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RPT Kimia T4 2013 100%

YEARLY TEACHING PLAN CHEMISTRY FORM 4 / 2013 1 Pn.

https://www.pdf-archive.com/2013/09/04/rpt-kimia-t4-2013/

04/09/2013 www.pdf-archive.com

Rios 93%

Green’s functions for dense matter &

https://www.pdf-archive.com/2017/10/11/rios/

11/10/2017 www.pdf-archive.com

GammaSpectr revised Diehl 72%

1 UV X-rays γ-rays (space) 2 6 γ-rays (ground) 10 14 [log E, eV] 8 12 16 20 24 28 [log n, Hz] 0 -4 -8 -12 -16 -20 [log l, m] electrons (mag.field) molecules, dust atomic nuclei atoms electromagnetic electrons+-, nucleons, pions, IC...

https://www.pdf-archive.com/2014/02/11/gammaspectr-revised-diehl/

11/02/2014 www.pdf-archive.com

Bira vK 66%

0) 2 4   scattering length unitarity limit ( a2−1 ≈ mB2 → 0 −1 2 T2 a −1 R  mπ a2,=I 1 S0 shape parameter r2 P  R, 2  R 3 ,  typically 2 4  1  4π −1  = kR ( ik ) 1 +   , kR   m  ka2   −1 ) unitarity window nucleons effective range a2,=I a2,=I 1,= I3 0 mπ 1,= I3 +1mπ 1,= I3 −1mπ no parameter!

https://www.pdf-archive.com/2017/10/11/bira-vk/

11/10/2017 www.pdf-archive.com

PPapakon 66%

A natural EDF Ansatz for homogeneous nuclear matter:

https://www.pdf-archive.com/2017/10/11/ppapakon/

11/10/2017 www.pdf-archive.com

Cosmic inflation and hidden thermodynamics 57%

Below this threshold (which matches the formation of nucleons, then atoms), the quantity of information is then sufficient for the principle of least action to apply.

https://www.pdf-archive.com/2016/10/12/cosmic-inflation-and-hidden-thermodynamics/

12/10/2016 www.pdf-archive.com

JDIT-2016-0618-021 32%

A quadrupolar nucleus has an asymmetric distribution of nucleons, producing a non-spherical positive charge distribution.

https://www.pdf-archive.com/2017/05/30/jdit-2016-0618-021/

29/05/2017 www.pdf-archive.com