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We propose the existence of ultracompact minihalos as a new type of massive compact halo object (MACHO) and suggest an observational test to discover them. These new MACHOs are a powerful probe into the nature of dark matter and physics in…

宇宙学与河外天体物理 · 物理学 2015-05-13 M. Ricotti , A. Gould

Ultracompact minihalos would be formed if there are larger density perturbations ($0.0003 < \delta\rho/\rho < 0.3$) in the earlier epoch. The density profile of them is steeper than the standard dark matter halos. If the dark matter can…

宇宙学与河外天体物理 · 物理学 2015-06-11 Yupeng Yang , Guilin Yang , Hongshi Zong

It has been proposed that ultracompact minihalos (UCMHs) might be formed in earlier epoch. If dark matter consists of Weakly Interacting Massive Particles (WIMPs), UCMHs can be treated as the {\gamma}-ray sources due to dark matter…

宇宙学与河外天体物理 · 物理学 2011-12-30 Yupeng Yang , Lei Feng , Xiaoyuan Huang , Xuelei Chen , Tan Lu , Hongshi Zong

Ultracompact minihalos (UCMHs) are dense dark matter structures which can form from large density perturbations shortly after matter-radiation equality. If dark matter is in the form of Weakly Interacting Massive Particles (WIMPs), then…

宇宙学与河外天体物理 · 物理学 2010-11-11 Amandeep S. Josan , Anne M. Green

Analytical calculations and recent numerical experiments have shown that a sizable of the mass in our Galaxy is in a form of clumpy, virialized substructures that, according to \cite{dms:05}, can be as light as $10^{-6} \msun$. In this work…

天体物理学 · 物理学 2009-11-11 Lidia Pieri , Enzo Branchini , Stefan Hofmann

Compared with that of standard dark matter halos, the density profile of the recently proposed new kind of dark matter structure named ultracompact minihalos (UCMHs) is steeper and its formation time is earlier. If the dark matter is…

宇宙学与河外天体物理 · 物理学 2013-06-27 Yupeng Yang , Guilin Yang , Hongshi Zong

Events like inflation or phase transitions can produce large density perturbations on very small scales in the early Universe. Probes of small scales are therefore useful for e.g. discriminating between inflationary models. Until recently,…

宇宙学与河外天体物理 · 物理学 2012-08-13 Pat Scott , Torsten Bringmann , Yashar Akrami

If the dark matter in the Universe is made of weakly self-interacting particles, they may self-annihilate and emit gamma-rays. We use high resolution numerical simulations to estimate directly the annihilation flux from the central regions…

天体物理学 · 物理学 2009-09-25 Felix Stoehr , Simon D. M. White , Volker Springel , Giuseppe Tormen , Naoki Yoshida

The possibility that primordial black hole binary mergers of stellar mass can explain the signals detected by the gravitational-wave interferometers has attracted much attention. In this scenario, primordial black holes can comprise only…

宇宙学与河外天体物理 · 物理学 2019-07-01 Tomohiro Nakama , Kazunori Kohri , Joseph Silk

It was proposed that the massive compact halo objects (MCHOs) would be produced during an earlier epoch of cosmology if the density perturbations are between $3 \times 10^{-4}$ and 0.3. Then these objects can accrete dark matter particles…

宇宙学与河外天体物理 · 物理学 2011-09-13 Yupeng Yang , Xiaoyuan Huang , Xuelei Chen , Hongshi Zong

We present the basics of microlensing and give an overview of the results obtained so far. We also describe a scenario in which dark clusters of MACHOs (Massive Astrophysical Compact Halo Objects) and cold molecular clouds (mainly of $H_2$)…

天体物理学 · 物理学 2009-10-31 Ph. Jetzer

Ultracompact minihalos (UCMHs) have emerged as a valuable probe of the primordial power spectrum of density fluctuations at small scales. UCMHs are expected to form at early times in regions with ${\delta\rho/\rho \gtrsim 10^{-3}}$, and…

宇宙学与河外天体物理 · 物理学 2018-03-07 M. Sten Delos , Adrienne L. Erickcek , Avery P. Bailey , Marcelo A. Alvarez

The ultracompact minihalos could be formed during the earlier epoch of the universe. The dark matter annihilation within them is very strong due to the steep density profile, $\rho \sim r^{-2.25}$. The high energy electrons and positrons…

高能天体物理现象 · 物理学 2013-05-01 Yupeng Yang , Guilin Yang , Xiaoyuan Huang , Xuelei Chen , Tan Lu , Hongshi Zong

Ultracompact dark matter minihalos (UCMHs) would be formed during the earlier universe if there were large density perturbations. If the dark matter can decay into the standard model particles, such as neutrinos, these objects would become…

宇宙学与河外天体物理 · 物理学 2015-01-06 Yun-Long Zheng , Yu-Peng Yang , Ming-Zhe Li , Hong-Shi Zong

Ultracompact minihalo (UCMH) is a special type of dark matter halo with a very steep density profile which may form in the early universe seeded by an overdense region or a primordial black hole. Constraints on its abundance give valuable…

宇宙学与河外天体物理 · 物理学 2022-03-18 Xing-Fu Zhang , Ji-Gui Cheng , Ben-Yang Zhu , Tian-Ci Liu , Yun-Feng Liang , En-Wei Liang

The paradigm of the neutralino dark matter predicts that the first gravitationally bound objects are earth-mass sized microhaloes, which would emit annihilation gamma-rays. Here we show that, though the flux from individual nearest…

天体物理学 · 物理学 2009-11-10 Takeshi Oda , Tomonori Totani , Masahiro Nagashima

The failure to find evidence for elementary particles that could serve as the constituents of dark matter brings to mind suggestions that dark matter might consist of massive compact objects (MACHOs). In particular, it has recently been…

广义相对论与量子宇宙学 · 物理学 2016-12-07 G. Chapline , P. H. Frampton

A new kind of dark matter structures, ultracompact minihalos (UCMHs) was proposed recently. They would be formed during the radiation dominated epoch if the large density perturbations are existent. Moreover, if the dark matter is made up…

高能天体物理现象 · 物理学 2011-12-30 Yupeng Yang , Xuelei Chen , Tan Lu , Hongshi Zong

Earth-mass dark matter microhalos with size of ~100 AUs are the first structures formed in the universe, if the dark matter of the Universe are made of neutralino. Here, we report the results of ultra-high-resolution simulations of the…

宇宙学与河外天体物理 · 物理学 2013-04-09 Tomoaki Ishiyama , Junichiro Makino , Toshikazu Ebisuzaki

The local environment is ideal for searching out compact dark structures via the microlensing and multi-frequency emissions as these objects are expected to be faint and microlensing experiments have already hinted at their possibility. In…

宇宙学与河外天体物理 · 物理学 2017-11-16 Geoff Beck , Sergio Colafrancesco
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