東華大學圖書館 |

語系: 繁體中文

說明(常見問題)

回圖書館首頁

手機版館藏查詢

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Emission of radio waves in particle ...

Zilles, Anne.

FindBook

Google Book

Amazon

博客來

Emission of radio waves in particle showers = validation of microscopic simulations with the SLAC T-510 experiment and their potential in the future square kilometre array /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Emission of radio waves in particle showers/ by Anne Zilles.
其他題名:	validation of microscopic simulations with the SLAC T-510 experiment and their potential in the future square kilometre array /
作者:	Zilles, Anne.
出版者:	Cham :Springer International Publishing : : 2017.,
面頁冊數:	xvi, 130 p. :ill., digital ;24 cm.
內容註:	Introduction -- Cosmic Rays -- Modeling of Radio Emission from Particle\Air Showers -- Testing Predictions for Radio Emission from Particle Showers -- Modeling the Radio Emission from a Particle Shower -- Comparison of Microscopic Simulations to Data of the T-510 Experiment -- Detecting Cosmic Rays with SKA1-low -- Conclusions.
Contained By:	Springer eBooks
標題:	Radio astronomy. -
電子資源:	http://dx.doi.org/10.1007/978-3-319-63411-1
ISBN:	9783319634111

Emission of radio waves in particle showers = validation of microscopic simulations with the SLAC T-510 experiment and their potential in the future square kilometre array /
Zilles, Anne.

Emission of radio waves in particle showersvalidation of microscopic simulations with the SLAC T-510 experiment and their potential in the future square kilometre array /[electronic resource] :by Anne Zilles. - Cham :Springer International Publishing :2017. - xvi, 130 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Cosmic Rays -- Modeling of Radio Emission from Particle\Air Showers -- Testing Predictions for Radio Emission from Particle Showers -- Modeling the Radio Emission from a Particle Shower -- Comparison of Microscopic Simulations to Data of the T-510 Experiment -- Detecting Cosmic Rays with SKA1-low -- Conclusions.

This thesis offers the first laboratory validation of microscopic simulations of radio emission from particle showers, including a detailed description of the simulation study. It presents a potential future avenue for resolving the mass composition of cosmic rays via radio detection of air showers. Particle showers are created from cascading interactions when high-energy particles collide with matter, e.g. with air in the case of cosmic radiation, or with a particle detector in the case of experiments at CERN. These showers can consist of billions of particles, mostly electrons, positrons and photons. They emit radio waves when the absorbing medium is in a magnetic field, and this radio emission can be used as a novel means of detecting and drawing inferences on the shower and the primary particle. The new method is currently being established in cosmic ray research, where large antenna arrays may soon replace or complement traditional particle detectors. In thi s study, a complete microscopic simulation of a radio-emission experiment conducted at Stanford Linear Accelerator Center (SLAC), Stanford/USA, is performed, and the underlying physical models are validated. The model is subsequently applied to the Square Kilometre Array (SKA) project, which is a large interferometer for radio astronomy. It is demonstrated that the SKA, with some modifications, might also be used for cosmic ray research based on radio detection of high-energy particles from the cosmos.

ISBN: 9783319634111

Standard No.: 10.1007/978-3-319-63411-1doiSubjects--Topical Terms:

649695
Radio astronomy.

LC Class. No.: QB476.5

Dewey Class. No.: 522.682

Emission of radio waves in particle showers = validation of microscopic simulations with the SLAC T-510 experiment and their potential in the future square kilometre array /
LDR:02904nmm a2200325 a 4500 001 2106474
003 DE-He213
005 20180320110104.0
006 m d
007 cr nn 008maaau
008 180417s2017 gw s 0 eng d
020 $a 9783319634111 $q (electronic bk.)
020 $a 9783319634104 $q (paper)
024 7 $a 10.1007/978-3-319-63411-1 $2 doi
035 $a 978-3-319-63411-1
040 $a GP $c GP
041 0 $a eng
050 4 $a QB476.5
072 7 $a PHVB $2 bicssc
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 522.682 $2 23
090 $a QB476.5 $b .Z69 2017
100 1 $a Zilles, Anne. $3 3252396
245 1 0 $a Emission of radio waves in particle showers $h [electronic resource] : $b validation of microscopic simulations with the SLAC T-510 experiment and their potential in the future square kilometre array / $c by Anne Zilles.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2017.
300 $a xvi, 130 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- Cosmic Rays -- Modeling of Radio Emission from Particle\Air Showers -- Testing Predictions for Radio Emission from Particle Showers -- Modeling the Radio Emission from a Particle Shower -- Comparison of Microscopic Simulations to Data of the T-510 Experiment -- Detecting Cosmic Rays with SKA1-low -- Conclusions.
520 $a This thesis offers the first laboratory validation of microscopic simulations of radio emission from particle showers, including a detailed description of the simulation study. It presents a potential future avenue for resolving the mass composition of cosmic rays via radio detection of air showers. Particle showers are created from cascading interactions when high-energy particles collide with matter, e.g. with air in the case of cosmic radiation, or with a particle detector in the case of experiments at CERN. These showers can consist of billions of particles, mostly electrons, positrons and photons. They emit radio waves when the absorbing medium is in a magnetic field, and this radio emission can be used as a novel means of detecting and drawing inferences on the shower and the primary particle. The new method is currently being established in cosmic ray research, where large antenna arrays may soon replace or complement traditional particle detectors. In thi s study, a complete microscopic simulation of a radio-emission experiment conducted at Stanford Linear Accelerator Center (SLAC), Stanford/USA, is performed, and the underlying physical models are validated. The model is subsequently applied to the Square Kilometre Array (SKA) project, which is a large interferometer for radio astronomy. It is demonstrated that the SKA, with some modifications, might also be used for cosmic ray research based on radio detection of high-energy particles from the cosmos.
650 0 $a Radio astronomy. $3 649695
650 0 $a Cosmic ray showers. $3 1245333
650 0 $a Antenna arrays. $3 606839
650 1 4 $a Physics. $3 516296
650 2 4 $a Astrophysics and Astroparticles. $3 1067087
650 2 4 $a Numerical and Computational Physics, Simulation. $3 2209853
650 2 4 $a Measurement Science and Instrumentation. $3 1066390
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 1314442
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-63411-1
950 $a Physics and Astronomy (Springer-11651)