Missing energy and cosmic expansion

Nature ◽  
1996 ◽  
Vol 382 (6594) ◽  
pp. 768-768 ◽  
Author(s):  
Paul J. Steinhardt
2019 ◽  
Vol 2019 (10) ◽  
Author(s):  
Doojin Kim ◽  
Konstantin T. Matchev ◽  
Prasanth Shyamsundar

1998 ◽  
Vol 631 ◽  
pp. 593-596 ◽  
Author(s):  
J.J. van Leeuwe ◽  
H.P. Blok ◽  
J.F.J. van den Brand ◽  
H.J. Bulten ◽  
G.E. Dodge ◽  
...  
Keyword(s):  

1998 ◽  
Vol 420 (1-2) ◽  
pp. 127-139 ◽  
Author(s):  
R Barate ◽  
D Buskulic ◽  
D Decamp ◽  
P Ghez ◽  
C Goy ◽  
...  

2020 ◽  
Vol 2020 (8) ◽  
Author(s):  
Luc Darmé ◽  
Marco Fedele ◽  
Kamila Kowalska ◽  
Enrico Maria Sessolo

Abstract We investigate solutions to the flavour anomalies in B decays based on loop diagrams of a “split” dark sector characterised by the simultaneous presence of heavy particles at the TeV scale and light particles around and below the B-meson mass scale. We show that viable parameter space exists for solutions based on penguin diagrams with a vector mediator, while minimal constructions relying on box diagrams are in strong tension with the constraints from the LHC, LEP, and the anomalous magnetic moment of the muon. In particular, we highlight a regime where the mediator lies close to the B-meson mass, naturally realising a resonance structure and a q2-dependent effective coupling. We perform a full fit to the relevant flavour observables and analyse the constraints from intensity frontier experiments. Besides new measurements of the anomalous magnetic moment of the muon, we find that decays of the B meson, Bs-mixing, missing energy searches at Belle-II, and LHC searches for top/bottom partners can robustly test these scenarios in the near future.


2011 ◽  
Vol 28 (12) ◽  
pp. 125006 ◽  
Author(s):  
Rudinei C de Souza ◽  
Gilberto M Kremer

Solar Physics ◽  
1981 ◽  
Vol 73 (1) ◽  
Author(s):  
Tadashi Hirayama ◽  
Tomizo Okamoto

2018 ◽  
Vol 33 (40) ◽  
pp. 1850240
Author(s):  
Babur M. Mirza

We present here a general relativistic mechanism for accelerated cosmic expansion and the Hubble’s parameter. It is shown that spacetime vorticity coupled to the magnetic field density in galaxies causes the galaxies to recede from one another at a rate equal to the Hubble’s constant. We therefore predict an oscillatory universe, with zero curvature, without assuming violation of Newtonian gravity at large distances or invoking dark energy/dark matter hypotheses. The value of the Hubble’s constant, along with the scale of expansion, as well as the high isotropy of CMB radiation are deduced from the model.


2018 ◽  
Vol 98 (5) ◽  
Author(s):  
Mohammad Abdullah ◽  
Julián Calle ◽  
Bhaskar Dutta ◽  
Andrés Flórez ◽  
Diego Restrepo
Keyword(s):  

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