Is the 0.36keV X-ray a Sign of the Existence of Antimatter Domains ? *
XU Chong-ming1 , WANG Xiang-yu1 , ZHAO Yong-heng2 , WU Xue-jun1
1 Department of Physics, Nanjing Normal University, Nanjing 210097
2 Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012
Is the 0.36keV X-ray a Sign of the Existence of Antimatter Domains ? *
XU Chong-ming1 ;WANG Xiang-yu1 ;ZHAO Yong-heng2 ;WU Xue-jun1
1 Department of Physics, Nanjing Normal University, Nanjing 210097
2 Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012
关键词 :
95.85.Nv ,
98.80.-k ,
98.70.Vc
Abstract : If the universe consisted of domains of matter and antimatter, annihilations of e+ -e- at the domain interface in the recombination time would leave an imprint on the x-ray band due to the high redshift. We found five ROSAT sources with the 0.36keV spectral line, especially the source lRXP J005510-3738.8 has a single sharp spectral line almost without a continuous spectrum. It is hard to be produced by any mechanism except the annihilations of e+ -e- .
Key words :
95.85.Nv
98.80.-k
98.70.Vc
出版日期: 1999-03-01
引用本文:
XU Chong-ming;WANG Xiang-yu;ZHAO Yong-heng;WU Xue-jun. Is the 0.36keV X-ray a Sign of the Existence of Antimatter Domains ? *[J]. 中国物理快报, 1999, 16(3): 232-234.
XU Chong-ming, WANG Xiang-yu, ZHAO Yong-heng, WU Xue-jun. Is the 0.36keV X-ray a Sign of the Existence of Antimatter Domains ? *. Chin. Phys. Lett., 1999, 16(3): 232-234.
链接本文:
https://cpl.iphy.ac.cn/CN/
或
https://cpl.iphy.ac.cn/CN/Y1999/V16/I3/232
[1]
HUANG Zhuo-Yi;WANG Bin;CAI Rong-Gen;SU Ru-Keng;. Dark Energy: Relating the Evolutions of the Universe from the Past to the Future [J]. 中国物理快报, 2006, 23(9): 2621-2624.
[2]
DENG Xue-Mei;WU Ya-Bo;ZHAO Guo-Ming. A Parametric Dynamic Model of Dark Energy [J]. 中国物理快报, 2006, 23(6): 1655-1658.
[3]
XIAO Wei-Ke;PENG Chang;YE Xian-Feng;HAO Heng. Detection of a Physical Difference between the CDM Halos in Simulation and in Nature [J]. 中国物理快报, 2006, 23(5): 1355-1358.
[4]
WANG Wei;GUI Yuan-Xing;SHAO Ying. Development of the Model of the Generalized Quintom Dark Energy [J]. 中国物理快报, 2006, 23(3): 762-764.
[5]
SHAO Ying;GUI Yuan-Xing;WANG Wei
. Scalar Field Model of Dark Energy In the Double Complex Symmetric Gravitational Theory [J]. 中国物理快报, 2006, 23(1): 7-9.
[6]
WU Pu-Xun;YU Hong-Wei. Relic Gravitational Waves and Trans-Planckian Physics [J]. 中国物理快报, 2005, 22(9): 2161-2164.
[7]
ZHANG Yang; ZHAO Wen;YUAN Ye-Fei;XIA Tian-Yang. Numeric Spectrum of Relic Gravitational Waves in Accelerating Universe [J]. 中国物理快报, 2005, 22(7): 1817-1820.
[8]
LIN Gui-Fang;ZHANG Li;. X-Ray Emission from Rotation-Powered Pulsars [J]. 中国物理快报, 2005, 22(4): 1022-1024.
[9]
HAO Jian-Gang;JIN Xing-Hua;KUANG Ji;LI Xin-Zhou. An Analytical Inflation Model with Born-Infeld Type Scalar Field [J]. 中国物理快报, 2004, 21(3): 592-594.
[10]
ZHANG Li;WU Jie;JIANG Ze-Jun;MEI Dong-Cheng. Gamma-Ray Pulsars Expected in the Outer Gap Model of Gamma-Ray
Emission [J]. 中国物理快报, 2003, 20(3): 433-435.
[11]
ZHANG Li;JIANG Ze-Jun. Fluxes and Death Lines of Gamma-Ray Pulsars [J]. 中国物理快报, 2003, 20(12): 2273-2276.
[12]
ZHANG Li;;K. S. Cheng;MEI Dong-Cheng;. Cosmic-Ray Positrons Produced by Pulsar Winds from Mature Gamma-Ray Pulsars [J]. 中国物理快报, 2001, 18(5): 701-704.
[13]
FENG Long-Long; XIANG Shou-Ping. Scale-Scale Correlation as Discriminant Among the Biased Galaxy Formation Models [J]. 中国物理快报, 2001, 18(5): 711-714.
[14]
CAO Li;ZHANG Yuan-Zhong;ZHU Zong-Hong;. Robustness of the Sunyaev-Zel’dovich Effect as a Measure of the Hubble Constant [J]. 中国物理快报, 2001, 18(4): 622-624.
[15]
LIN Wen-Bin. Remarks on the Theory of Cosmological Perturbation [J]. 中国物理快报, 2001, 18(11): 1539-1542.