Pavlov, A. K. 2013 银河系伽马暴解释AD 775的C14增加

主要内容:
主要集中于爆发后如果产生地球上各种元素的演化。

精彩摘抄:

文章信息:

· Find Similar Abstracts (with default settings below)

· Electronic Refereed Journal Article (HTML)

· Full Refereed Journal Article (PDF/Postscript)

· arXiv e-print (arXiv:1308.1272)

· References in the article

· Citations to the Article (1) (Citation History)

· Refereed Citations to the Article

· Also-Read Articles (Reads History)

·

· Translate This Page

Title:		AD 775 pulse of cosmogenic radionuclides production as imprint of a Galactic gamma-ray burst
Authors:		Pavlov, A. K.; Blinov, A. V.; Konstantinov, A. N.; Ostryakov, V. M.; Vasilyev, G. I.; Vdovina, M. A.; Volkov, P. A.
Affiliation:		AA(A.F. Ioffe Physical Technical Institute of RAS, 26 Polytechnicheskaya, St. Petersburg 194021, Russian Federation; St. Petersburg State Polytechnic University, 29 Polytechnicheskaya, St. Petersburg 195251, Russian Federation; anatoli.pavlov@mail.ioffe.ru), AB(St. Petersburg State Polytechnic University, 29 Polytechnicheskaya, St. Petersburg 195251, Russian Federation), AC(St. Petersburg State Polytechnic University, 29 Polytechnicheskaya, St. Petersburg 195251, Russian Federation), AD(St. Petersburg State Polytechnic University, 29 Polytechnicheskaya, St. Petersburg 195251, Russian Federation), AE(A.F. Ioffe Physical Technical Institute of RAS, 26 Polytechnicheskaya, St. Petersburg 194021, Russian Federation), AF(A.F. Ioffe Physical Technical Institute of RAS, 26 Polytechnicheskaya, St. Petersburg 194021, Russian Federation), AG(St. Petersburg State Polytechnic University, 29 Polytechnicheskaya, St. Petersburg 195251, Russian Federation)
Publication:		Monthly Notices of the Royal Astronomical Society, Volume 435, Issue 4, p.2878-2884 (MNRAS Homepage)
Publication Date:		11/2013
Origin:		OUP
Astronomy Keywords:		Earth, gamma-ray burst: general, Galaxy: general
Abstract Copyright:		2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
DOI:		10.1093/mnras/stt1468
Bibliographic Code:		2013MNRAS.435.2878P

Abstract

We suggest an explanation of a sharp increase in the abundance of cosmogenic radiocarbon found in tree rings dated AD 775. The increase could originate from high-energy irradiation of the atmosphere by a Galactic gamma-ray burst. We argue that, unlike a cosmic ray event, a gamma-ray burst does not necessarily result in a substantial increase in long-lived ¹⁰Be atmospheric production. At the same time, the ³⁶Cl nuclide would be generated in the amounts detectable in the corresponding ice-core samples from Greenland and Antarctica. These peculiar features allow experimental discrimination of nuclide effects caused by gamma-ray bursts and by powerful proton events.

---

Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)