Dark Matter Signals from Cascade Annihilations

A leading interpretation of the electron/positron excesses seen by PAMELA and ATIC is dark matter annihilation in the galactic halo. Depending on the annihilation channel, the electron/positron signal could be accompanied by a galactic gamma ray or neutrino flux, and the non-detection of such fluxes constrains the couplings and halo properties of dark matter. In this paper, we study the interplay of electron data with gamma ray and neutrino constraints in the context of cascade annihilation models, where dark matter annihilates into light degrees of freedom which in turn decay into leptons in one or more steps. Electron and muon cascades give a reasonable fit to the PAMELA and ATIC data. Compared to direct annihilation, cascade annihilations can soften gamma ray constraints from final state radiation by an order of magnitude. However, if dark matter annihilates primarily into muons, the neutrino constraints are robust regardless of the number of cascade decay steps. We also examine the electron data and gamma ray/neutrino constraints on the recently proposed "axion portal" scenario.Comment: 36 pages, 11 figures, 7 tables; references adde

Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array (AERA) addresses both technological and scientific aspects of the radio technique. A first phase of AERA has been operating since September 2010 with detector stations observing radio signals at frequencies between 30 and 80 MHz. In this paper we present comparative studies to identify and optimize the antenna design for the final configuration of AERA consisting of 160 individual radio detector stations. The transient nature of the air shower signal requires a detailed description of the antenna sensor. As the ultra-wideband reception of pulses is not widely discussed in antenna literature, we review the relevant antenna characteristics and enhance theoretical considerations towards the impulse response of antennas including polarization effects and multiple signal reflections. On the basis of the vector effective length we study the transient response characteristics of three candidate antennas in the time domain. Observing the variation of the continuous galactic background intensity we rank the antennas with respect to the noise level added to the galactic signal

Fenologia reprodutiva, sazonalidade e germinação de Kielmeyera regalis Saddi (Clusiaceae), espécie endêmica dos campos rupestres da Cadeia do Espinhaço, Brasil Reproductive phenology, seasonality and germination of Kielmeyera regalis Saddi (Clusiaceae), a species endemic to rock outcrops in the Espinhaço Range, Brazil

A fenologia reprodutiva e a germinação de sementes foram estudadas em uma população de Kielmeyera regalis da Serra do Cipó, MG. Foram calculados os índices de atividade e intensidade de produção de botões, flores, frutos imaturos e frutos maduros ao longo de 2001. A influência do clima sobre a fenologia foi avaliada por Análise de Correspondência Canônica (CCA). A germinação foi avaliada a temperaturas constantes de 15-35 ºC (com intervalos de 5 ºC) em câmaras de germinação com fotoperíodo de 12 h. A variância dos dados explicada pela CCA foi de 72,8%. A temperatura média do ar, evaporação e radiação solar global apresentaram altos coeficientes de correlação com a fenologia. O florescimento ocorreu nos meses quentes e úmidos, a maturação de frutos se estendeu na estação seca e fria, e a dispersão das sementes, logo antes da estação chuvosa. A germinabilidade foi superior a 80% nas temperaturas de 20-30 ºC, faixa ocorrente no período chuvoso logo após a dispersão das sementes. Comparações com outros estudos indicam que a dispersão e rápida germinação nesses períodos são fortes fatores adaptativos dentro do gênero. Os resultados são importantes para a compreensão dos fatores que afetam o sucesso reprodutivo e expansão populacional, e devem ser considerados para ações de manejo desta espécie rupestre endêmica.<br>The reproductive phenology and seed germination of a Kielmeyera regalis population, from Serra do Cipó (MG), Brazil, were studied. During 2001, the intensity and activity indices were calculated to estimate production of flower buds, flowers, and immature and mature fruits. Influence of the climate on phenology was determined by a Canonical Correspondence Analysis (CCA). Germination was studied under a 12 h photoperiod at seven fixed temperatures (15-35ºC at 5ºC intervals). The CCA explained 72.8% of the phenological data variation. The highest correlation coefficients with phenology were observed for mean air temperature, evaporation and solar global radiation. Flowering occurred during the hot and wet season, fruit maturation extended during the entire cold and dry season, and seed dispersal peaked before the onset of the rainy season. Germinability reached values above 80% under temperatures of 20-30ºC, which occurred during the rainy period, just after seed dispersal. The results of this and other studies indicate that seed dispersal just before the rainy season, and fast germination at the beginning of the rainy season, are highly adaptive traits within the genus. In addition, the results provide important information for understanding basic factors that affect reproductive success and population growth, and should be considered when managing this endemic species from rock outcrop

Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory

Extent: 50p.The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array (AERA) addresses both technological and scientific aspects of the radio technique. A first phase of AERA has been operating since September 2010 with detector stations observing radio signals at frequencies between 30 and 80 MHz. In this paper we present comparative studies to identify and optimize the antenna design for the final configuration of AERA consisting of 160 individual radio detector stations. The transient nature of the air shower signal requires a detailed description of the antenna sensor. As the ultra-wideband reception of pulses is not widely discussed in antenna literature, we review the relevant antenna characteristics and enhance theoretical considerations towards the impulse response of antennas including polarization effects and multiple signal reflections. On the basis of the vector effective length we study the transient response characteristics of three candidate antennas in the time domain. Observing the variation of the continuous galactic background intensity we rank the antennas with respect to the noise level added to the galactic signal.The Pierre Auger Collaboration, P. Abreu... K. B. Barber... J. A. Bellido... R. W. Clay... M. J. Cooper... B. R. Dawson... T. A. Harrison... A. E. Herve... V. C. Holmes... J. Sorokin... P. S. Wahrlich.. B. J. Whelan... et al

Limits on point-like sources of ultra-high-energy neutrinos with the Pierre Auger Observatory

International audienceWith the Surface Detector array (SD) of the Pierre Auger Observatory we can detect neutrinos with energy between 1017 eV and 1020 eV from point-like sources across the sky, from close to the Southern Celestial Pole up to 60ˆ in declination, with peak sensitivities at declinations around ∼ −53ˆ and ∼+55ˆ, and an unmatched sensitivity for arrival directions in the Northern hemisphere. A search has been performed for highly-inclined air showers induced by neutrinos of all flavours with no candidate events found in data taken between 1 Jan 2004 and 31 Aug 2018. Upper limits on the neutrino flux from point-like steady sources have been derived as a function of source declination. An unrivaled sensitivity is achieved in searches for transient sources with emission lasting over an hour or less, if they occur within the field of view corresponding to the zenith angle range between 60ˆ and  95ˆ where the SD of the Pierre Auger Observatory is most sensitive to neutrinos