Waste management in the stingless bee Melipona beecheii Bennett (Hymenoptera: Apidae)

Waste management is important in insect societies because waste can be hazardous to adults, brood and food stores. The general organization of waste management and the influence of task partitioning, division of labor and age polyethism on waste processing were studied in three colonies of the tropical American stingless bee Melipona beecheii Bennett in Yucatán, Mexico. Waste generated in the colony (feces, old brood cells, cocoons, dead adults and brood) was collected by workers throughout the nest and taken to specific waste dumps within the nest. During the day, workers based at the waste dumps formed waste pellets, which they directly transferred in 93% of cases, to other workers who subsequently removed them from the nest. This is an example of task partitioning and is hypothesized to improve nest hygiene as has been found in leafcutting ants, Atta. To investigate division of labor and age polyethism we marked a cohort of 144 emerging workers. Workers forming waste pellets were on average 31.2±6.5 days old (±SD, N= 40, range of 18-45 days). The life span of M. beecheii workers was 49.0±14.0 days (N= 144). There was no difference in the life span of workers who formed (52.2±11.6 days, N= 40) or did not form (49.9±11.5 days, N= 97) waste pellets, suggesting that waste work did not increase mortality. Although waste was probably not hazardous to adults and brood, because the dumps are located outside the brood chamber, its presence inside the nests can attract phorid flies and predators, which can harm the colony

On the possibility of neutrino flavor identification at the highest energies

High energy astrophysical neutrinos carry relevant information about the origin and propagation of cosmic rays. They can be created as a by-product of the interactions of cosmic rays in the sources and during propagation of these high energy particles through the intergalactic medium. The determination of flavor composition in this high energy flux is important because it presents a unique chance to probe our understanding of neutrino flavor oscillations at gamma factors >10^21. In this work we develop a new statistical technique to study the flavor composition of the incident neutrino flux, which is based on the multipeak structure of the longitudinal profiles of very deep electron and tau neutrino horizontal air showers. Although these longitudinal profiles can be observed by means of fluorescence telescopes placed over the Earth's surface, orbital detectors are more suitable for neutrino observations owing to their much larger aperture. Therefore, we focus on the high energy region of the neutrino spectrum relevant for observations with orbital detectors like the planned JEM-EUSO telescope.Comment: Accepted for publication in Physical Review

PENGARUH BUDAYA ORGANISASI TERHADAP KEBERHASILAN PENGEMBANGAN E-GOVERNMENT

Sejak diterbitkannya Instruksi Presiden No. 3/2003 dan UU No 14/2008, lembaga-lembaga pemerintah mulai dari pusat sampai dengan tingkat kabupaten/kota berlomba-lomba menjadi yang terdepan dalam implementasi e-government dan memenuhi keterbukaan informasi kepada public. Pada saat ini pada Kementerian Agama penerapkan e-Governement masih belum terlihat dalam menunjang pekerjaan mereka yang dapat dilihat dari masih kurang dimanfaatkannya sarana e-mail sebagai sarana komunikasi dan website sebagai alat untuk memberikan informasi baik kepada public maupun kepada kalangan internal organisasi. Tampaknya hal ini dikarenakan masih kurangnya budaya organisasi di kementerian. Penelitian ini ingin melihat seberapa besar budaya organisasi mempengaruhi keberhasilan pengembangan e-government dengan metode pengukuran budaya organisasi Luthans (1998), di mana budaya organisasi merupakan norma-norma dan nilainilai yang mengarahkan perilaku anggota organisasi, sehingga budaya organisasi diukur melalui perilaku organisasi melalui dimensi orang, struktur, teknologi, dan lingkungan tempat organisasi beroperasi. Sedangkan e-Government diukur sesuai dengan menurut manfaatnya. Dengan menggunakan model Structural Equation Model (SEM) didapatkan bahwa Budaya Organisasi berpengaruh signifikan terhadap keberhasilan pengembangan e-Government dimana yang paling signifikant mempengaruhi adalah dimensi orang dan lingkungan luar

Linear recurrences and asymptotic behavior of exponential sums of symmetric boolean functions

In this paper we give an improvement of the degree of the homogeneous linear recurrence with integer coefficients that exponential sums of symmetric Boolean functions satisfy. This improvement is tight. We also compute the asymptotic behavior of symmetric Boolean functions and provide a formula that allows us to determine if a symmetric boolean function is asymptotically not balanced. In particular, when the degree of the symmetric function is a power of two, then the exponential sum is much smaller than $2^n$.Comment: 18 pages, 3 figure

Ensemble fluctuations of the cosmic ray energy spectrum and the intergalactic magnetic field

The origin of the most energetic cosmic ray particles is one of the most important open problems in astrophysics. Despite a big experimental effort done in the past years, the sources of these very energetic particles remain unidentified. Therefore, their distribution on the Universe and even their space density are still unknown. It has been shown that different spatial configurations of the sources lead to different energy spectra and composition profiles (in the case of sources injecting heavy nuclei) at Earth. These ensemble fluctuations are more important at the highest energies because only nearby sources, which are necessarily few, can contribute to the flux observed at Earth. This is due to the interaction of the cosmic rays with the low energy photons of the radiation field, present in the intergalactic medium, during propagation. It is believed that the intergalactic medium is permeated by a turbulent magnetic field. Although at present it is still unknown, there are several constraints for its intensity and coherence length obtained from different observational techniques. Charged cosmic rays are affected by the intergalactic magnetic field because of the bending of their trajectories during propagation through the intergalactic medium. In this work, the influence of the intergalactic magnetic field on the ensemble fluctuations is studied. Sources injecting only protons and only iron nuclei are considered. The ensemble fluctuations are studied for different values of the density of sources compatible with the constraints recently obtained from cosmic ray data. Also, the possible detection of the ensemble fluctuations in the context of the future JEM-EUSO mission is discussed.Comment: Accepted for publication in Physical Review