Test of exotic scalar and tensor interactions in K_e3 decay using stopped positive kaons

The form factors of the decay K+ --> pi0 e+ nu (K_e3) have been determined from the comparison of the experimental and Monte Carlo Dalitz distributions containing about 10^5 K_e3 events. The following values of the parameters were obtained: lambda_+ = 0.0278 +- 0.0017(stat) +- 0.0015(syst), f_S/f_+(0) = 0.0040 +- 0.0160(stat) +- 0.0067(syst) and f_T/f_+(0) = 0.019 +- 0.080(stat) +- 0.038(syst). Both scalar f_S and tensor f_T form factors are consistent with the Standard Model predictions of zero values.Comment: 10 pages, 5 figures, contributed to the proceedings of NANP Conference, Dubna, June 19-23, 200

Spectroscopic Evidence for the Localization of Skyrmions near Nu=1 as T->0

Optically pumped nuclear magnetic resonance measurements of Ga-71 spectra were carried out in an n-doped GaAs/Al0.1Ga0.9As multiple quantum well sample near the integer quantum Hall ground state Nu=1. As the temperature is lowered (down to T~0.3 K), a ``tilted plateau'' emerges in the Knight shift data, which is a novel experimental signature of quasiparticle localization. The dependence of the spectra on both T and Nu suggests that the localization is a collective process. The frozen limit spectra appear to rule out a 2D lattice of conventional skyrmions.Comment: 4 pages (REVTEX), 5 eps figures embedded in text, published versio

Dynamic nuclear polarization and spin-diffusion in non-conducting solids

There has been much renewed interest in dynamic nuclear polarization (DNP), particularly in the context of solid state biomolecular NMR and more recently dissolution DNP techniques for liquids. This paper reviews the role of spin diffusion in polarizing nuclear spins and discusses the role of the spin diffusion barrier, before going on to discuss some recent results.Comment: submitted to Applied Magnetic Resonance. The article should appear in a special issue that is being published in connection with the DNP Symposium help in Nottingham in August 200

Hamiltonian theory of gaps, masses and polarization in quantum Hall states: full disclosure

I furnish details of the hamiltonian theory of the FQHE developed with Murthy for the infrared, which I subsequently extended to all distances and apply it to Jain fractions \nu = p/(2ps + 1). The explicit operator description in terms of the CF allows one to answer quantitative and qualitative issues, some of which cannot even be posed otherwise. I compute activation gaps for several potentials, exhibit their particle hole symmetry, the profiles of charge density in states with a quasiparticles or hole, (all in closed form) and compare to results from trial wavefunctions and exact diagonalization. The Hartree-Fock approximation is used since much of the nonperturbative physics is built in at tree level. I compare the gaps to experiment and comment on the rough equality of normalized masses near half and quarter filling. I compute the critical fields at which the Hall system will jump from one quantized value of polarization to another, and the polarization and relaxation rates for half filling as a function of temperature and propose a Korringa like law. After providing some plausibility arguments, I explore the possibility of describing several magnetic phenomena in dirty systems with an effective potential, by extracting a free parameter describing the potential from one data point and then using it to predict all the others from that sample. This works to the accuracy typical of this theory (10 -20 percent). I explain why the CF behaves like free particle in some magnetic experiments when it is not, what exactly the CF is made of, what one means by its dipole moment, and how the comparison of theory to experiment must be modified to fit the peculiarities of the quantized Hall problem

Ретроперитонеоскопический доступ при органосохраняющем лечении почечно-клеточного рака

Background. Renal cell carcinoma is one of the most common urologic cancers. Due to development of modern diagnostic methods, kidney tumors are often diagnosed at early stages (cT1a-T1b). The golden standard of treatment of localized renal cell carcinoma is tumor resection. In retroperitoneoscopic access, the time to artery access is decreased, the risk of intra- and postoperative complications is reduced. Retroperitoneal access is preferable for tumors located on the lateral or posterior kidney surface.Aim. To analyze the results of treatment of patients after retroperitoneoscopic kidney resection.Materials and methods. Between 2018 and 2021, at the A.F. Tsyb Medical Radiological Research Center - branch of the National Medical Research Radiological Center 47 retroperitoneoscopic kidney resections were performed (29 (61.7 %) in men, 18 (38.3 %) in women) due to stage cT1aN0M0 renal cell carcinoma. Retrospective analysis of demographic data, comorbid status, tumor characteristics, operative time, blood loss volume, frequency and severity of complications per the Clavien-Dindo classification was performed. Complexity of resection was evaluated using the R.E.N.A.L. scale.Results. Mean patient age was 63 (38-79) years, body mass index was 29.9 (22-39) kg/m2. Tumor of the left kidney was diagnosed in 24 (51.0 %) cases, of the right kidney - in 22 (46.8 %) cases, bilateral lesions - in 1 (2.2 %) case. Mean tumor size was 22.4 (11-39) mm. Resection had low complexity in 35 (74.5 %) cases, intermediate complexity in 12 (25.5 %) cases. Mean operative time was 156 (80-280) minutes, mean warm ischemia time was 19 (7-32) minutes, number of resections with zero ischemia was 15 (31.9 %), mean blood loss volume was 53 (10-300) mL, number of resections without renal parenchyma suturing was 10 (21.3 %). Mean hospitalization time after surgery was 5 days. Postoperative complications were observed in 4 (8.5 %) cases: bleeding (severity grade II per the Clavien-Dindo classification) in 1 (2.1 %) case, postoperative infectious complications (severity grade II) - in 2 (4.2 %) cases, subcutaneous hematoma (severity grade I) - in 1 (2.1 %) case.Conclusion. Retroperitoneoscopic access is effective and safe. This is confirmed by low frequency and severity of postoperative complications. This access allows to reduce hospitalization time and pain management medication which accelerates patient mobilization and recovery. Comparative analysis shows that retroperitoneoscopic kidney resection has the same effectiveness as laparoscopic resection.Введение. Почечно-клеточный рак - одно из наиболее распространенных онкоурологических заболеваний. Благодаря развитию современных методов диагностики опухоли почек часто выявляются на ранней стадии (cT1a-T1b). «Золотым стандартом» лечения локализованного почечно-клеточного рака является резекция почки. При ретроперитонеоскопическом доступе уменьшается время доступа к артерии, снижается риск развития интра- и послеоперационных осложнений. Забрюшинный доступ предпочтителен при расположении опухоли по латеральной или по задней поверхности почки.Цель исследования - проанализировать результаты лечения пациентов после ретроперитонеоскопической резекции почки.Материалы и методы. С 2018 по 2021 г. на базе МРНЦ им. А.Ф. Цыба - филиала НМИЦ радиологии было выполнено 47 ретроперитонеоскопических резекций почки (29 (61,7 %) мужчинам, 18 (38,3 %) женщинам) по поводу почечно-клеточного рака с клинической стадией cT1aN0M0. Проведен ретроспективный анализ демографических данных, коморбидного статуса, характеристик опухоли, длительности операции, объема кровопотери, частоты и тяжести осложнений по классификации Clavien-Dindo. Сложность резекции оценивали по шкале R.E.N.A.L.Результаты. Средний возраст пациентов составил 63 (38-79) года, индекс массы тела - 29,9 (22-39) кг/м2. Опухоль левой почки имела место в 24 (51,0 %) случаях, правой - в 22 (46,8 %), двустороннее поражение - в 1 (2,2 %). Средний размер опухоли составил 22,4 (11-39) мм. Количество резекций низкой сложности было в 35 (74,5 %) случаях, умеренной сложности - в 12 (25,5 %). Средняя продолжительность операции составила 156 (80-280) мин, среднее время тепловой ишемии - 19 (7-32) мин, количество резекций в условиях «нулевой» ишемии - 15 (31,9 %), средний объем кровопотери - 53 (10-300) мл, количество резекций без ушивания почечной паренхимы - 10 (21,3 %). Средняя продолжительность пребывания в стационаре после операции - 5 дней. Послеоперационные осложнения зарегистрированы в 4 (8,5 %) случаях: кровотечение (II степень тяжести по классификации Clavien-Dindo) - в 1 (2,1 %), послеоперационные инфекционные осложнения (II степень тяжести) - в 2 (4,2 %), подкожная гематома (I степень тяжести) - в 1 (2,1 %).Заключение. Ретроперитонеоскопический доступ является эффективным и безопасным. Об этом свидетельствуют низкие частота и степень тяжести послеоперационных осложнений. Данный доступ позволяет уменьшить продолжительность госпитализации и снизить потребность в обезболивании, что ускоряет активизацию и восстановление пациентов. При сравнительном анализе установлено, что ретроперитонеоскопическая резекция почки не уступает по эффективности лапароскопической резекции

Morphino: A nature-inspired tool for the design of shape-changing interfaces

The HCI community has a strong and growing interest in shape-changing interfaces (SCIs) that can offer dynamic af- fordance. In this context, there is an increasing need for HCI researchers and designers to form close relationships with dis- ciplines such as robotics and material science in order to be able to truly harness the state-of-the-art in morphing technolo- gies. To help these synergies arise, we present Morphino: a card-based toolkit to inspire shape-changing interface designs. Our cards bring together a collection of morphing mechanisms already established in the multidisciplinary literature and illustrate them through familiar examples from nature. We begin by detailing the design of the cards, based on a review of shape-change in nature; then, report on a series of design sessions conducted to demonstrate their usefulness in generating new ideas and in helping end-users gain a better understanding of the possibilities for shape-changing materials

Редкая злокачественная опухоль почки – лейомиосаркома почечной вены (клинический случай)

Soft tissue sarcomas are a rare group of malignant tumors that develop from different types of connective tissue. One of the histological variants of primary renal sarcoma is renal leiomyosarcoma. Leiomyosarcoma of kidneys can develop from the renal vasculature, renal veins, pelvic muscles, smooth muscle components of the renal capsule. Clinical and radiologic signs of leiomyosarcoma are nonspecific. Diagnosis is based on histological and immunohistochemical studies after surgical intervention. This article presents a clinical case of diagnosis and treatment of leiomyosarcoma of the renal vein.Саркомы мягких тканей – редкая группа злокачественных опухолей, развивающихся из разных типов соединительной ткани. Одним из гистологических вариантов первичной саркомы почки является лейомиосаркома. Лейомиосаркома почки может развиваться из почечной сосудистой сети, почечных вен, мышц лоханки, гладкомышечных элементов почечной капсулы. Клинические и рентгенологические признаки лейомиосаркомы неспецифичны. Основой диагностики является проведение гистологического и иммуногистохимического исследования после выполнения хирургического вмешательства. В настоящей статье представлен клинический случай диагностики и лечения лейомиосаркомы почечной вены

Multiwavelength behaviour of the blazar 3C 279: decade-long study from γ-ray to radio

We report the results of decade-long (2008–2018) γ-ray to 1 GHz radio monitoring of the blazar 3C 279, including GASP/WEBT, Fermi and Swift data, as well as polarimetric and spectroscopic data. The X-ray and γ-ray light curves correlate well, with no delay ≳3 h, implying general cospatiality of the emission regions. The γ-ray–optical flux–flux relation changes with activity state, ranging from a linear to a more complex dependence. The behaviour of the Stokes parameters at optical and radio wavelengths, including 43 GHz Very Long Baseline Array images, supports either a predominantly helical magnetic field or motion of the radiating plasma along a spiral path. Apparent speeds of emission knots range from 10 to 37c, with the highest values requiring bulk Lorentz factors close to those needed to explain γ-ray variability on very short time-scales. The Mg II emission line flux in the ‘blue’ and ‘red’ wings correlates with the optical synchrotron continuum flux density, possibly providing a variable source of seed photons for inverse Compton scattering. In the radio bands, we find progressive delays of the most prominent light-curve maxima with decreasing frequency, as expected from the frequency dependence of the τ = 1 surface of synchrotron self-absorption. The global maximum in the 86 GHz light curve becomes less prominent at lower frequencies, while a local maximum, appearing in 2014, strengthens toward decreasing frequencies, becoming pronounced at ∼5 GHz. These tendencies suggest different Doppler boosting of stratified radio-emitting zones in the jet

Multiwavelength behaviour of the blazar 3C 279: Decade-long study from γ -ray to radio

We report the results of decade-long (2008-2018) γ -ray to 1 GHz radio monitoring of the blazar 3C 279, including GASP/WEBT, Fermi and Swift data, as well as polarimetric and spectroscopic data. The X-ray and γ -ray light curves correlate well, with no delay ≳ 3 h, implying general cospatiality of the emission regions. The γ -ray-optical flux-flux relation changes with activity state, ranging from a linear to amore complex dependence. The behaviour of the Stokes parameters at optical and radio wavelengths, including 43 GHz Very Long Baseline Array images, supports either a predominantly helical magnetic field or motion of the radiating plasma along a spiral path. Apparent speeds of emission knots range from 10 to 37c, with the highest values requiring bulk Lorentz factors close to those needed to explain γ -ray variability on very short time-scales. The MgII emission line flux in the 'blue' and 'red' wings correlates with the optical synchrotron continuum flux density, possibly providing a variable source of seed photons for inverse Compton scattering. In the radio bands, we find progressive delays of the most prominent light-curve maxima with decreasing frequency, as expected from the frequency dependence of the τ= 1 surface of synchrotron self-absorption. The global maximum in the 86 GHz light curve becomes less prominent at lower frequencies, while a local maximum, appearing in 2014, strengthens toward decreasing frequencies, becoming pronounced at ∼5 GHz. These tendencies suggest different Doppler boosting of stratified radio-emitting zones in the jet. © 2020 The Author(s).We thank the referee for attentive reading and comments that helped to improve presentation of the manuscript. The data collected by the WEBT collaboration are stored in the WEBT archive at the Osservatorio Astrofisico di Torino -INAF (ht tp://www.oato.inaf.it/blazars/webt/); for questions regarding their availability, please contact the WEBT President Massimo Villata([email protected]).TheSt.Petersburg University team acknowledges support from Russian Science Foundation grant 17-12-01029. The research at BU was supported in part by National Science Foundation grant AST-1615796 and NASA Fermi Guest Investigator grants 80NSSC17K0649, 80NSSC19K1504, and 80NSSC19K1505. The PRISM camera at Lowell Observatory was developed by K. Janes et al. at BU and Lowell Observatory, with funding from the NSF, BU, and Lowell Observatory. The emission-line observations made use of the DCT at Lowell Observatory, supported by Discovery Communications, Inc., BU, the University of Maryland, the University of Toledo, and Northern Arizona University. The VLBA is an instrument of the National Radio Astronomy Observatory. The National Radio Astronomy Observatory is a facility of the US NSF, operated under cooperative agreement by Associated Universities, Inc. This research has used data from the UMRAO which was supported by the University of Michigan; research at this facility was supported by NASA under awards NNX09AU16G, NNX10AP16G, NNX11AO13G, and NNX13AP18G, and by the NSF under award AST-0607523. The Steward Observatory spectropolarimetric monitoring project was supported by NASA Fermi Guest Investigator grants NNX08AW56G, NNX09AU10G, NNX12AO93G, and NNX15AU81G. The Torino group acknowledges financial contribution from agreement ASI-INAF n.2017-14-H.0 and from contract PRIN-SKA-CTA-INAF 2016. I.A. acknowledges support by a Ramon y Cajal grant (RYC-2013-14511) of the 'Ministerio de Ciencia, Innovacion, y Universidades (MICIU)' of Spain and from MCIU through the 'Center of Excellence Severo Ochoa' award for the Instituto de Astrofisica de Andalucia-CSIC (SEV-20170709). Acquisition and reduction of the POLAMI and MAPCAT data were supported by MICIU through grant AYA2016-80889-P. The POLAMI observations were carried out at the IRAM 30-m Telescope, supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain). The MAPCAT observations were carried out at theGerman-Spanish Calar Alto Observatory, jointly operated by the Max-Plank-Institut fur Astronomie and the Instituto de Astrofisica de Andalucia-CSIC. The study is based partly on data obtained with the STELLA robotic telescopes in Tenerife, an AIP facility jointly operated by AIP and IAC. The OVRO 40-m monitoring program is supported in part by NASA grants NNX08AW31G, NNX11A043G, and NNX14AQ89G, and NSF grants AST-0808050 and AST-1109911. TH was supported by the Academy of Finland projects 317383 and 320085. AZT-24 observations were made within an agreement between Pulkovo, Rome and Teramo observatories. The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. The Abastumani team acknowledges financial support by the Shota Rustaveli National Science Foundation under contract FR/217950/16. r This research was partially supported by the Bulgarian National Science Fund of the Ministry of Education and Science under grants DN 081/2016, DN 18-13/2017, KP-06-H28/3 (2018), and KP-06-PN38/1 (2019), Bulgarian National Science Programme 'Young Scientists and Postdoctoral Students 2019', Bulgarian National Science Fund under grant DN18-10/2017 and National RI Roadmap Projects DO1-157/28.08.2018 and DO1-153/28.08.2018 of the Ministry of Education and Science of the Republic of Bulgaria. GD and OV gratefully acknowledge observing grant support from the Institute of Astronomy and Rozhen National Astronomical Observatory via bilateral joint research project `Study of ICRF radio-sources and fast variable astronomical objects' (head -G. Damljanovic). This work was partly supported by the National Science Fund of the Ministry of Education and Science of Bulgaria under grant DN 08-20/2016, and by project RD-08-37/2019 of the University of Shumen. This work is a part of projects nos 176011, 176004, and 176021, supported by theMinistry of Education, Science and Technological Development of the Republic of Serbia. MGM acknowledges support through the Russian Government Program of Competitive Growth of Kazan Federal University. The Astronomical Observatory of the Autonomous Region of the Aosta Valley (OAVdA) is managed by the Fondazione Clement Fillietroz-ONLUS, which is supported by the Regional Government of the Aosta Valley, the Town Municipality of Nus and the 'Unite des Communes vald 'otainesMont-Emilius'. The research at the OAVdA was partially funded by several `Research and Education' annual grants from Fondazione CRT. This article is partly based on observations made with the IAC80 and TCS telescopes operated by the Instituto de Astrofisica de Canarias in the Spanish Observatorio del Teide on the island of Tenerife. A part of the observations were carried out using theRATAN-600 scientific equipment (SAO of the Russian Academy of Sciences)