ERRATUM: "SEARCH FOR DARK MATTER ANNIHILATION SIGNALS FROM THE FORNAX GALAXY CLUSTER WITH H.E.S.S." (2012, ApJ, 750, 123)

ERRATUM: "SEARCH FOR DARK MATTER ANNIHILATION SIGNALS FROM THE FORNAX GALAXY CLUSTER WITH H.E.S.S." (2012, ApJ, 750, 123)
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勘误表:“用 H.E.S.S 搜索来自福纳克斯星系团的暗物质湮灭信号。”

DOI:
10.1088/0004-637x/783/1/63
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发表时间:
2014
期刊:
The Astrophysical Journal
影响因子:
--
通讯作者:
Abramowski A
Abramowski A
中科院分区:
--
文献类型:
--
作者:
Abramowski A

文献摘要

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图1.MDM=1 TeV暗物质粒子自湮没进入不同通道的光子光谱。给出了从DM完全湮没到BB(点虚线)、τ+τ−(黑色实线)和W+W−(长虚线)的光谱。后者显示了W+W−通道发生的内韧致辐射(IB)效应。文中还绘出了超电子能级模型中B(1)超规范玻色子对被超电子衍射湮没的γ射线谱。这条长虚线显示了在DM粒子湮没成Muon对的情况下,来自终态辐射(FSR)和逆康普顿(IC)散射的光子光谱。
Figure 1. Photon spectra from the self-annihilation of mDM= 1 TeV dark matter particles into different channels. Spectra from DM annihilating purely into bb (dot-dashed line), τ+ τ−(black solid line), and W+W−(long-dashed-dotted line) are shown. The latter shows the effect of Internal Bremsstrahlung (IB) occurring for the W+W− channel. The γ-ray spectrum from the annihilation of B (1) hypergauge boson pairs arising in Kaluza-Klein (KK) models with UED is also plotted (dotted line). The long dashed line show the photon spectra from final-state radiation (FSR) and the inverse Compton (IC) scattering contribution in the case of DM particles annihilating into muon pairs.