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The Search for Coincident Gamma-Ray Emission From Fast Radio Bursts With the HAWC Observatory
The Search for Coincident Gamma-Ray Emission From Fast Radio Bursts With the HAWC Observatory
상세정보
- 자료유형
- 학위논문 서양
- 최종처리일시
- 20250211151126
- ISBN
- 9798383182987
- DDC
- 523
- 서명/저자
- The Search for Coincident Gamma-Ray Emission From Fast Radio Bursts With the HAWC Observatory
- 발행사항
- [Sl] : University of Maryland, College Park, 2024
- 발행사항
- Ann Arbor : ProQuest Dissertations & Theses, 2024
- 형태사항
- 185 p
- 주기사항
- Source: Dissertations Abstracts International, Volume: 86-01, Section: B.
- 주기사항
- Advisor: Goodman, Jordan A.
- 학위논문주기
- Thesis (Ph.D.)--University of Maryland, College Park, 2024.
- 초록/해제
- 요약In 2007 a new class of radio transients was discovered, coming from outside of our galaxy with high fluence emitted in the radio band on millisecond timescales. These bursts of radio waves emitted within an order of magnitude of the power of the least bright gamma- ray bursts. These fast radio bursts (FRBs) have since become the target of many searches across radio observatories and multiwavelength follow-up campaigns, but their origin re- mains unknown. In order to understand more about these fascinating events, continued multiwavelength follow-ups are necessary to provide a more complete picture. The High Altitude Water Cherenkov (HAWC) observatory is a very-high-energy gamma-ray detector covering the range of 100 GeV to 300 TeV that is well suited to the detection of transient phenomena due its high live-time and wide field of view, and in particular for a follow- up search on FRBs to determine possible very high energy gamma-ray coincidences. The search for gamma-ray signals from FRBs consists of two searches: first is a persistent source search to identify if FRB emission ever comes from TeV gamma-ray emitting galaxies, and a transient search centered on the reported burst time and location. The results of the FRB search within the HAWC data sets the most constraining limits on the widest population of FRBs ever searched in the VHE band.
- 일반주제명
- Astrophysics
- 일반주제명
- Electromagnetics
- 일반주제명
- Astronomy
- 일반주제명
- Particle physics
- 기타저자
- University of Maryland, College Park Physics
- 기본자료저록
- Dissertations Abstracts International. 86-01B.
- 전자적 위치 및 접속
- 로그인 후 원문을 볼 수 있습니다.
MARC
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■020 ▼a9798383182987
■035 ▼a(MiAaPQ)AAI31147002
■040 ▼aMiAaPQ▼cMiAaPQ
■0820 ▼a523
■1001 ▼aWillox, Elijah Job.▼0(orcid)0000-0002-6623-0277
■24510▼aThe Search for Coincident Gamma-Ray Emission From Fast Radio Bursts With the HAWC Observatory
■260 ▼a[Sl]▼bUniversity of Maryland, College Park▼c2024
■260 1▼aAnn Arbor▼bProQuest Dissertations & Theses▼c2024
■300 ▼a185 p
■500 ▼aSource: Dissertations Abstracts International, Volume: 86-01, Section: B.
■500 ▼aAdvisor: Goodman, Jordan A.
■5021 ▼aThesis (Ph.D.)--University of Maryland, College Park, 2024.
■520 ▼aIn 2007 a new class of radio transients was discovered, coming from outside of our galaxy with high fluence emitted in the radio band on millisecond timescales. These bursts of radio waves emitted within an order of magnitude of the power of the least bright gamma- ray bursts. These fast radio bursts (FRBs) have since become the target of many searches across radio observatories and multiwavelength follow-up campaigns, but their origin re- mains unknown. In order to understand more about these fascinating events, continued multiwavelength follow-ups are necessary to provide a more complete picture. The High Altitude Water Cherenkov (HAWC) observatory is a very-high-energy gamma-ray detector covering the range of 100 GeV to 300 TeV that is well suited to the detection of transient phenomena due its high live-time and wide field of view, and in particular for a follow- up search on FRBs to determine possible very high energy gamma-ray coincidences. The search for gamma-ray signals from FRBs consists of two searches: first is a persistent source search to identify if FRB emission ever comes from TeV gamma-ray emitting galaxies, and a transient search centered on the reported burst time and location. The results of the FRB search within the HAWC data sets the most constraining limits on the widest population of FRBs ever searched in the VHE band.
■590 ▼aSchool code: 0117.
■650 4▼aAstrophysics
■650 4▼aElectromagnetics
■650 4▼aAstronomy
■650 4▼aParticle physics
■653 ▼aFast radio bursts
■653 ▼aGamma-ray astronomy
■653 ▼aHigh Altitude Water Cherenkov
■653 ▼aHigh energy astrophysics
■653 ▼aMulti-wavelength astronomy
■690 ▼a0596
■690 ▼a0798
■690 ▼a0606
■690 ▼a0607
■71020▼aUniversity of Maryland, College Park▼bPhysics.
■7730 ▼tDissertations Abstracts International▼g86-01B.
■790 ▼a0117
■791 ▼aPh.D.
■792 ▼a2024
■793 ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17160849▼nKERIS▼z이 자료의 원문은 한국교육학술정보원에서 제공합니다.
