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D. Bemmerer | Researchclopedia

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D. Bemmerer

Helmholtz-Zentrum Dresden-Rossendorf ORCID

272

Works

6,085

Citations

42

h-index

105

i10-index

Research Topics

Nuclear physics research studies Nuclear Physics and Applications Radiation Detection and Scintillator Technologies

Affiliations

TRIUMF2008–2008

Istituto Nazionale di Fisica Nucleare2010–2010

GSI Helmholtz Centre for Heavy Ion Research2011–2011

Duke University2010–2010

HUN-REN Institute for Nuclear Research2015–2015

Top Works

Solar fusion cross sections. II. The<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi>p</mml:mi></mml:math>chain and CNO cycles

E. G. Adelberger,A. Garcı́a,et al.

2011766 citations

Neutrino Physics Research

Astronomical and nuclear sciences

Astrophysical S-factor of 14N(p,γ)15O

A. Formicola,G. Imbriani,et al.

2004331 citations

S-factor of 14N(p,γ)15O at astrophysical energies⋆

G. Imbriani,H. Costantini,et al.

2005246 citations

The baryon density of the Universe from an improved rate of deuterium burning

V. Mossa,K. Stöckel,et al.

2020191 citations

The LUNA II 400 accelerator

A. Formicola,G. Imbriani,et al.

2003190 citations

Activation Measurement of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>He</mml:mi><mml:mprescripts/><mml:none/><mml:mn>3</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mi>Be</mml:mi><mml:mprescripts/><mml:none/><mml:mn>7</mml:mn></mml:mmultiscripts></mml:math>Cross Section at Low Energy

D. Bemmerer,F. Confortola,et al.

2006150 citations

Astrophysical<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>S</mml:mi></mml:mrow></mml:math>factor of the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">He</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>3</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>α</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>)<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">Be</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>7</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>reaction measured at low energy via detection of prompt and delayed γ rays

F. Confortola,D. Bemmerer,et al.

2007138 citations

The bottleneck of CNO burning and the age of Globular Clusters

G. Imbriani,H. Costantini,et al.

2004132 citations

First measurement of the 14N(<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.gif" overflow="scroll"><mml:mi mathvariant="normal">p</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:math>)15O cross section down to 70 keV

A. Lemut,D. Bemmerer,et al.

2006122 citations