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Items: 1 to 20 of 131

1.

Gravity resonance spectroscopy constrains dark energy and dark matter scenarios.

Jenke T, Cronenberg G, Burgdörfer J, Chizhova LA, Geltenbort P, Ivanov AN, Lauer T, Lins T, Rotter S, Saul H, Schmidt U, Abele H.

Phys Rev Lett. 2014 Apr 18;112(15):151105. Epub 2014 Apr 16.

PMID:
24785025
2.

Ultracold neutron detectors based on 10B converters used in the qBounce experiments.

Jenke T, Cronenberg G, Filter H, Geltenbort P, Klein M, Lauer T, Mitsch K, Saul H, Seiler D, Stadler D, Thalhammer M, Abele H.

Nucl Instrum Methods Phys Res A. 2013 Dec 21;732:1-8.

3.

Search for Screened Interactions Associated with Dark Energy below the 100 μm Length Scale.

Rider AD, Moore DC, Blakemore CP, Louis M, Lu M, Gratta G.

Phys Rev Lett. 2016 Sep 2;117(10):101101. doi: 10.1103/PhysRevLett.117.101101. Epub 2016 Aug 29.

PMID:
27636465
4.

Laboratory constraints on chameleon dark energy and power-law fields.

Steffen JH, Upadhye A, Baumbaugh A, Chou AS, Mazur PO, Tomlin R, Weltman A, Wester W.

Phys Rev Lett. 2010 Dec 31;105(26):261803. Epub 2010 Dec 28.

PMID:
21231645
5.

Model selection for modified gravity.

Kitching TD, Simpson F, Heavens AF, Taylor AN.

Philos Trans A Math Phys Eng Sci. 2011 Dec 28;369(1957):5090-101. doi: 10.1098/rsta.2011.0287.

6.

Symmetron dark energy in laboratory experiments.

Upadhye A.

Phys Rev Lett. 2013 Jan 18;110(3):031301. Epub 2013 Jan 18.

PMID:
23373910
7.

ASTROPHYSICS. Atom-interferometry constraints on dark energy.

Hamilton P, Jaffe M, Haslinger P, Simmons Q, Müller H, Khoury J.

Science. 2015 Aug 21;349(6250):849-51. doi: 10.1126/science.aaa8883.

8.

Planckian Interacting Massive Particles as Dark Matter.

Garny M, Sandora M, Sloth MS.

Phys Rev Lett. 2016 Mar 11;116(10):101302. doi: 10.1103/PhysRevLett.116.101302. Epub 2016 Mar 10.

PMID:
27015472
9.

Phantom energy mediates a long-range repulsive force.

Amendola L.

Phys Rev Lett. 2004 Oct 29;93(18):181102. Epub 2004 Oct 29.

PMID:
15525149
10.

Strongly coupled chameleons and the neutronic quantum bouncer.

Brax P, Pignol G.

Phys Rev Lett. 2011 Sep 9;107(11):111301. Epub 2011 Sep 8.

PMID:
22026655
11.
12.

Einstein's theory of gravity and the problem of missing mass.

Ferreira PG, Starkman GD.

Science. 2009 Nov 6;326(5954):812-5. doi: 10.1126/science.1172245. Erratum in: Science. 2009 Dec 11;326(5959):1482.

PMID:
19892973
13.

Quantum stability of chameleon field theories.

Upadhye A, Hu W, Khoury J.

Phys Rev Lett. 2012 Jul 27;109(4):041301. Epub 2012 Jul 23.

PMID:
23006073
14.

Chameleon fields: awaiting surprises for tests of gravity in space.

Khoury J, Weltman A.

Phys Rev Lett. 2004 Oct 22;93(17):171104. Epub 2004 Oct 22.

PMID:
15525066
15.

Catastrophic consequences of kicking the chameleon.

Erickcek AL, Barnaby N, Burrage C, Huang Z.

Phys Rev Lett. 2013 Apr 26;110(17):171101. Epub 2013 Apr 23.

PMID:
23679701
16.

Precision physics of simple atoms and constraints on a light boson with ultraweak coupling.

Karshenboim SG.

Phys Rev Lett. 2010 Jun 4;104(22):220406. Epub 2010 Jun 4.

PMID:
20867154
17.

Broadband and Resonant Approaches to Axion Dark Matter Detection.

Kahn Y, Safdi BR, Thaler J.

Phys Rev Lett. 2016 Sep 30;117(14):141801. Epub 2016 Sep 30.

PMID:
27740816
18.

Tests of the gravitational inverse-square law below the dark-energy length scale.

Kapner DJ, Cook TS, Adelberger EG, Gundlach JH, Heckel BR, Hoyle CD, Swanson HE.

Phys Rev Lett. 2007 Jan 12;98(2):021101. Epub 2007 Jan 8.

PMID:
17358595
19.

Laboratory search for a long-range T-odd, P-odd interaction from axionlike particles using dual-species nuclear magnetic resonance with polarized 129Xe and 131Xe gas.

Bulatowicz M, Griffith R, Larsen M, Mirijanian J, Fu CB, Smith E, Snow WM, Yan H, Walker TG.

Phys Rev Lett. 2013 Sep 6;111(10):102001. Epub 2013 Sep 3.

PMID:
25166656
20.

Tensor interpretation of BICEP2 results severely constrains axion dark matter.

Marsh DJ, Grin D, Hlozek R, Ferreira PG.

Phys Rev Lett. 2014 Jul 4;113(1):011801. Epub 2014 Jul 2.

PMID:
25032918

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