Fetching the paper…

Reading the bibliography…

2007

Why we need to see the dark matter to understand the dark energy

Kunz, Martin

Original
PDF
Post on X

Understand

The cosmological concordance model contains two separate constituents which interact only gravitationally with themselves and everything else, the dark matter and the dark energy.

In the standard dark energy models, the dark matter makes up some 20% of the total energy budget today, while the dark energy is responsible for about 75%.
Here we show that these numbers are only robust for specific dark energy models and that in general we cannot measure the abundance of the dark constituents separately without making strong assumptions.

Why we need to see the dark matter to understand the dark energy · Around

Built on

Zwicky F 1933 Helv. Phys. Acta
1933
Earlier work this paper cites.
Kodama H and Sasaki M 1984 Progr. Theor. Phys. Suppl
1995
Earlier work this paper cites.
Riess A et al 1998 Astron. J
1999
Earlier work this paper cites.
Wasserman I Phys.Rev
2002
Earlier work this paper cites.

Similar

Hu W 2004 lecture notes
2004
Cited alongside, same era.
Corasaniti P S et al 2004 Phys. Rev
2004
Cited alongside, same era.
Kunz M and Sapone D 2006 Phys. Rev
2006
Cited alongside, same era.

Then

Astier P et al 2006 Astron. Astrophys
Original
2006
Later among the works it cites.
Kunz M 2007 Preprint
2007
Closest in time.
Spergel D N et al. 2007 Astrophys. J. Suppl
2007
Closest in time.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…