STATUS REPORT ON THE ROSEBUD DARK MATTER EXPERIMENT

Author(s):  
S. CEBRIÁN ◽  
E. GARCÍA ◽  
D. GONZÁLEZ ◽  
I. G. IRASTORZA ◽  
A. MORALES ◽  
...  
Keyword(s):  
1999 ◽  
Vol 70 (1-3) ◽  
pp. 101-105 ◽  
Author(s):  
B. van den Brandt ◽  
S. Casalbuoni ◽  
G. Czapek ◽  
U. Diggelmann ◽  
T. Ebert ◽  
...  

2010 ◽  
Author(s):  
Lars Bergström ◽  
Jean-Michel Alimi ◽  
André Fuözfa
Keyword(s):  

2015 ◽  
Vol 30 (15) ◽  
pp. 1540011 ◽  
Author(s):  
Géraldine Servant

Although they do not address the hierarchy problem, models with Universal Extra Dimensions have attracted a lot of attention as simple benchmark models characterized by small mass splittings and a dark matter (DM) WIMP played by the Lightest Kaluza–Klein particle (LKP). We review their status, with emphasis on minimal implementation in five dimensions (MUED) in which the LKP is a massive hypercharge gauge boson. In this case, the mass range accounting for the correct DM abundance (around 1.4 TeV) remains untouched by LHC8 and is out of reach of present DM direct detection experiments. However, LHC14 can probe the relevant region in the 3-lepton channel.


Author(s):  
Aurélien Barrau ◽  
Killian Martineau ◽  
Flora Moulin

The understanding of black holes in loop quantum gravity is becoming increasingly accurate. This review focuses on the possible experimental or observational consequences of the underlying spinfoam structure of space-time. It adresses both the aspects associated with the Hawking evaporation and the ones due to the possible existence of a bounce. Finally, consequences for dark matter and gravitational waves are considered.


Universe ◽  
2018 ◽  
Vol 4 (10) ◽  
pp. 102 ◽  
Author(s):  
Aurélien Barrau ◽  
Killian Martineau ◽  
Flora Moulin

The understanding of black holes in loop quantum gravity is becoming increasingly accurate. This review focuses on the possible experimental or observational consequences of the underlying spinfoam structure of space-time. It addresses both the aspects associated with the Hawking evaporation and the ones due to the possible existence of a bounce. Finally, consequences for dark matter and gravitational waves are considered.


1999 ◽  
Vol 190 ◽  
pp. 313-319
Author(s):  
J. P. Beaulieu ◽  
H.J.G.L.M. Lamers ◽  
W.J. de Wit

We present a status report of the original EROS and the on-going EROS-2 microlensing surveys, which were created to search for dark matter in the Galactic halo via microlensing effects on LMC/SMC stars. Microlensing surveys provide long-term systematic observations of millions of stars in both Clouds which yield a unique database of stellar photometry and variability. We review the results obtained on pulsating stars and detail the similarities and differences of the Magellanic Cloud Herbig Ae/Be stars with their Galactic counterparts.


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