1,086 research outputs found

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    Extended GeV-TeV Emission around Gamma-Ray Burst Remnants, and the Case of W49B

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    We investigate the high-energy photon emission around Gamma-Ray Burst (GRB) remnants caused by ultrahigh-energy cosmic rays (UHECRs) from the GRBs. We apply the results to the recent report that the supernova remnant W49B is a GRB remnant in our Galaxy. If this is correct, and if GRBs are sources of UHECRs, a natural consequence of this identification would be a detectable TeV photon emission around the GRB remnant. The imaging of the surrounding emission could provide new constraints on the jet structure of the GRB.Comment: 12 pages, 2 figures, accepted for publication in ApJ

    A Crazy Question: Can Apparently Brighter Gamma-ray Bursts Be Farther Away?

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    The cosmological relationships between observed and emitted quantities are determined for gamma-ray bursts (GRBs). The relationship shows that apparently fainter bursts need not, in general, lie at larger redshifts.This is possible when the luminosities (or emitted energies) in a sample of bursts increase faster than the dimming of the observed values with redshift. Four different samples of long bursts suggest that this is what really happens

    Gamma-ray bursts: optical afterglows in the deep Newtonian phase

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    Gamma-ray burst remnants become trans-relativistic typically in days to tens of days, and they enter the deep Newtonian phase in tens of days to months, during which the majority of shock-accelerated electrons will no longer be highly relativistic. However, a small portion of electrons are still accelerated to ultra-relativistic speeds and capable of emitting synchrotron radiation. The distribution function for electrons is re-derived here so that synchrotron emission from these relativistic electrons can be calculated. Based on the revised model, optical afterglows from both isotropic fireballs and highly collimated jets are studied numerically, and compared to analytical results. In the beamed cases, it is found that, in addition to the steepening due to the edge effect and the lateral expansion effect, the light curves are universally characterized by a flattening during the deep Newtonian phase.Comment: MNRAS in press (originally submitted in October 2002), 8 pages with 8 eps figures embedded, references update

    Large scale magnetic fields and their dissipation in GRB fireballs

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    We consider possible geometries of magnetic fields in GRB outflows, and their evolution with distance from the source. For magnetically driven outflows, with an assumed ratio of magnetic to kinetic energy density of order unity, the field strengths are sufficient for efficient production of gamma-rays by synchrotron emission in the standard internal shock scenario, without the need for local generation of small scale fields. In these conditions, the MHD approximation is valid to large distances (>10^19cm). In outflows driven by nonaxisymmetric magnetic fields, changes of direction of the field cause dissipation of magnetic energy by reconnection. This dissipation takes place outside the photosphere of the outflow, and can convert a significant fraction of the magnetic energy flux into radiation.Comment: 12 pages including 3 figures, submitted to A&

    Fungal diversity in floral and honeydew honeys

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    Studying fungal diversity in various environmental samples provides us with valuable knowledge about the occurrence of fungi of medical and ecological importance. Moreover, fungal composition may also characterise well the botanical and geographical source of food products, such as the origin of the spore enriched honeydew honeys. Thereby, we identified a wide spectrum of fungi found in 100 of honey samples from various geographical sources – most of them were from Italy, Greece and Hungary. Our honeydew honeys had a higher mean of the number of spore types found in them than floral honeys had. Statistically significant differences in diversity were found regarding the botanical source (p = 1.29 × 10–9) and the climatic classification (p = 2.28 × 10–2) according to Kruskal– Wallis rank sum tests. Most frequently encountered genera included ubiquitous saprotrophic species (Alternaria, Cladosporium, Epicoccum nigrum, Stemphylium), both in floral and honeydew honeys. On the other hand, certain sooty moulds like Aureobasidium pullulans, Tripospermum and Capnobotrys were rather present in different types of honeydew honeys. Metschnikowia reukaufii, the nectar inhabiting yeast reached considerably high quantities in floral honey samples. Present findings encourage further studies on quantifying the occurrence and the indicator value of specific fungal elements in honey, concerning its origin

    On the detectability of gravitational waves background produced by gamma ray bursts

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    In this paper we discuss a new strategy for the detection of gravitational radiation likely emitted by cosmological gamma ray burst. Robust and conservative estimates lead to the conclusion that the uncorrelated superimposition of bursts of gravitational waves can be detected by interferometric detectors like VIRGO or LIGO. The expected signal is predicted to carry two very distinctive signatures: the cosmological dipole anisotropy and a characteristic time scale in the auto correlation spectrum, which might be exploited, perhaps with ad hoc modifications and/or upgrading of the planned experiments, to confirm the non-instrumental origin of the signal.Comment: 9 pages, 2 figures, LATEX2e, Accepted for pubblications as a Letter to the Editor in Journal of Physics G: Nuclear and Particle Physic

    A hagyomĂĄnyos kĂ­nai orvoslĂĄs magyarorszĂĄgi szabalyozĂĄsĂĄnak egyes problĂ©mĂĄi Ă©s lehetsĂ©ges megoldĂĄsai az EgyesĂŒlt KirĂĄlysĂĄg pĂ©ldĂĄjĂĄn keresztĂŒl

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    This paper aims to present factual information and to suggest possible solutions regarding some of the recent questions which have arisen regarding the regulation of traditional Chinese medicine in Hungary. According to current legislation "traditional Chinese doctors", who are the most highly trained professionals in this field, are not allowed to practice Chinese medicine and acupuncture in Hungary. This situation cannot be explained by their educational background, as they receive thorough training in both Chinese medicine and modern medical sciences. Furthermore, this legislation is not supported by any EU standard: Traditional Chinese medicine professionals can practice Chinese medicine and acupuncture in a number of European countries within a legal and regulated framework. Different kinds of healthcare professionals may practice Chinese medicine and acupuncture in the UK - this could be a good example for Hungarian regulation. The five-year bachelor level traditional Chinese medicine training at the Faculty of Health Sciences, Semmelweis University and the increasing number of locally trained traditional Chinese medicine professionals could be a good basis for laying the groundwork of the new system. Orv., Hetil., 2014, 155(15), 575-581

    TeV Neutrinos from Successful and Choked Gamma-Ray Bursts

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    Core collapse of massive stars resulting in a relativistic fireball jet which breaks through the stellar envelope is a widely discussed scenario for gamma-ray burst production. For very extended or slow rotating stars, the fireball may be unable to break through the envelope. Both penetrating and choked jets will produce, by photo-meson interactions of accelerated protons, a burst of neutrinos with energies in excess of 5 TeV while propagating in the envelope. The predicted flux, from both penetrating and chocked fireballs, should be easily detectable by planned cubic kilometer neutrino telescopes.Comment: Phys.Rev.Letters, in press, final version accepted 8/31/01 (orig. 3/17/01
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