Search for Hidden photons with Sumico

We searched for solar hidden photons in the visible photon energy range using a hidden photon detector add-on attached to Sumico. It consists of a parabolic mirror of dia. 0.5m and f=1m installed in a vacuum chamber, and a low noise photomultiplier tube at the focal point. No evidence for the existence of hidden photons was found in the latest measurement giving a new limit on the photon-hidden photon mixing parameter in the hidden photon mass range 0.001-1eV.Comment: 6 pages. Contributed to the 9th Patras Workshop on Axions, WIMPs and WISPs, Mainz, June 24-28, 201

Limits on deeply penetrating particles in the 10(17) eV cosmic ray flux

Deeply penetrating particles in the 10 to the 17th power eV cosmic ray flux were investigated. No such events were found in 8.2 x 10 to the 6th power sec of running time. Limits were set on the following: quark-matter in the primary cosmic ray flux; long-lived, weakly interacting particles produced in p-air collisions; the astrophysical neutrino flux. In particular, the neutrino flux limit at 10 to the 17th power eV implies that z, the red shift of maximum activity is 10 in the model of Hill and Schramm

The structure of EAS at E 0.1 EeV

The ratio of extensive air showers (EAS) total shower energy in the electromagnetic channel (E em) to the size of the shower at maximum development (N max) from a direct measurement of shower longitudinal development using the air fluorescence technique was calculated. The values are not inconsistent with values based upon track length integrals of the Gaisser-Hillas formula for shower development or the known relation between shower energy and size at maximum for pure electromagnetic cascades. Using Linsley's estimates for undetected shower energy based on an analysis of a wide variety of cosmic ray data, the following relation for total shower energy E vs N max is obtained. The Gaisser Hillas implied undetected shower energy fractions

Hallucinogen Rating Scale (HRS) - A Brazilian version: translation and cross-cultural adaptation

BACKGROUND: There is a growing scientific interest in the effects of hallucinogens in general and the religious use of psychoactive brew ayahuasca in Brazil in particular. However, there is not yet a standard instrument used in Brazil to evaluate the effects of hallucinogens. The Hallucinogen Rating Scale (HRS) is a questionnaire widely used in the U.S. and Europe to evaluate the effects of several psychoactive substances, including hallucinogens. OBJECTIVE: To translate and adapt the HRS to Brazilian Portuguese. METHOD: We followed three steps: 1) the authors of the article translated the HRS into Portuguese, in order to establish an initial version; 2) two independent translators back-translated this version into English; 3) a revision committee produced a final version of the Brazilian Portuguese version. This final version was developed comparing the initial translations and back-translations, through a dialogic process with the author of the instrument. RESULTS: A final Portuguese version of the HRS, following the guidelines for semantic and conceptual equivalence between English and Portuguese to describe hallucinogen-induced subjective states. DISCUSSION: A Brazilian version of the HRS - an instrument widely used throughout the world to quantify effects of psychoactive drugs - provides a sensitive instrument for evaluation of the effects of hallucinogenic substances in Brazil.CONTEXTO: Existe um crescente interesse científico pelos efeitos de alucinógenos em geral e, particularmente, pelo uso religioso da bebida psicoativa ayahuasca no Brasil. Todavia, não há no Brasil um instrumento padronizado para avaliar os efeitos de alucinógenos. A Hallucinogen Rating Scale (HRS) é um questionário amplamente usado nos Estados Unidos e na Europa para avaliar os efeitos de diversas substâncias psicoativas, incluindo as alucinógenas. OBJETIVO: Traduzir e adaptar a HRS para o português brasileiro. MÉTODO: A adaptação foi realizada em três etapas: 1) os autores do artigo traduziram a HRS para o português, visando à elaboração de uma versão-síntese inicial; 2) foi feita retrotradução dessa versão para o inglês por dois tradutores independentes; 3) foi elaborada uma versão final em português brasileiro por um comitê de revisão. Esta versão final foi desenvolvida pela comparação entre as traduções iniciais e as retrotraduções, por um processo dialógico com o autor do instrumento. RESULTADOS: Produção da versão final da HRS em português. Observaram-se as diretrizes para equivalência semântica e conceitual entre o português e inglês na descrição de estados subjetivos induzidos por alucinógenos. CONCLUSÃO: Uma versão brasileira da HRS - instrumento largamente empregado em todo o mundo para quantificar os efeitos de psicoativos - fornece um instrumento sensível para a avaliação de efeitos de substâncias alucinógenas no Brasil.Universidade Federal de São Paulo (UNIFESP) Departamento de PsiquiatriaUniversidade Estadual de Santa Cruz Departamento de Filosofia e Ciências Humanasda Universidade do Novo México Escola de MedicinaUNIFESP, Depto. de PsiquiatriaSciEL

500 TeV gamma rays from Hercules X-1

A signal (chance probability = .0002) with the 1.24 s period of Hercules X-1 has been observed using the Utah Fly's Eye. The signal's relatively long period and high shower energy conflict with some popular models of particle acceleration by pulsars. Optical and X-ray data suggest a picture in which energetic particles produce multi-TeV gamma rays by collisions with Hercules X-1's accretion disk

All sky Northern Hemisphere 10(15) EV gamma-ray survey

Flux limits in the range 10 to the minus 13th power-10 to the minus 12 power/sq cm/s have been obtained by observing Cerenkov flashes from small air showers. During 1983, a 3.5 sigma excess of showers was observed during the phase interval 0.2 to 0.3 of the 4.8h period of Cygnus X-3, but no excess was found in 1984 observations

Proton-air inelastic cross section at S(1/2) = 30 TeV

The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosphere was measured as a function of atmospheric depth. From the exponential tail of this distribution, it was determined that the proton-air inelastic cross section at 30 TeV center-of-mass energy to be 540 + or - 40mb

Arrival directions of cosmic rays of E .4 EeV

The anisotropy of cosmic rays observed by the Utah Fly's Eye detector has been studied. Emphasis has been placed on examining distributions of events in galactic coordinates. No statistically significant departure from isotropy has been observed for energies greater than 0.4 EeV (1 EeV = 10 to the 18th power eV). Results of the standard harmonic analysis in right ascension are also presented