activity
20152026
most citedET White Paper: To Find the First Earth 2.0

18 citations · 80 across the 19 of their papers we have counts for

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Showing 2017Show all

7 papers · 1 filter

hep-ph2017

A simple and natural interpretations of the DAMPE cosmic-ray electron/positron spectrum within two sigma deviations

Jia-Shu Niu, Tianjun Li, Fang-Zhou Xu

The DArk Matter Particle Explorer (DAMPE) experiment has recently announced the first results for the measurement of total electron plus positron fluxes between 25 GeV and 4.6 TeV.…

astro-ph.HE2017

Bayesian analysis of the break in DAMPE lepton spectra

Jia-Shu Niu, Tianjun Li, Ran Ding +3

Recently, DAMPE has released its first results on the high-energy cosmic-ray electrons and positrons (CREs) from about GeV to TeV, which directly detect a break at $\sim…

hep-ph2017

Naturalness and Dark Matter in a Realistic Intersecting D6-Brane Model

Waqas Ahmed, Lorenzo Calibbi, Tianjun Li +3

We revisit a three-family Pati-Salam model with a realistic phenomenology from intersecting D6-branes in Type IIA string theory compactified on a $\mathbf{T}^6/(\mathbb{Z}_2 \times…

hep-ph2017

Status of Natural Supersymmetry from the GmSUGRA in Light of the current LHC Run-2 and LUX data

Waqas Ahmed, Xiao-Jun Bi, Tianjun Li +4

We study natural supersymmetry in the Generalized Minimal Supergravity (GmSUGRA). For the parameter space with low energy electroweak fine-tuning measures less than 50, we are left…

astro-ph.HE2017

Probing the dark matter-electron interactions via hydrogen-atmosphere pulsating white dwarfs

Jia-Shu Niu, Tianjun Li, Weikai Zong +2

In this work, we propose a novel scenario to probe the interactions between dark matter (DM) particles and electrons, via hydrogen-atmosphere pulsating white dwarfs (DAVs) in globu…

astro-ph.HE2017

Galactic cosmic-ray model in the light of AMS-02 nuclei data

Jia-Shu Niu, Tianjun Li

Cosmic ray (CR) physics has entered a precision-driven era. With the latest AMS-02 nuclei data (boron-to-carbon ratio, proton flux, helium flux and antiproton-to-proton ratio), we…