93 research outputs found
Diffuse Gamma Rays: Galactic and Extragalactic Diffuse Emission
"Diffuse" gamma rays consist of several components: truly diffuse emission
from the interstellar medium, the extragalactic background, whose origin is not
firmly established yet, and the contribution from unresolved and faint Galactic
point sources. One approach to unravel these components is to study the diffuse
emission from the interstellar medium, which traces the interactions of high
energy particles with interstellar gas and radiation fields. Because of its
origin such emission is potentially able to reveal much about the sources and
propagation of cosmic rays. The extragalactic background, if reliably
determined, can be used in cosmological and blazar studies. Studying the
derived "average" spectrum of faint Galactic sources may be able to give a clue
to the nature of the emitting objects.Comment: 32 pages, 28 figures, kapproc.cls. Chapter to the book "Cosmic
Gamma-Ray Sources," to be published by Kluwer ASSL Series, Edited by K. S.
Cheng and G. E. Romero. More details can be found at
http://www.gamma.mpe-garching.mpg.de/~aws/aws.htm
Nonthermal Emission from Star-Forming Galaxies
The detections of high-energy gamma-ray emission from the nearby starburst
galaxies M82 & NGC253, and other local group galaxies, broaden our knowledge of
star-driven nonthermal processes and phenomena in non-AGN star-forming
galaxies. We review basic aspects of the related processes and their modeling
in starburst galaxies. Since these processes involve both energetic electrons
and protons accelerated by SN shocks, their respective radiative yields can be
used to explore the SN-particle-radiation connection. Specifically, the
relation between SN activity, energetic particles, and their radiative yields,
is assessed through respective measures of the particle energy density in
several star-forming galaxies. The deduced energy densities range from O(0.1)
eV/cm^3 in very quiet environments to O(100) eV/cm^3 in regions with very high
star-formation rates.Comment: 17 pages, 5 figures, to be published in Astrophysics and Space
Science Proceeding
Subcycle Quantum Electrodynamics
Besides their stunning physical properties which are unmatched in a classical
world, squeezed states of electromagnetic radiation bear advanced application
potentials in quantum information systems and precision metrology, including
gravitational wave detectors with unprecedented sensitivity. Since the first
experiments on such nonclassical light, quantum analysis has been based on
homodyning techniques and photon correlation measurements. These methods
require a well-defined carrier frequency and photons contained in a quantum
state need to be absorbed or amplified. They currently function in the visible
to near-infrared and microwave spectral ranges. Quantum nondemolition
experiments may be performed at the expense of excess fluctuations in another
quadrature. Here we generate mid-infrared time-locked patterns of squeezed
vacuum noise. After propagation through free space, the quantum fluctuations of
the electric field are studied in the time domain by electro-optic sampling
with few-femtosecond laser pulses. We directly compare the local noise
amplitude to the level of bare vacuum fluctuations. This nonlinear approach
operates off resonance without absorption or amplification of the field that is
investigated. Subcycle intervals with noise level significantly below the pure
quantum vacuum are found. Enhanced fluctuations in adjacent time segments
manifest generation of highly correlated quantum radiation as a consequence of
the uncertainty principle. Together with efforts in the far infrared, this work
opens a window to the elementary quantum dynamics of light and matter in an
energy range at the boundary between vacuum and thermal background conditions.Comment: 19 pages, 4 figure
Search for gamma-ray emission from magnetars with the Fermi Large Area Telescope
We report on the search for 0.1-10 GeV emission from magnetars in 17 months
of Fermi Large Area Telescope (LAT) observations. No significant evidence for
gamma-ray emission from any of the currently-known magnetars is found. The most
stringent upper limits to date on their persistent emission in the Fermi-LAT
energy range are estimated between ~10^{-12}-10^{-10} erg/s/cm2, depending on
the source. We also searched for gamma-ray pulsations and possible outbursts,
also with no significant detection. The upper limits derived support the
presence of a cut-off at an energy below a few MeV in the persistent emission
of magnetars. They also show the likely need for a revision of current models
of outer gap emission from strongly magnetized pulsars, which, in some
realizations, predict detectable GeV emission from magnetars at flux levels
exceeding the upper limits identified here using the Fermi-LAT observations.Comment: ApJ Letters in press; Corresponding authors: Caliandro G. A., Hadasch
D., Rea N., Burnett
Detection of Gamma-Ray Emission from the Starburst Galaxies M82 and NGC 253 with the Large Area Telescope on Fermi
We report the detection of high-energy gamma-ray emission from two starburst
galaxies using data obtained with the Large Area Telescope on board the Fermi
Gamma-ray Space Telescope. Steady point-like emission above 200 MeV has been
detected at significance levels of 6.8 sigma and 4.8 sigma respectively, from
sources positionally coincident with locations of the starburst galaxies M82
and NGC 253. The total fluxes of the sources are consistent with gamma-ray
emission originating from the interaction of cosmic rays with local
interstellar gas and radiation fields and constitute evidence for a link
between massive star formation and gamma-ray emission in star-forming galaxies.Comment: Submitted to ApJ Letter
Fermi Gamma-ray Imaging of a Radio Galaxy
The Fermi Gamma-ray Space Telescope has detected the gamma-ray glow emanating
from the giant radio lobes of the radio galaxy Centaurus A. The resolved
gamma-ray image shows the lobes clearly separated from the central active
source. In contrast to all other active galaxies detected so far in high-energy
gamma-rays, the lobe flux constitutes a considerable portion (>1/2) of the
total source emission. The gamma-ray emission from the lobes is interpreted as
inverse Compton scattered relic radiation from the cosmic microwave background
(CMB), with additional contribution at higher energies from the
infrared-to-optical extragalactic background light (EBL). These measurements
provide gamma-ray constraints on the magnetic field and particle energy content
in radio galaxy lobes, and a promising method to probe the cosmic relic photon
fields.Comment: 27 pages, includes Supplementary Online Material; corresponding
authors: C.C. Cheung, Y. Fukazawa, J. Knodlseder, L. Stawar
Fermi Large Area Telescope observations of PSR J1836+5925
The discovery of the gamma-ray pulsar PSR J1836+5925, powering the formerly
unidentified EGRET source 3EG J1835+5918, was one of the early accomplishments
of the Fermi Large Area Telescope (LAT). Sitting 25 degrees off the Galactic
plane, PSR J1836+5925 is a 173 ms pulsar with a characteristic age of 1.8
million years, a spindown luminosity of 1.1 erg s, and a
large off-peak emission component, making it quite unusual among the known
gamma-ray pulsar population. We present an analysis of one year of LAT data,
including an updated timing solution, detailed spectral results and a long-term
light curve showing no indication of variability. No evidence for a surrounding
pulsar wind nebula is seen and the spectral characteristics of the off-peak
emission indicate it is likely magnetospheric. Analysis of recent XMM
observations of the X-ray counterpart yields a detailed characterization of its
spectrum, which, like Geminga, is consistent with that of a neutron star
showing evidence for both magnetospheric and thermal emission.Comment: Accepted to Astrophysical Journa
A change in the optical polarization associated with a gamma-ray flare in the blazar 3C 279
It is widely accepted that strong and variable radiation detected over all
accessible energy bands in a number of active galaxies arises from a
relativistic, Doppler-boosted jet pointing close to our line of sight. The size
of the emitting zone and the location of this region relative to the central
supermassive black hole are, however, poorly known, with estimates ranging from
light-hours to a light-year or more. Here we report the coincidence of a
gamma-ray flare with a dramatic change of optical polarization angle. This
provides evidence for co-spatiality of optical and gamma-ray emission regions
and indicates a highly ordered jet magnetic field. The results also require a
non-axisymmetric structure of the emission zone, implying a curved trajectory
for the emitting material within the jet, with the dissipation region located
at a considerable distance from the black hole, at about 10^5 gravitational
radii.Comment: Published in Nature issued on 18 February 2010. Corresponding
authors: Masaaki Hayashida and Greg Madejsk
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
Cosmic Rays and the Search for a Lorentz Invariance Violation
This is an introductory review about the on-going search for a signal of
Lorentz Invariance Violation (LIV) in cosmic rays. We first summarise basic
aspects of cosmic rays, focusing on rays of ultra high energy (UHECRs). We
discuss the Greisen-Zatsepin-Kuz'min (GZK) energy cutoff for cosmic protons,
which is predicted due to photopion production in the Cosmic Microwave
Background (CMB). This is a process of modest energy in the proton rest frame.
It can be investigated to a high precision in the laboratory, if Lorentz
transformations apply even at factors . For heavier
nuclei the energy attenuation is even faster due to photo-disintegration, again
if this process is Lorentz invariant. Hence the viability of Lorentz symmetry
up to tremendous gamma-factors - far beyond accelerator tests - is a central
issue. Next we comment on conceptual aspects of Lorentz Invariance and the
possibility of its spontaneous breaking. This could lead to slightly particle
dependent ``Maximal Attainable Velocities''. We discuss their effect in decays,
Cerenkov radiation, the GZK cutoff and neutrino oscillation in cosmic rays. We
also review the search for LIV in cosmic gamma-rays. For multi TeV gamma-rays
we possibly encounter another puzzle related to the transparency of the CMB,
similar to the GZK cutoff. The photons emitted in a Gamma Ray Burst occur at
lower energies, but their very long path provides access to information not far
from the Planck scale. No LIV has been observed so far. However, even extremely
tiny LIV effects could change the predictions for cosmic ray physics
drastically. An Appendix is devoted to the recent hypothesis by the Pierre
Auger Collaboration, which identifies nearby Active Galactic Nuclei - or
objects next to them - as probable UHECR sources.Comment: 81 pages, 15 figures, some points extended and improved, references
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