Experiment 11: NUCLEAR MAGNETIC RESONANCE SPECTROSCOPY
• By splitting pattern, we are referring to whether a signal is showing up as a singlet, doublet, triplet, quadruplet, quintuplet or multiplet • The splitting pattern (or multiplicity) reflects the number of protons on the adjacent atom The number of peaks equals the number of protons on the adjacent atom plus one This is commonly
Multiplet Guide and Workbook
Doublet of Doublets Description: A doublet of doublets (dd) is a pattern of up four lines that results from coupling to two protons (or other spin 1/2 nuclei) The lines are of all equal intensities (or close to equal intensities)
[5em] Triplet-Quadruplet Fermionic Dark Matter
Singlet-doublet DM model [Mahbubani & Senatore, hep-ph/0510064; D’Eramo, 0705 4493; Cohen et al , 1109 2604] Doublet-triplet DM model [Dedes & Karamitros, 1403 7744] Zhao-Huan Yu (Melbourne) Triplet-Quadruplet Fermionic Dark Matter December 2016 4 / 28
The all-Photochemical Synthesis an OGP (10-14) Precursor
Hertz (multiplicity: s = singulet, d = doublet, dd = double doublet, t = triplet, dt = double tiplet, q = quadruplet, quint = quintuplet, sext = sextuplet, sept = septuplet, m = multiplet) IR spectra were recorded with a Fourier transform Mattson 5000 FTIR spectrometer, neat, in CHCl3 (NaCl cell) or in KBr; absorption bands are in cm –1 UV
Scale Photoredox Additive-Free Minisci Reaction Development
downfield from TMS as an internal standard The letters s, d, t, q, and m are used to indicate singlet, doublet, triplet, quadruplet, and multiplet, respectively 1H NMR strength assays were measured using > 99 w/w tetra-chloronitrobenzene as standard Reaction monitoring was performed using
Continuous Flow Synthesis of Terminal Epoxides from Ketones
downfield from TMS as internal standard The letters s, d, t, q, and m are used to indicate singlet, doublet, triplet, quadruplet, and multiplet, respectively GC-FID analysis was performed on a ThermoFisher Focus GC with a flame ionization detector, using a TR-5MS column (30 m × 0 25 mm ID × 0 25 μm) and helium
Triplet-quadruplet fermionic dark matter
Doublet-triplet DM model [Dedes & Karamitros, 1403 7744] Zhao-Huan Yu Triplet-quadruplet fermionic dark matter Oct 2015 4 / 23 Introduction Model details Mass corrections Constraints Conclusion
[PDF] protons equivalents exemple
[PDF] regle n+1 uplet
[PDF] developpement construit
[PDF] influence des conditions du milieu sur la reproduction du hibou moyen duc
[PDF] hopital jacques monod le havre
[PDF] ghh
[PDF] organigramme de l'oréal
[PDF] document de référence l'oréal 2013
[PDF] document de référence l'oréal 2016
[PDF] rapport annuel l'oréal 2016
[PDF] document de référence l'oréal 2014
[PDF] présentation de l'oréal
[PDF] bilan social l'oréal 2014
[PDF] rapport annuel l'oréal 2014
dark matter halo stellar disk gasM33
25.8%Ω
ch2=0.11860.00204.8%Ω bh2=0.022260.00023 69.3%Ω =0.6920.012 hannvi h2≃31027cm3s1 hannvi Ωh2≃0.1 hannvi ≃31026cm3s1SU(2)L g≃0.64 mO(TeV)
hannvi g4162m2O(1026)cm3s1
hannvi h2≃31027cm3s1 hannvi Ωh2≃0.1 hannvi ≃31026cm3s1SU(2)L g≃0.64 mO(TeV)
hannvi g4162m2O(1026)cm3s1
˜0 1B(1)W3(1) (1)
SU(2)L
Z2 ˜0 1B(1)W3(1) (1)
SU(2)L
Z2 T=0 @T T 0 T 1 A :(3,0),Q1=0 B B@Q 1 Q0 1 Q 1 Q 11 C 4,1 2 ,Q2=0 B B@Q 2 Q+ 2 Q0 2 Q 21C 4,+1 2 L
T=iT†¯DT1
2 m TTT+h.c.)
LQ=iQ†
1¯DQ1+iQ†
2¯DQ2(
m Q Q1Q2+h.c.)
LHTQ= y 1 jl(Q1)jk iTi kHl y 2 (Q2)jk iTi kH† j+h.c. Z 2 ) TLHTecH†H†Q1L†HH†Q2LHH†Lmass=mQQ
1Q++212(T0,Q0
1,Q0 2)MN0 @T 0 Q 0 1 Q0 21A (T,Q 1,Q 2)MC0 @T Q 1 Q+ 21
A +h.c. =mQ++1 2 3 i=1m0i0 i0 i3∑ i=1m i i+ i+h.c. M N=0 B B@m T1 p 3 y1v1 p 3 y2v 1 p 3 y1v0mQ 1 p 3 y2v mQ01 C CA, M C=0 B B@m T1 p 2 y1v1 p 6 y2v 1 p 6 y1v0mQ 1 p 2 y2vmQ01 C CA 0 @T 0 Q 0 1 Q0 21
A N 0 0 1 0 2 0 31
A ,0 @T Q 1 Q+ 21
A C L 0 1 2 31
A ,0 @T Q 1 Q 21
A C R 0 1 2 31
A Q
1,++Q++
2 0 1 y1=y2 SU(2)R y=y1=y2 SU(2)LSU(2)R
LQ+LHTQ=i(Q†A)k
ij¯D(QA)ij k1 2 [mQϵABϵil(QA)ij k(QB)lk j+h.c.] +[yϵAB(QA)jk iTi k(HB)j+h.c.]SU(2)R(QA)ij
k=0 (Q1)ij k (Q2)ij k1 A ,(HA)i=0H†
i H i1 A U(1)Y y1=y2 SU(2)R Mass (GeV)
yLO, mQ = 200 GeV, mT = 400 GeV, y = y1 = y2
150200
250
300
350
400
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500
-1.0-0.50.00.51.0 mc0
1 = mc±
1 = mc±±
mc02 = mc±
2 mc03 = mc±
3Mass (GeV)
yLO, mQ = 400 GeV, mT = 200 GeV, y = y1 = y2
150200
250
300
350
400
450
500
-1.0-0.50.00.51.0 mc0
1 = mc±
1 mc02 = mc±
2 = mc±±
mc03 = mc±
3 m QT = 400 GeV
mQ = 400 GeV mT = 200 GeV
gZ c0 1 c0 1 y2 / y1y 1 = 1 -0.20 -0.15 -0.10 -0.05 0.00 0.05 0.10 -2.0-1.5-1.0-0.50.00.51.01.52.0 mQ = 200 GeV mT = 400 GeV
mQ = 400 GeV mT = 200 GeV
h0 10 1 Z0 101 m
Q 0 1= (Q0
1+Q0 2)=p2 0 1 hZ 0 1 m0 i≃m i Mass (GeV) y2LO, m Q = 200 GeV, mT = 400 GeV, y1 = 1
0 100
200
300
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600
-2.0-1.5-1.0-0.50.00.51.01.52.0 mc±± mc0 1 mc± 1 mc0 2 mc± 2 mc0 3 mc± 3 Mass (GeV)
y2LO, m Q = 400 GeV, mT = 200 GeV, y1 = 1
0 100
200
300
400
500
600
-2.0-1.5-1.0-0.50.00.51.01.52.0quotesdbs_dbs16.pdfusesText_22
1= (Q0
1+Q0 2)=p2 0 1 hZ 0 1 m0 i≃m i Mass (GeV) y2LO, mQ = 200 GeV, mT = 400 GeV, y1 = 1
0 100200
300
400
500
600
-2.0-1.5-1.0-0.50.00.51.01.52.0 mc±± mc0 1 mc± 1 mc0 2 mc± 2 mc0 3 mc± 3
Mass (GeV)
y2LO, mQ = 400 GeV, mT = 200 GeV, y1 = 1
0 100200
300
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600
-2.0-1.5-1.0-0.50.00.51.01.52.0quotesdbs_dbs16.pdfusesText_22