These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.


BIOMARKERS

Molecular Biopsy of Human Tumors

- a resource for Precision Medicine *

188 related articles for article (PubMed ID: 23006073)

  • 1. Quantum stability of chameleon field theories.
    Upadhye A; Hu W; Khoury J
    Phys Rev Lett; 2012 Jul; 109(4):041301. PubMed ID: 23006073
    [TBL] [Abstract][Full Text] [Related]  

  • 2. Catastrophic consequences of kicking the chameleon.
    Erickcek AL; Barnaby N; Burrage C; Huang Z
    Phys Rev Lett; 2013 Apr; 110(17):171101. PubMed ID: 23679701
    [TBL] [Abstract][Full Text] [Related]  

  • 3. ASTROPHYSICS. Atom-interferometry constraints on dark energy.
    Hamilton P; Jaffe M; Haslinger P; Simmons Q; Müller H; Khoury J
    Science; 2015 Aug; 349(6250):849-51. PubMed ID: 26293958
    [TBL] [Abstract][Full Text] [Related]  

  • 4. No-go theorems for generalized chameleon field theories.
    Wang J; Hui L; Khoury J
    Phys Rev Lett; 2012 Dec; 109(24):241301. PubMed ID: 23368302
    [TBL] [Abstract][Full Text] [Related]  

  • 5. Compatibility of the chameleon-field model with fifth-force experiments, cosmology, and PVLAS and CAST results.
    Brax P; van de Bruck C; Davis AC
    Phys Rev Lett; 2007 Sep; 99(12):121103. PubMed ID: 17930493
    [TBL] [Abstract][Full Text] [Related]  

  • 6. Neutron limit on the strongly-coupled chameleon field.
    Li K; Arif M; Cory DG; Haun R; Heacock B; Huber MG; Nsofini J; Pushin DA; Saggu P; Sarenac D; Shahi CB; Skavysh V; Snow WM; Young AR;
    Phys Rev D; 2016 Mar; 93(6):. PubMed ID: 34859165
    [TBL] [Abstract][Full Text] [Related]  

  • 7. Search for chameleon scalar fields with the axion dark matter experiment.
    Rybka G; Hotz M; Rosenberg LJ; Asztalos SJ; Carosi G; Hagmann C; Kinion D; van Bibber K; Hoskins J; Martin C; Sikivie P; Tanner DB; Bradley R; Clarke J
    Phys Rev Lett; 2010 Jul; 105(5):051801. PubMed ID: 20867906
    [TBL] [Abstract][Full Text] [Related]  

  • 8. Screening long-range forces through local symmetry restoration.
    Hinterbichler K; Khoury J
    Phys Rev Lett; 2010 Jun; 104(23):231301. PubMed ID: 20867225
    [TBL] [Abstract][Full Text] [Related]  

  • 9. Detecting chameleon dark energy via an electrostatic analogy.
    Jones-Smith K; Ferrer F
    Phys Rev Lett; 2012 Jun; 108(22):221101. PubMed ID: 23003583
    [TBL] [Abstract][Full Text] [Related]  

  • 10. Searching for Chameleon Dark Energy with Mechanical Systems.
    Betz J; Manley J; Wright EM; Grin D; Singh S
    Phys Rev Lett; 2022 Sep; 129(13):131302. PubMed ID: 36206421
    [TBL] [Abstract][Full Text] [Related]  

  • 11. Experiment to Detect Dark Energy Forces Using Atom Interferometry.
    Sabulsky DO; Dutta I; Hinds EA; Elder B; Burrage C; Copeland EJ
    Phys Rev Lett; 2019 Aug; 123(6):061102. PubMed ID: 31491160
    [TBL] [Abstract][Full Text] [Related]  

  • 12. Connection between a possible fifth force and the direct detection of dark matter.
    Bovy J; Farrar GR
    Phys Rev Lett; 2009 Mar; 102(10):101301. PubMed ID: 19392100
    [TBL] [Abstract][Full Text] [Related]  

  • 13. 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; 105(26):261803. PubMed ID: 21231645
    [TBL] [Abstract][Full Text] [Related]  

  • 14. Symmetron dark energy in laboratory experiments.
    Upadhye A
    Phys Rev Lett; 2013 Jan; 110(3):031301. PubMed ID: 23373910
    [TBL] [Abstract][Full Text] [Related]  

  • 15. Strongly coupled chameleons and the neutronic quantum bouncer.
    Brax P; Pignol G
    Phys Rev Lett; 2011 Sep; 107(11):111301. PubMed ID: 22026655
    [TBL] [Abstract][Full Text] [Related]  

  • 16. Strongly coupled chameleon fields: new horizons in scalar field theory.
    Mota DF; Shaw DJ
    Phys Rev Lett; 2006 Oct; 97(15):151102. PubMed ID: 17155313
    [TBL] [Abstract][Full Text] [Related]  

  • 17. Quantum gravitational contributions to the cosmic microwave background anisotropy spectrum.
    Kiefer C; Krämer M
    Phys Rev Lett; 2012 Jan; 108(2):021301. PubMed ID: 22324668
    [TBL] [Abstract][Full Text] [Related]  

  • 18. Tests of chameleon gravity.
    Burrage C; Sakstein J
    Living Rev Relativ; 2018; 21(1):1. PubMed ID: 29576739
    [TBL] [Abstract][Full Text] [Related]  

  • 19. 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; 112(15):151105. PubMed ID: 24785025
    [TBL] [Abstract][Full Text] [Related]  

  • 20. Dark Energy after GW170817 and GRB170817A.
    Creminelli P; Vernizzi F
    Phys Rev Lett; 2017 Dec; 119(25):251302. PubMed ID: 29303308
    [TBL] [Abstract][Full Text] [Related]  

    [Next]    [New Search]
    of 10.