dejected
发表于 2025-3-21 19:31:07
书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0872095<br><br> <br><br>书目名称Sources and Detection of Dark Matter and Dark Energy in the Universe读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0872095<br><br> <br><br>
灌输
发表于 2025-3-21 20:49:35
http://reply.papertrans.cn/88/8721/872095/872095_2.png
助记
发表于 2025-3-22 01:03:35
http://reply.papertrans.cn/88/8721/872095/872095_3.png
Itinerant
发表于 2025-3-22 05:51:38
http://reply.papertrans.cn/88/8721/872095/872095_4.png
倔强不能
发表于 2025-3-22 11:02:27
http://reply.papertrans.cn/88/8721/872095/872095_5.png
Cosmopolitan
发表于 2025-3-22 15:18:54
David G. Cerdeño,Ji-Haeng Huh,Miguel Peiró,Osamu Seto
Odyssey
发表于 2025-3-22 17:56:15
Sources and Detection of Dark Matter and Dark Energy in the UniverseProceedings of the 1
Nuance
发表于 2025-3-22 22:31:41
Finite Temperature Density Profile in SFDMt produces cores naturally and that does not require large amounts of feedback would be preferable. We find both requirements to be satisfied in the scalar field dark matter model. Here, we consider that the dark matter is an auto-interacting real scalar field in a thermal bath of temperature T with
CEDE
发表于 2025-3-23 04:52:51
The X,1T Dark Matter Search Experimentand housed in a water Cherenkov muon veto at LNGS, is presented. With an experimental aim of probing WIMP interaction cross-sections above of order .. ∼ 2 × 10. cm. within 2 years of operation, X.1T will provide the sensitivity to probe a particularly favourable region of electroweak physics on a ti
anesthesia
发表于 2025-3-23 09:32:26
http://reply.papertrans.cn/88/8721/872095/872095_10.png