Heavy flavour production at HERA
- V. Aushev
(on behalf of the H1 and ZEUS Collaborations)
Gatchina, Russia, June 30 – July 4, 2014
1
Heavy flavour production at HERA V. Aushev (on behalf of the H1 and - - PowerPoint PPT Presentation
Heavy flavour production at HERA V. Aushev (on behalf of the H1 and ZEUS Collaborations) Gatchina, Russia, June 30 July 4, 2014 1 V. Aushev, Heavy flavour production at HERA 2 V. Aushev, Heavy flavour production at HERA 3 Deep
1
2
3
4
5
ZEUS Collaboration DESY–14–083, arXiv:1405.6915 May 2014
6
7
8
Contents of the negative bins of the significance distribution, N(S-), were subtracted from the contents of the corresponding positive bins, N(S+), yielding a subtracted decay length significance distribution: contribution from light-flavour quarks is minimized. To reduce the contamination of tracks originating from the primary vertex: |S| > 4 .
T
9
10
11
12
bb measurement as a function of Q2 for fixed x
13
bb at HERA.
14
15
16
17
18
19
20
21
22
well described by FFNS NLO; data are more precise than theory; more advanced theory is really needed !
23
24
25
+, D*+, Λc)
+,
26
∗ ∗ ∗± photoproduction has been measured for the
+, D*+, Λc : fragmentation fractions of
27