Particle Dark Matter: List of contributors

By G. Bertone. 2010

496 citations recorded by the source corpus.

Subfields: Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/f80640c7f36030789df327f7e278cf7e9718290f

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atomic and Molecular Physics, and Optics

1. Paolo Pani
2. H. Ara'ujo
3. V. Chepel
4. V. Cardoso
5. R. Brito
6. L. Strigari
7. P. Salucci
8. M. Pospelov

In Nuclear and High Energy Physics

1. V. Cardoso
2. Paolo Pani
3. R. Brito
4. L. Strigari
5. Lavinia Heisenberg
6. Kent Yagi
7. T. Harmark
8. Justin I. Read

Citations in the corpus

• First results from the NEWS-G direct dark matter search experiment at the LSM (2017, background): “B by summer 2018. Keywords: Spherical Proportional Counter, dark matter, direct detection, low-mass WIMPs 1. Introduction It is now well established, from a wide variety of astrophysical observations [1, 2] and precise measurements of the Cosmological Microwave Background (CMB) [3], that non-baryoni”
• Understanding the shape and diversity of dwarf galaxy rotation curves in ΛCDM (2016, background): “This is typically taken as evidence for an exotic missing mass component – most likely a new particle that lies beyond the standard model of particle physics(1) (e.g. Jungman et al. 1996; Boyarsky et al. 2009; Bertone 2010; Read 2014).”
• Liquid noble gas detectors for low energy particle physics (2012, methodology): “-rotating with the baryon disc to some degree. However, we adopt the simpler halo model for the purpose of this article. For a recent and comprehensive review of dark matter the reader is referred to [11]. Elastic scattering of WIMPs off the atomic nuclei of a target material should result in nuclea”
• AMS-02 antiprotons, at last! Secondary astrophysical component and immediate implications for Dark Matter (2015, background): “In modern times, antiprotons have often been argued to be an important diagnostic tool for cosmic ray sources and propagation properties, and constitute one of the prime channels for indirect searches of Dark Matter (DM) [4, 5], which so far has only been detected gravitationally.”
• Hunting for topological dark matter with atomic clocks (2013, background): “composed of heavy-particlelike matter, and searches for the results of its scattering off individual nuclei [2].”
• Galactic Searches for Dark Matter (2012, background): “…candidates also arise from theories of universal extra dimensions (Cheng et al., 2002; Hooper and Profumo, 2007), as well as many others (Duffy and van Bibber, 2009; Feng, 2010b) (see the recent reviews of Bertone et al. (2005) and Bertone (2010) for a more complete list of dark matter candidates).”
• The distribution of dark matter in galaxies (2018, background): “In the current Λ cold dark matter (Λ CDM) paradigm, the DM is non-relativistic since its decoupling time and can be described by a collisionless fluid, whose particles interact only gravitationally and very weakly with the Standard Model particles (Jungman and al. 1996; Bertone 2010).”
• Black holes, gravitational waves and fundamental physics: a roadmap (2018, background): “The evidence for this mysterious form of matter started to grow in the early 20th century [278], and it is today firmly established thanks to a wide array of independent observations [279].”