subject: Ecology
subject: FOS: Biological sciences
classificationCode: 3109
subject: Zoology

description: Interactions between people and wild animals often result in negative impacts, and different views on the management of such interactions can lead to conflicts. Both intentional and unintentional negative human-wildlife interactions are increasing problems in many places where people share space with wild animals. Here we focus on negative interactions between people and Nile crocodiles Crocodylus niloticus in and around Lake Kariba in Zimbabwe. In the study area, crocodile attacks on people occur frequently, leading to people being injured or killed, which in turn prompts retaliatory actions against crocodiles. However, despite the negative impact of such interactions on both people and crocodiles, little is known about the spatio-temporal patterns of crocodile attacks or environmental conditions under which attacks occur. We collected information about crocodile attacks on people that occurred during 2000-2020, including the date, time, season and location of attacks, the age of victims and the activities they were carrying out when attacks occurred, and water conditions during attacks. We analysed these data to discern patterns and trends of crocodile attacks on people. Attacks occurred in clear as well as turbid water, and nearly half of all reported attacks were at night or in the early morning. The locations with the highest number of recorded attacks were Nyanyana and Charara lakeside, and the fewest attacks occurred at Andora harbour. Most victims were 26-40 years old, and most were attacked in the dry-hot season, while they were fishing. Our findings can be used to design area-specific mitigation strategies to reduce negative human-crocodile interactions.
Band Structure, Phase transitions and Semiconductor Analogs in One-Dimensional Solid Light Systems
Creators: name: Quach, James
name: Makin, Melissa I.
name: Su, Chun-Hsu
name: Greentree, Andrew D.
name: Hollenberg, Lloyd C. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The conjunction of atom-cavity physics and photonic structures (``solid light'' systems) offers new opportunities in terms of more device functionality and the probing of designed emulators of condensed matter systems. By analogy to the canonical one-electron approximation of solid state physics, we propose a one-polariton approximation to study these systems. Using this approximation we apply Bloch states to the uniformly tuned Jaynes-Cummings-Hubbard model to analytically determine the energy band structure. By analyzing the response of the band structure to local atom-cavity control we explore its application as a quantum simulator and show phase transition features absent in mean field theory. Using this novel approach for solid light systems we extend the analysis to include detuning impurities to show the solid light analogy of the semiconductor. This investigation also shows new features with no semiconductor analog.
description: 7 pages
title: Ð Ð°ÑÑÐµÑ Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐ¸Ð²Ð¾ÑÐ°Ð·ÑÑÐ´Ð½ÑÑ Ð¿Ð¾ÐºÑÑÑÐ¸Ð¹ Ð¾Ð±Ð¼Ð¾ÑÐ¾Ðº ÑÑÐ°ÑÐ¾ÑÐ° Ð¼Ð¾ÑÐ½ÑÑ Ð³ÐµÐ½ÐµÑÐ°ÑÐ¾ÑÐ¾Ð²
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¸Ð¼ÐµÑÐ¾Ð², ÐÐ°Ð¼Ð¸Ð»Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐ±Ð¼Ð¾ÑÐºÐ¸ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð°ÑÐ¸Ð½
Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾Ð»Ðµ
Ð­Ð»ÐµÐºÑÑÐ¾Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½Ð°Ñ
Ð²Ð¾Ð·Ð´ÑÑÐ½ÑÐµ Ð²ÐºÐ»ÑÑÐµÐ½Ð¸Ñ

description: ÐÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½ÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð°ÑÐ¸Ð½ (Ð­Ð) Ð¼Ð¾Ð³ÑÑ Ð¿ÑÐ¾Ð¸ÑÑÐ¾Ð´Ð¸ÑÑ ÑÐ°ÑÑÐ¸ÑÐ½ÑÐµ ÑÐ°Ð·ÑÑÐ´Ñ Ð² ÑÐ¾Ð»ÑÐµ Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¸ Ð¸ Ð½Ð° ÐµÐµ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸. ÐÐ»Ñ Ð¸Ñ Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ñ Ð¸ ÑÑÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐ°ÑÑÐµÑ ÑÐ°ÑÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð² ÑÐ¸ÑÑÐµÐ¼Ðµ Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¸ Ð²ÑÑÐ¾ÐºÐ¾Ð²Ð¾Ð»ÑÑÐ½Ð¾Ð¹ Ð¾Ð±Ð¼Ð¾ÑÐºÐ¸ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Comsol 5.2Ð°. Ð Ð°ÑÑÐµÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð», ÑÑÐ¾ Ð½Ð°Ð½ÐµÑÐµÐ½Ð¸Ðµ Ð´Ð²ÑÑÑÑÑÐ¿ÐµÐ½ÑÐ°ÑÐ¾Ð³Ð¾ Ð¿Ð¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐµÐ³Ð¾ Ð¿Ð¾ÐºÑÑÑÐ¸Ñ Ð½Ð° Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÑ Ð¸Ð·Ð¾Ð»ÑÑÐ¸Ð¸ Ð² Ð»Ð¾Ð±Ð¾Ð²Ð¾Ð¹ ÑÐ°ÑÑÐ¸ Ð·Ð½Ð°ÑÐ¸ÑÐµÐ»ÑÐ½Ð¾ ÑÐ½Ð¸Ð¶Ð°ÐµÑ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð½Ð¾ÑÑÑ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð»Ñ. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð½ÑÐµ ÑÐ¾ÑÐµÑÐ°Ð½Ð¸Ñ ÑÑÑÐºÐ¾Ð² Ð¿Ð¾ÐºÑÑÑÐ¸Ð¹ Ð¼Ð¾Ð³ÑÑ Ð»ÑÑÑÐµ Ð²ÑÑÐ°Ð²Ð½Ð¸Ð²Ð°ÑÑ ÐºÐ°ÑÑÐ¸Ð½Ñ Ð¿Ð¾Ð»Ñ
title: ÐÐ¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ° Ð¸ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ°
title: ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÐºÑÑÑÑ
titleType: Subtitle
Creators: name: Ð¡Ð¾ÐºÐ¾Ð²Ð¸ÑÐ¸Ð½, Ð®ÑÐ¸Ð¹
Publisher: name: ÐÐÐ]
Year: 1971
Subjects: ÐÐ¸Ð´ÑÐ¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ°
ÐÐ°Ð·Ð¾Ð²Ð°Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ°

description: Ð ÐµÑÐµÐ½Ð¸Ðµ ÑÑÐ´Ð° Ð·Ð°Ð´Ð°Ñ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸ÐµÐ¼ ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ñ, Ð½Ð°ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾ ÑÑÐµÐ±ÑÐµÑ ÑÐ³Ð»ÑÐ±Ð»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐ¸Ñ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² Ð³Ð¸Ð´ÑÐ¾Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸. Ð¡ÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð·Ð°Ð´Ð°ÑÐ½Ð¸ÐºÐ¸ Ð¿Ð¾ ÐºÑÑÑÑ Ð¸Ð·-Ð·Ð° Ð³ÑÐ¾Ð¼Ð¾Ð·Ð´ÐºÐ¾ÑÑÐ¸ Ð¸ ÑÑÑÐ´Ð¾ÐµÐ¼ÐºÐ¾ÑÑÐ¸ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð½Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ñ Ð¿ÑÐ¸Ð¼ÐµÑÐ¾Ð² ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÑ Ð·Ð°Ð´Ð°Ñ. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ Ð²ÐºÐ»ÑÑÐ°ÐµÑ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ð°Ð¼ ÐºÑÑÑÐ°: Ð³Ð¸Ð´ÑÐ°Ð²Ð»Ð¸ÐºÐ° ÑÑÑÐ±Ð¾Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¾Ð², Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ ÑÐ°Ð±Ð¾ÑÐ¸Ñ ÑÐµÐ» Ð² ÑÐ¾Ð¿Ð»Ð°Ñ, Ð¿Ð»Ð¾ÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐ¸, Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ðº ÑÐ°ÑÑÐµÑÐ°Ð¼ ÑÐ²ÐµÑÑÐ·Ð²ÑÐºÐ¾Ð²ÑÑ ÑÐµÑÐµÐ½Ð¸Ð¹ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿Ð¾Ð³ÑÐ°Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ»Ð¾Ñ. Ð Ð·Ð°Ð´Ð°Ð½Ð¸Ð¸ ÐºÑÐ°ÑÐºÐ¾ Ð¸Ð·Ð»Ð°Ð³Ð°ÐµÑÑÑ ÑÐµÐ¾ÑÐ¸Ñ, Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ Ð¿ÑÐ¸Ð¼ÐµÑ ÑÐ°ÑÑÐµÑÐ° Ð¸ Ð²Ð°ÑÐ¸Ð°Ð½ÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ. ÐÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐµ Ð·Ð°Ð´Ð°Ð½Ð¸Ñ Ð¼Ð¾Ð³ÑÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼Ð¸ ÑÐ½ÐµÑÐ³Ð¾Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÑ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹ Ð´Ð½ÐµÐ²Ð½Ð¾Ð³Ð¾, Ð²ÐµÑÐµÑÐ½ÐµÐ³Ð¾ Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ¾Ð². ÐÐ°Ð´Ð°Ð½Ð¸Ñ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ñ Ðº Ð¿ÐµÑÐ°ÑÐ¸ Ð´Ð¾ÑÐµÐ½ÑÐ¾Ð¼ ÐºÐ°ÑÐµÐ´ÑÑ Ð®. Ð. Ð¡Ð¾ÐºÐ¾Ð²Ð¸ÑÐ¸Ð½ÑÐ¼.
Universal Kaluza-Klein reductions of type IIB to N=4 supergravity in five dimensions
Creators: name: Gauntlett, Jerome P.
name: Varela, Oscar
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct explicit consistent Kaluza-Klein reductions of type IIB supergravity on HK_4 x S^1, where HK_4 is an arbitrary four-dimensional hyper-Kaehler manifold, and on SE5, an arbitrary five-dimensional Sasaki-Einstein manifold. In the former case we obtain the bosonic action of D=5 N=4 (ungauged) supergravity coupled to two vector multiplets. For the SE_5 case we extend a known reduction, which leads to minimal D=5 N=2 gauged supergravity, to also include a multiplet of massive fields, containing the breathing mode of the SE_5. We show that the resulting D=5 action is also consistent with N=4 gauged supergravity coupled to two vector multiplets. This theory has a supersymmetric AdS_5 vacuum, which uplifts to the class of supersymmetric AdS_5 x SE_5 solutions, that spontaneously breaks N=4 to N=2, and also a non-supersymmetric AdS_5 vacuum which uplifts to a class of solutions first found by Romans.
description: 1+34 pages. v2: Minor typos corrected, three references added. Version to be published in JHEP