ASTROPARTICLE PHYSICS

投稿咨询

官方网站：http://www.journals.elsevier.com/astroparticle-physics/

投稿网址：http://www.journals.elsevier.com/astroparticle-physics/

PMC链接：http://www.ncbi.nlm.nih.gov/nlmcatalog?term=0927-6505%5BISSN%5D

天体粒子物理学在宇宙线物理学、天文学和天体物理学、宇宙学和粒子物理学等相互作用领域发表实验和理论研究论文，重点介绍以下领域的新发展:?高能宇宙射线物理学和天体物理学;?粒子宇宙学;?粒子天体物理学;?相关天体物理学:超新星、AGN、宇宙丰度、暗物质等;?引力波?高能、VHE和UHE伽马天文学;?高能和低能中微子天文学;?与上述领域相关的仪器仪表和检测器开发。新奇和相关性天体粒子物理学的目标是只发表对国际读者有意义的论文，其中包含大量的新颖性和科学影响。编辑保留拒绝接受不符合这些标准的论文的权利，无论是否接受外部审查。这可能包括与以前的出版物非常相似的论文，或者超出范围的论文，例如主要集中在非常理论的发展上，几乎没有直接的直接观测结果，或者缺乏与天文或粒子物理学的直接联系。天体粒子物理学可以考虑发表科学任务建议书。编辑将共同决定此类论文是否适合该期刊，建议作者直接与其中一位编辑联系，讨论建议。

Astroparticle Physics publishes experimental and theoretical research papers in the interacting fields of Cosmic Ray Physics, Astronomy and Astrophysics, Cosmology and Particle Physics focusing on new developments in the following areas:? High-energy cosmic-ray physics and astrophysics;? Particle cosmology;? Particle astrophysics;? Related astrophysics: supernova, AGN, cosmic abundances, dark matter etc.;? Gravitational waves? High-energy, VHE and UHE gamma-ray astronomy;? High- and low-energy neutrino astronomy;? Instrumentation and detector developments related to the above-mentioned fields.Novelty and relevanceAstroparticle Physics aims to only publish papers with significance to an international audience, containing substantial novelty and scientific impact. The Editors reserve the rights to reject, with or without external review, papers that do not meet these criteria. This could include papers that are very similar to previous publications, or that are out of scope, such as concentrated mostly on very theoretical developments with few direct immediate observational consequences, or lacking a direct connection to either astro- or particle physics.Astroparticle Physics may consider the publication of scientific mission proposal papers. The Editors will jointly decide on the suitability of such papers for the journal, authors are advised to contact one of the Editors directly to discuss proposals.