Energy-momentum tensor for scalar fields coupled to the dilaton in two dimensions

We clarify some issues related to the evaluation of the mean value of the energy-momentum tensor for quantum scalar fields coupled to the dilaton field in two-dimensional gravity. Because of this coupling, the energy-momentum tensor for matter is not conserved and therefore it is not determined by the trace anomaly. We discuss different approximations for the calculation of the energy-momentum tensor and show how to obtain the correct amount of Hawking radiation. We also compute cosmological particle creation and quantum corrections to the Newtonian potential.

Cherenkov mesons as in-medium quark energy loss

We recently showed that a heavy quark moving sufficiently fast through a quark-gluon plasma may lose energy by Cherenkov-radiating mesons [1]. Here we review our previous holographic calculation of the energy loss in N=4 Super Yang-Mills and extend it to longitudinal vector mesons and scalar mesons. We also discuss phenomenological implications for heavy-ion collision experiments. Although the Cherenkov energy loss is an O(1/Nc) effect, a ballpark estimate yields a value of dE/dx for Nc=3 which is comparable to that of other mechanisms.

Cherenkov mesons as in-medium quark energy loss

We recently showed that a heavy quark moving sufficiently fast through a quark-gluon plasma may lose energy by Cherenkov-radiating mesons [1]. Here we review our previous holographic calculation of the energy loss in N=4 Super Yang-Mills and extend it to longitudinal vector mesons and scalar mesons. We also discuss phenomenological implications for heavy-ion collision experiments. Although the Cherenkov energy loss is an O(1/Nc) effect, a ballpark estimate yields a value of dE/dx for Nc=3 which is comparable to that of other mechanisms.

Very-High-Energy gamma rays from a Distant Quasar: How Transparent Is the Universe?

The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detected very-high-energy gamma rays from a giant flare of the distant Quasi-Stellar Radio Source (in short: radio quasar) 3C 279, at a distance of more than 5 billion light-years (a redshift of 0.536). No quasar has been observed previously in very-high-energy gamma radiation, and this is also the most distant object detected emitting gamma rays above 50 gigaelectron volts. Because high-energy gamma rays may be stopped by interacting with the diffuse background light in the universe, the observations by MAGIC imply a low amount for such light, consistent with that known from galaxy counts.

Teollisuuden energiaverorasitus EU-maissa ja eräissä muissa maissa

Useat maat ovat 1990-luvulla ottaneet käyttöön energiaveroja. Energiaverot vaikuttavat etenkin energiavaltaisen teollisuuden toimintaan. Energiaverojen aiheuttamien kustannusten siirto hintoihin on hankalaa tuotteiden kilpaillessa maailmanmarkkinoilla. Suomen perusteollisuus on hyvin energiaintensiivistä ja sen monet tuotteet on suunnattu vientiin. Suomen lisäksi kaikkia teollisuuden käyttämiä polttoaineita verotetaan vain Alanko-maissa, Italiassa ja Tanskassa. Teollisuudelle on usein lisäksi alhaisempi verotaso kuin kotitalouksille. Energiaverotasojen tarkastelu sellaisenaan ei kerro veron todellista vaikutusta. Diplo-mityössä tarkastellaan teollisuuden maksamien energiaverojen taloudellista rasittavuutta vertaamalla maksettuja energiaveroja tuotannon jalostusarvoon. Energiaveroja ympä-ristönäkökohdista tarkastellaan vertaamalla maksettuja energiaveroja hiilidioksidipäästöihin. Diplomityössä käsitellään kolmea teollisuuden energiavaltaisinta toimialaa: metsäteollisuutta, metallien jalostusta sekä kemianteollisuutta. Vertailumaina ovat Euroopan Unionin 15 jäsenmaan lisäksi Norja, Sveitsi, Japani, Kanada ja Yhdysvallat. Sähkön kulutus- ja/tai tuotantovero on monissa maissa ja useimmilla toimialoilla merkittävin yksittäinen energiavero. Sähkön käyttö teollisuudessa on runsasta, joten sillä on muita veroja selvemmin havaittava vaikutus verorasitusten kasvuun.

Spectral energy distribution of the gamma-ray microquasar LS 5039

The microquasar LS 5039 has recently been detected as a source of very high energy (VHE) $\gamma$-rays. This detection, that confirms the previously proposed association of LS 5039 with the EGRET source 3EG~J1824$-$1514, makes of LS 5039 a special system with observational data covering nearly all the electromagnetic spectrum. In order to reproduce the observed spectrum of LS 5039, from radio to VHE $\gamma$-rays, we have applied a cold matter dominated jet model that takes into account accretion variability, the jet magnetic field, particle acceleration, adiabatic and radiative losses, microscopic energy conservation in the jet, and pair creation and absorption due to the external photon fields, as well as the emission from the first generation of secondaries. The radiative processes taken into account are synchrotron, relativistic Bremsstrahlung and inverse Compton (IC). The model is based on a scenario that has been characterized with recent observational results, concerning the orbital parameters, the orbital variability at X-rays and the nature of the compact object. The computed spectral energy distribution (SED) shows a good agreement with the available observational data.