BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:CR Erzions Search Results\, Received on the Modernizated Telescop e "Doch-4AM" with New Analog Digital Converter DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-798@cern.ch DESCRIPTION:Speakers: Yury Bazhutov (Scientific Research Center of Enginee ring Physical Problems (SRCEPhP) “ERZION”)\nTo search cosmic ray Erzio ns the telescope "Doch-4AM" was used. For the digitization and transmissio n to the personal computer of scintillation detectors amplitudes the new L A-n10-12 two-channel ADC circuit became used. The thick amount (ρh$\\sim$ 60g/cm2) of arid soda (Na2CO3)\, surrounded by the thick amount ($\\rho$h$ \\sim$120g/cm2) of graphite been chosen for the optimum converter-material placed on the Al ($\\rho$h$\\sim$ 15.5g/cm2) plate above the telescope t o convert neutral primary cosmic ray Erzions to negative one for their reg istration. There are presented and analyzed received results.\n\nhttps://i ndico.particle.mephi.ru/event/4/contributions/798/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/798/ END:VEVENT BEGIN:VEVENT SUMMARY:Erzion Model at its Supplement to Cosmic Rays\, Astrophysics\, Geo physics\, Cold Nuclear Transmutation and Other Nature Phenomena DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-793@cern.ch DESCRIPTION:Speakers: Yury Bazhutov (Scientific Research Center of Enginee ring Physical Problems (SRCEPhP) “ERZION”)\nAlthough Cold Nuclear Tran smutation (CNT) is rather reliable phenomenon\, but there are few theoreti c models for its explanation. Erzion model of the catalytic nuclear transm utation (EM) was one of the first such models which could in detail interp ret this phenomenon. So in the report it is described the shot history of Erzion (new massive stable hadron) hypothesis appearance in Cosmic Rays in 1982 and Erzion Model development to explain the main features of Cold Nu clear Transmutation Experiments. Erzion Model can give principle explanati on for many problems in Cosmic Ray\, Astrophysics and Geophysics. In frame work of EM Erzion is object of Dark Matter. Moreover\, some applied proble ms can be decided in framework of Erzion Model\, such as: 1) to create the new energy-capacious\, ecology-pure with rather simple technology nuclear energetics\; 2) principle and radical utilization of radioactive wastes\; 3) cheap production of some chemical elements and isotopes (gold for exam ple). Erzion Model can explain many experiments in Cold Fusion and can pre dict many new experiments for its testing.\n\nhttps://indico.particle.meph i.ru/event/4/contributions/793/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/793/ END:VEVENT BEGIN:VEVENT SUMMARY:DISCOVERY OF NEW COSMIC RAYS EFFECT: THE PLANETS MODULATION DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-766@cern.ch DESCRIPTION:Speakers: Alexey Retejum (MSU)\nThe author has performed an an alysis of long-term variations of cosmic rays variation in connection with the planets motion\, All neutron monitors selected for the study (Moscow\ , Apatyti\, Irkutsk\, Novosibirsk\, Oulu\, Jungfraujoch\, Lomnicky Stit\, Sanae\, Calgary\, McMurdo\, Thule).show the same picture: the cosmic rays intensity changes depending on the planets position on their orbits. At t he same time the obtained results reveal clearly that the process of modul ation is controlled differently by planets with direct and retrograde rota tion. At the moment when the planet with direct rotation passes its apheli on the intensity of cosmic rays as a rule is below normal and the occurre nce of Forbush decrease events is increasing. At their perihelion the cold celestial bodies of this type produce an opposite effect. \n\nVenus and e specially Uranus unlike the planets with direct rotation\, are increasing the the intensity of cosmic rays at their aphelion points. \n\nA sharp c ontrast between action of the planets with direct and retrograde rotation action simulates the situation of the thought critical experiment in which we are able to find the only explanation of the observed effect\, namely slowing down and speeding up of the Sun as consequences derived from the c ontact of its invisible envelop with similar envelops belonging to the pla nets. These outer parts of the celestial bodies consist of superlight gas newtonium – – transhydrogen chemical element predicted by D.I.Mendele ev along with other six elements which were discovered earlier.\n \nDescr ibed findings create a base for prediction of cosmic rays anomalies both i n the near and distant future.\n\nhttps://indico.particle.mephi.ru/event/4 /contributions/766/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/766/ END:VEVENT BEGIN:VEVENT SUMMARY:CP-sensitive observables of a hypothetical heavy spin-0 particle w ith the dominant $\\gamma\\gamma$ and $Z\\gamma$-interaction. DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-694@cern.ch DESCRIPTION:Speakers: Nikita Belyaev (NRNU MEPhI)\nWe study observables se nsitive to tensor structure of interactions of a hypothetical heavy spin-0 boson. It is assumed that interactions of this particle are dominated by interactions with photons. The interactions with other vector bosons and q uarks are supposed to be suppressed. The above assumptions favor the produ ction of this hypothetical particle through the vector boson fusion mechan ism structurally dominated by the photon and Z-interactions. This particle will be produced in association with two light quarks. It is shown that t he azimuthal angle difference between the tagging jets provides an observa ble to probe the tensor structure of the interaction vertices of such hypo thetical particle.\n\nhttps://indico.particle.mephi.ru/event/4/contributio ns/694/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/694/ END:VEVENT BEGIN:VEVENT SUMMARY:Thermodynamic and relativistic uncertainty relations DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-662@cern.ch DESCRIPTION:Speakers: Anton Artamonov (University of Oulu)\nThermodynamic uncertainty relation (UR) was verified experimentally. The experiments ha ve shown the validity of the quantum analogue of the zeroth law of stochas tic thermodynamics in the form of the saturated Schrödinger UR. \nWe have also proposed a new type of UR for the relativistic mechanics.\n\nThese r elations allow us to consider macroscopic phenomena in the within the limi ts of the ratio of the uncertainty relations for different physical quanti ties\n\nhttps://indico.particle.mephi.ru/event/4/contributions/662/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/662/ END:VEVENT BEGIN:VEVENT SUMMARY:Study of LHC experiments sensitivity to anomalous quartic gauge couplings in $Z\\gamma\\gamma$ production during Run2 DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-658@cern.ch DESCRIPTION:Speakers: Anastasia Kurova (NRNU MEPhI)\nRun2 sensitivity to q uartic anomalous gauge couplings was estimated for ATLAS experiment at LHC with increased energy of proton-proton collisions $\\sqrt{s} = 13$ TeV an d expected 40 fb$^{-1}$ (2016) and 100 fb$^{-1}$ (2016-2017) of integral l uminosity. Simulation of $Z\\gamma\\gamma$ process with anomalous $ZZ\\gam ma\\gamma$ and $Z\\gamma\\gamma\\gamma$ couplings was performed using VBFN LO MC generator. Differential distributions on four body invariant mass of final state particles was used for extraction of expected limits on Effec tive Field Theory parameters $f_{T0}/\\Lambda^{4}\, f_{T5}/\\Lambda^{4}\,  f_{T9}/\\Lambda^{4}\, f_{M2}/\\Lambda^{4}\, f_{M3}/\\Lambda^{4}$. Comb ined limits are obtained from two charged leptonic decay channels of Z bos on ($Z\\gamma\\gamma\\rightarrow l^{+}l^{−}\\gamma\\gamma$\, where $l = e$ or $\\mu$). Unitarity of expected limits was studied using dipole form factor.\n\nhttps://indico.particle.mephi.ru/event/4/contributions/658/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/658/ END:VEVENT BEGIN:VEVENT SUMMARY:The abnormal daily distributions of events received on the Doch-4 A telescope by search of Erzion in Cosmic Ray DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-650@cern.ch DESCRIPTION:Speakers: Albina Gerasimova (Scientific Research Center of Eng ineering Physical Problems (SRCEPhP) “ERZION”)\nFor search in space be ams of Erzion the Doch-4A telescope within 150 days of its operation was u sed (15.07.14 - 05.03.15). As optimum substance - the converter of neutral Erzion (E0) of primary space radiation into charged (E0 → E-) for the p urpose of their registration the dehydrated calcinated soda was chosen (Na 2CO3\, ρh~50 g/cm2). In the report new results are presented and discusse d: correlation dependence of scintillation detectors amplitudes\, abnormal daily distributions of the events which are selected with the 10th multip ly increased specific ionization (10m) and their daily intensity. The best data on daily distribution of events for the thick homogeneous converter from the dried-up Na2CO3 soda at its 30-day summer exposition are obtained new and even more. They testify about considerable (~ 50%\, 4\,8σ) a sha re of events with the Erzion nature (in morning period from E0 and in even ing period from E-) for high ionization (10m) components of cosmic ray. It occurs only for the summer period of a solstice when the high-standing Su n on the heavenly sphere gets to a telescope aperture for registration neu tral Erzion (E0). Charged Erzion (E-) from the Sun under the influence of a deviation with a magnetic field of Earth can come in the evening to Eart h surface in near vertical direction during any season of year with differ ent efficiency.\n\nhttps://indico.particle.mephi.ru/event/4/contributions/ 650/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/650/ END:VEVENT BEGIN:VEVENT SUMMARY:Midday the CR component in abnormal daily distributions on the Doc h-4A telescope DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-592@cern.ch DESCRIPTION:Speakers: Albina Gerasimova (Scientific Research Center of Eng ineering Physical Problems (SRCEPhP) “ERZION”)\nFor search in space be ams of Erzion the Doch-4A telescope was used. Are presented in the report and new results are discussed: correlation dependence of amplitudes of sci ntillation detectors for the midday events which are selected with the 10t h multiply increased specific ionization and their daily intensity in comp arison with daily intensity of a stream of solar protons in solar flashes for the same period (11.09-26.11).14. The carried-out analysis gave their good coincidence and\, thereby\, indicated on solar origin of registed Erz ions.\n\nhttps://indico.particle.mephi.ru/event/4/contributions/592/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/592/ END:VEVENT BEGIN:VEVENT SUMMARY:The COHERENT Experiment: CENNS-10 Detector DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-525@cern.ch DESCRIPTION:Speakers: Alexander Kumpan (National Research Nuclear Universi ty MEPhI)\nThe COHERENT experiment goal are to detect and to study neutrin o coherent scattering of elastic neutrino-nucleus scattering (CE$\\nu$NS). This process is predicted by Standard Model but it has never been observe d experimentally because of very low energy of recoil nucleus. COHERENT is using different detector technologies: germanium detectors\, CsI[Na] and NaI scintillators and single-phase liquid Ar calorimeter. A description of liquid Ar detector\, named CENNS-10\, its current status and future plans will be presented.\n\nhttps://indico.particle.mephi.ru/event/4/contributi ons/525/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/525/ END:VEVENT BEGIN:VEVENT SUMMARY:Apparatus complex based on liquid xenon detector for gamma spectro metry in the intervals between pulses of intense radiation DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-522@cern.ch DESCRIPTION:Speakers: Mikhail Kirsanov (MEPhI)\nTo investigate the effects of intense radiation on the operation of the liquid xenon spectrometer wa s created apparatus complex based on liquid xenon detector. The experiment al setup consists of a multifunctional chamber\, gas system\, cooling syst em\, temperature control system\, a special preamp\, passive protection\, scintillation monitor the accelerator beam\, thermoluminescent dosimeters. Multifunctional chamber includes a detecting unit (flat or cylindrical io nization chamber)\, the cleaning unit of the xenon\, control unit of the p urity of liquid xenon. The liquid xenon detector was irradiated by bremsst rahlung pulses of the microtron. The frequency of irradiation pulses was 4 00 Hz. The absorbed dose was varied from 10-7 to 0.1 Gy per pulse. The ele ctronic and ionic processes in liquid xenon at different radiation doses w ere investigated. Stable operation of the liquid xenon spectrometer in the intervals between the pulses of the accelerator shown for a long time.\n\ nhttps://indico.particle.mephi.ru/event/4/contributions/522/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/522/ END:VEVENT BEGIN:VEVENT SUMMARY:Search for a high-mass Higgs boson decaying to a pair of W bosons in pp collisions at 13 TeV with the ATLAS detector DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-489@cern.ch DESCRIPTION:Speakers: Aleksandr Gavriliuk (Institute for Theoretical and E xperimental Physics (RU))\nIn this poster a search for a high-mass Higgs b oson in the\nH-->WW-->lvlv decay channel is presented. The search is using pp\ncollision data corresponding to an integrated luminosity of 13.2 fb-1 \ncollected at a centre-of-mass energy of 13 TeV by the ATLAS detector\nat the Large Hadron Collider.\nNo evidence of a high-mass Higgs boson is fou nd. Upper limits on\nHxBR(H-->WW) as a function of the Higgs boson mass a nd width are\nobtained in the mass range between\n300 GeV and 3 TeV.\n\nht tps://indico.particle.mephi.ru/event/4/contributions/489/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/489/ END:VEVENT BEGIN:VEVENT SUMMARY:The use of liquid xenon detectors in the conditions of intensive i rradiation DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-484@cern.ch DESCRIPTION:Speakers: Mikhail Kirsanov (MEPhI)\nThe detectors based on liq uid xenon have high radiation resistance. They are promising detectors for operation in the conditions of intense radiation. The recovery time of th e spectrometric mode of the liquid xenon detector after intensive irradiat ion was investigated. We presented the results of the calculation of xenon activation by thermal neutrons and gamma rays. The operation of the liqui d xenon spectrometer in the intervals between pulses of the radiation was studied. The possibility of using the liquid xenon spectrometer for activa tion analysis for the short-lived nuclides was shown.\n\nhttps://indico.pa rticle.mephi.ru/event/4/contributions/484/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/484/ END:VEVENT BEGIN:VEVENT SUMMARY:Measurement of CP-violation parameters in decays of B0s->JpsiPhi w ith the ATLAS detector DTSTART;VALUE=DATE-TIME:20161010T121500Z DTEND;VALUE=DATE-TIME:20161010T124500Z DTSTAMP;VALUE=DATE-TIME:20260814T152256Z UID:indico-contribution-95-482@cern.ch DESCRIPTION:Speakers: Artem Maevskiy (Skobeltsyn Institute of Nuclear Phys ics (SINP MSU))\nA measurement of the CP-violating weak phase phi_s and th e B0s meson decay width difference with Bs->JpsiPhi decays in the ATLAS ex periment is presented. It is based on integrated luminosity of 14.3 fb-1 c ollected by the ATLAS detector from 8 TeV pp collisions at the LHC. The me asured values are statistically combined with those from 4.9 fb-1 of 7 TeV collisions data\, yielding an overall Run-1 ATLAS result.\n\nhttps://indi co.particle.mephi.ru/event/4/contributions/482/ LOCATION:Milan Hotel Hall of the 2nd floor URL:https://indico.particle.mephi.ru/event/4/contributions/482/ END:VEVENT END:VCALENDAR