Hunting 1-500 GeV Dark Matter Gamma-ray Lines with the Fermi LAT

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Publisher :
ISBN 13 :
Total Pages : 28 pages
Book Rating : 4.:/5 (724 download)

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Book Synopsis Hunting 1-500 GeV Dark Matter Gamma-ray Lines with the Fermi LAT by : Gilles Vertongen

Download or read book Hunting 1-500 GeV Dark Matter Gamma-ray Lines with the Fermi LAT written by Gilles Vertongen and published by . This book was released on 2010 with total page 28 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Hunting Dark Matter Gamma-ray Lines with the Fermi LAT

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Publisher :
ISBN 13 :
Total Pages : 31 pages
Book Rating : 4.:/5 (837 download)

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Book Synopsis Hunting Dark Matter Gamma-ray Lines with the Fermi LAT by : Gilles Vertongen

Download or read book Hunting Dark Matter Gamma-ray Lines with the Fermi LAT written by Gilles Vertongen and published by . This book was released on 2011 with total page 31 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Searching for Dark Matter with Cosmic Gamma Rays

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Publisher : Morgan & Claypool Publishers
ISBN 13 : 1681742705
Total Pages : 82 pages
Book Rating : 4.6/5 (817 download)

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Book Synopsis Searching for Dark Matter with Cosmic Gamma Rays by : Andrea Albert

Download or read book Searching for Dark Matter with Cosmic Gamma Rays written by Andrea Albert and published by Morgan & Claypool Publishers. This book was released on 2016-09-06 with total page 82 pages. Available in PDF, EPUB and Kindle. Book excerpt: Searching for Dark Matter with Cosmic Gamma Rays summarizes the evidence for dark matter and what we can learn about its particle nature using cosmic gamma rays. It has almost been 100 years since Fritz Zwicky first detected hints that most of the matter in the Universe that doesn't directly emit or reflect light. Since then, the observational evidence for dark matter has continued to grow. Dark matter may be a new kind of particle that is governed by physics beyond our Standard Model of particle physics. In many models, dark matter annihilation or decay produces gamma rays. There are a variety of instruments observing the gamma-ray sky from tens of MeV to hundreds of TeV. Some make deep, focused observations of small regions, while others provide coverage of the entire sky. Each experiment offers complementary sensitivity to dark matter searches in a variety of target sizes, locations, and dark matter mass scales. We review results from recent gamma-ray experiments including anomalies some have attributed to dark matter. We also discuss how our gamma-ray observations complement other dark matter searches and the prospects for future experiments.

Fermi LAT Search for Photon Lines from 30 to 200 GeV.

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ISBN 13 :
Total Pages : 6 pages
Book Rating : 4.:/5 (893 download)

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Book Synopsis Fermi LAT Search for Photon Lines from 30 to 200 GeV. by :

Download or read book Fermi LAT Search for Photon Lines from 30 to 200 GeV. written by and published by . This book was released on 2010 with total page 6 pages. Available in PDF, EPUB and Kindle. Book excerpt: Dark matter (DM) particle annihilation or decay can produce monochromatic [gamma]-rays readily distinguishable from astrophysical sources. [gamma]-ray line limits from 30 GeV to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selection based on requirements for a [gamma]-ray line analysis, and integrated over most of the sky. We obtain [gamma]-ray line flux upper limits in the range 0.6-4.5 x 10−9 cm−2s−1, and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.

Search for Gamma-ray Spectral Lines with the Fermi Large Area Telescope and Dark Matter Implications

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ISBN 13 :
Total Pages : pages
Book Rating : 4.:/5 (858 download)

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Book Synopsis Search for Gamma-ray Spectral Lines with the Fermi Large Area Telescope and Dark Matter Implications by : Andrea Marie Albert

Download or read book Search for Gamma-ray Spectral Lines with the Fermi Large Area Telescope and Dark Matter Implications written by Andrea Marie Albert and published by . This book was released on 2013 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: Abstract: Measurements indicate that ~85% of the matter in the universe neither emits nor reflects light--appropriately called "dark matter". We believe dark matter may be primary composed of new particles, but we know very little about their nature. What dark matter is and how it interacts is one of the top cosmological mysteries today. Detecting a signal from particle dark matter would not only offer insight into the fundamental nature of dark matter, but it would also be strong evidence for physics existing beyond the Standard Model. A promising dark matter candidate is a weakly interacting massive particle (WIMP). Measurements indicate that the Milky Way Galaxy resides in a halo of dark matter, making it an ideal laboratory for investigating these elusive particles. As WIMPs are predicted to be heavy, their interactions should produce high-energy gamma rays that would be detected by the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope (Fermi). If WIMPs annihilate directly into gamma rays, the gamma-ray energy would be the same as the rest mass energy of the WIMPs, which is currently unknown. This process would cause a "pile-up" of gamma rays at a specific energy, producing a sharp line (or bump) in the otherwise relatively smooth gamma-ray energy spectrum. This distinctive signal would not only be strong evidence for the existence of WIMPs, but would also provide information about their mass. We have searched for spectral lines in the energy range 5 to 300 GeV using 3.7 years of Fermi LAT data, reprocessed with updated calorimeter calibration constants, and an improved energy dispersion model from previous LAT Collaboration line searches. We search in five regions selected to optimize sensitivity to different theoretically-motivated density distributions of WIMPs. We do not find any globally significant lines in our a priori search regions and present 95% confidence limits for annihilation cross section and decay lifetimes. We extensively discuss potential systematic effects in the search. Finally, we consider claims of evidence for a spectral line at 130 GeV, compare our results to previous work, and discuss why this search finds a somewhat lower statistical significance for a potential line than other works.

Fermi LAT Search for Dark Matter in Gamma-Ray Lines and the Inclusive Photon Spectrum

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Publisher :
ISBN 13 :
Total Pages : pages
Book Rating : 4.:/5 (951 download)

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Book Synopsis Fermi LAT Search for Dark Matter in Gamma-Ray Lines and the Inclusive Photon Spectrum by :

Download or read book Fermi LAT Search for Dark Matter in Gamma-Ray Lines and the Inclusive Photon Spectrum written by and published by . This book was released on 2013 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt:

The Search for WIMP Dark Matter Continuum Gamma-ray Emission from Dark Matter Satellites in the Milky Way Using the Fermi LAT

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Publisher : Stanford University
ISBN 13 :
Total Pages : 167 pages
Book Rating : 4.F/5 ( download)

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Book Synopsis The Search for WIMP Dark Matter Continuum Gamma-ray Emission from Dark Matter Satellites in the Milky Way Using the Fermi LAT by : Wang Ping

Download or read book The Search for WIMP Dark Matter Continuum Gamma-ray Emission from Dark Matter Satellites in the Milky Way Using the Fermi LAT written by Wang Ping and published by Stanford University. This book was released on 2011 with total page 167 pages. Available in PDF, EPUB and Kindle. Book excerpt: This thesis focuses on the search for unknown dark matter (DM) satellites in the Milky Way using the Fermi Large Area Space Telescope (LAT). The Fermi Gamma-ray Space Telescope (Fermi) is a next generation space observatory, which was successfully launched on June 11th, 2008. The LAT is the principal scientific instrument onboard. Its unprecedented angular resolution and sensitivity in the 100 MeV to > 300 GeV energy range makes it an excellent instrument for probing the sky for DM satellites. Current N-body simulations based on the Lambda-CDM cosmology model predict a large number of as yet unobserved DM satellites in our galaxy; some satellites are predicted to be extended sources (> 1deg extension) as seen by the LAT. Our work assumes that a significant component of DM is a Weakly Interacting Massive Particle (WIMP) in the 100 GeV mass range. The annihilation of WIMPs results in many high energy gamma rays that can be well measured by the LAT. The WIMP produced gamma-ray spectrum from the putative DM satellites is considerably harder than most astrophysical sources. Also, DM satellites have no astronomical counterparts in the X-ray and radio bands, and the emission has no time variability. My thesis will focus on a blind analysis in the search for unknown DM satellites using one year of LAT data, and setting constraints on some WIMP models based on the results of our analysis in which we find no candidates.

The 111 and 129 GeV Gamma-ray Lines from Annihilations in the Milky Way Dark Matter Halo, Dark Disk and Subhalos

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Publisher :
ISBN 13 :
Total Pages : 13 pages
Book Rating : 4.:/5 (951 download)

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Book Synopsis The 111 and 129 GeV Gamma-ray Lines from Annihilations in the Milky Way Dark Matter Halo, Dark Disk and Subhalos by :

Download or read book The 111 and 129 GeV Gamma-ray Lines from Annihilations in the Milky Way Dark Matter Halo, Dark Disk and Subhalos written by and published by . This book was released on 2013 with total page 13 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Detecting Dark Matter Annihilation Lines with Fermi

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Publisher :
ISBN 13 :
Total Pages : 4 pages
Book Rating : 4.:/5 (727 download)

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Book Synopsis Detecting Dark Matter Annihilation Lines with Fermi by :

Download or read book Detecting Dark Matter Annihilation Lines with Fermi written by and published by . This book was released on 2009 with total page 4 pages. Available in PDF, EPUB and Kindle. Book excerpt: Dark matter constitutes one of the most intriguing but so far unresolved issues in physics today. In many extensions of the Standard Model the existence of a stable Weakly Interacting Massive Particle (WIMP) is predicted. The WIMP is an excellent dark matter particle candidate and one of the most interesting scenarios include an annihilation of two WIMPs into two gamma-rays. If the WIMPs are assumed to be non-relativistic, the resulting photons will both have an energy equal to the mass of the WIMP and manifest themselves as a monochromatic spectral line in the energy spectrum. This type of signal would represent a 'smoking gun' for dark matter, since no other known astrophysical process should be able to produce it. In these proceedings we give an overview of the different approaches to a search for dark matter lines that the Fermi-LAT collaboration is pursuing and the various challenges involved.

Gamma Ray Lines from Dark Matter Annihilation

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ISBN 13 :
Total Pages : 13 pages
Book Rating : 4.:/5 (893 download)

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Book Synopsis Gamma Ray Lines from Dark Matter Annihilation by :

Download or read book Gamma Ray Lines from Dark Matter Annihilation written by and published by . This book was released on 1989 with total page 13 pages. Available in PDF, EPUB and Kindle. Book excerpt: If direct annihilation of dark matter particles into a pair of photons occurs in the galactic halo, a narrow [gamma]-ray line can be discovered at future [gamma]-ray detectors sensitive to the GeV region. The signals predicted by different dark matter candidates are analyzed. 16 refs., 3 figs.

Indirect Searches for Dark Matter with the Fermi Large Area Telescope

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ISBN 13 :
Total Pages : 7 pages
Book Rating : 4.:/5 (925 download)

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Book Synopsis Indirect Searches for Dark Matter with the Fermi Large Area Telescope by :

Download or read book Indirect Searches for Dark Matter with the Fermi Large Area Telescope written by and published by . This book was released on 2015 with total page 7 pages. Available in PDF, EPUB and Kindle. Book excerpt: There is overwhelming evidence that non-baryonic dark matter constitutes ~ 27% of the energy density of the Universe. Weakly Interacting Massive Particles (WIMPs) are promising dark matter candidates that may produce [gamma] rays via annihilation or decay detectable by the Fermi Large Area Telescope (LAT). A detection of WIMPs would also indicate the existence of physics beyond the Standard Model. We present recent results from the two cleanest indirect WIMP searches by the Fermi-LAT Collaboration: searches for [gamma]-ray spectral lines and [gamma]-ray emission associated with Milky Way dwarf spheroidal satellite galaxies.

The Characterization of the Gamma-Ray Signal from the Central Milky Way

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Publisher :
ISBN 13 :
Total Pages : 26 pages
Book Rating : 4.:/5 (951 download)

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Book Synopsis The Characterization of the Gamma-Ray Signal from the Central Milky Way by :

Download or read book The Characterization of the Gamma-Ray Signal from the Central Milky Way written by and published by . This book was released on 2014 with total page 26 pages. Available in PDF, EPUB and Kindle. Book excerpt: Past studies have identified a spatially extended excess of ~1-3 GeV gamma rays from the region surrounding the Galactic Center, consistent with the emission expected from annihilating dark matter. We revisit and scrutinize this signal with the intention of further constraining its characteristics and origin. By applying cuts to the Fermi event parameter CTBCORE, we suppress the tails of the point spread function and generate high resolution gamma-ray maps, enabling us to more easily separate the various gamma-ray components. Within these maps, we find the GeV excess to be robust and highly statistically significant, with a spectrum, angular distribution, and overall normalization that is in good agreement with that predicted by simple annihilating dark matter models. For example, the signal is very well fit by a 31-40 GeV dark matter particle annihilating to b quarks with an annihilation cross section of sigma v = (1.4-2.0) x 10^-26 cm^3/s (normalized to a local dark matter density of 0.3 GeV/cm^3). Furthermore, we confirm that the angular distribution of the excess is approximately spherically symmetric and centered around the dynamical center of the Milky Way (within ~0.05 degrees of Sgr A*), showing no sign of elongation along or perpendicular to the Galactic Plane. The signal is observed to extend to at least 10 degrees from the Galactic Center, disfavoring the possibility that this emission originates from millisecond pulsars.

Constraining Decaying Dark Matter with Fermi LAT Gamma-rays

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Publisher :
ISBN 13 :
Total Pages : 23 pages
Book Rating : 4.:/5 (52 download)

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Book Synopsis Constraining Decaying Dark Matter with Fermi LAT Gamma-rays by :

Download or read book Constraining Decaying Dark Matter with Fermi LAT Gamma-rays written by and published by . This book was released on 2009 with total page 23 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Detecting Gamma-ray Anisotropies from Decaying Dark Matter

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Publisher :
ISBN 13 :
Total Pages : 0 pages
Book Rating : 4.:/5 (466 download)

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Book Synopsis Detecting Gamma-ray Anisotropies from Decaying Dark Matter by : Alejandro Ibarra

Download or read book Detecting Gamma-ray Anisotropies from Decaying Dark Matter written by Alejandro Ibarra and published by . This book was released on 2009 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt:

The Search for Dark Matter with the Fermi Gamma Ray Space Telescope

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Publisher :
ISBN 13 :
Total Pages : pages
Book Rating : 4.:/5 (94 download)

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Book Synopsis The Search for Dark Matter with the Fermi Gamma Ray Space Telescope by :

Download or read book The Search for Dark Matter with the Fermi Gamma Ray Space Telescope written by and published by . This book was released on 2011 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: The Fermi Gamma-Ray Space Telescope has been scanning the gamma ray sky since it was launched by NASA in June 2008 and has a mission lifetime goal of 10 years. Largely due to our particle physics heritage, one of the main physics topics being studied by the Fermi LAT Collaboration is the search for dark matter via indirect detection. My talk will review the progress of these studies, something on how the LAT detector enables them, and expectations for the future. I will discuss both gamma-ray and (electron + positron) searches for dark matter, and some resulting theoretical implications.

Intense Gamma-ray Lines from Hidden Vector Dark Matter Decay

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Publisher :
ISBN 13 :
Total Pages : 28 pages
Book Rating : 4.:/5 (52 download)

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Book Synopsis Intense Gamma-ray Lines from Hidden Vector Dark Matter Decay by : Chiara Arina

Download or read book Intense Gamma-ray Lines from Hidden Vector Dark Matter Decay written by Chiara Arina and published by . This book was released on 2009 with total page 28 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Limits on Dark Matter Annihilation Signals from the Fermi LAT 4-year Measurement of the Isotropic Gamma-Ray Background

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Publisher :
ISBN 13 :
Total Pages : 47 pages
Book Rating : 4.:/5 (925 download)

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Book Synopsis Limits on Dark Matter Annihilation Signals from the Fermi LAT 4-year Measurement of the Isotropic Gamma-Ray Background by :

Download or read book Limits on Dark Matter Annihilation Signals from the Fermi LAT 4-year Measurement of the Isotropic Gamma-Ray Background written by and published by . This book was released on 2015 with total page 47 pages. Available in PDF, EPUB and Kindle. Book excerpt: We search for evidence of dark matter (DM) annihilation in the isotropic gamma-ray background (IGRB) measured with 50 months of Fermi Large Area Telescope (LAT) observations. An improved theoretical description of the cosmological DM annihilation signal, based on two complementary techniques and assuming generic weakly interacting massive particle (WIMP) properties, renders more precise predictions compared to previous work. More specifically, we estimate the cosmologically-induced gamma-ray intensity to have an uncertainty of a factor ~ 20 in canonical setups. We consistently include both the Galactic and extragalactic signals under the same theoretical framework, and study the impact of the former on the IGRB spectrum derivation. We find no evidence for a DM signal and we set limits on the DM-induced isotropic gamma-ray signal. Our limits are competitive for DM particle masses up to tens of TeV and, indeed, are the strongest limits derived from Fermi LAT data at TeV energies. This is possible thanks to the new Fermi LAT IGRB measurement, which now extends up to an energy of 820 GeV. As a result, we quantify uncertainties in detail and show the potential this type of search offers for testing the WIMP paradigm with a complementary and truly cosmological probe of DM particle signals.