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Some remarks about UHECR origin and interaction

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Title: Some remarks about UHECR origin and interaction


1
Some remarks about UHECR origin and
interaction
A.A.Petrukhin Moscow Engineering Physics
Institute CRIS 2006
Contents
1. Two approaches to the problem 2. Generation
of CR in plasma pinches 3. Unusual events in
UHECR 4. New physics in cosmic rays 5.
CR energy spectrum description 6. Conclusions
2
Introduction
  • UHECR problems begin from VHECR problems (in the
    first turn from the knee).
  • Experimentally the knee is observed as the change
    of the slope in EAS energy spectrum in the
    atmosphere.
  • But EAS is a secondary phenomenon and its energy
    can differ from the energy of primary particle.
  • Therefore in principle two approaches are
    possible.

3
1. The knee exists in primary CR
  • In favour of this approach two basic
    arguments were usually given
  • Sources and processes of CR generation without
    the knee were unknown (the knee energy is a
    limiting energy of galactic cosmic rays).
  • There were no experimental evidences in
    accelerator physics for inclusion of new physical
    processes with relatively large cross-section,
    which is necessary for the knee formation due to
    interaction processes.

4
2. The knee appears at interactions of primary
CR in the atmosphere
  • In favour of this approach, three basic
    arguments can be given
  • Model of CR generation in plasma pinches, which
    predicts infinite energy spectrum with a single
    slope .
  • Many experimental observations of unusual events
    and phenomena above the knee.
  • New experimental and theoretical results on QGP
    behavior at the energy increase (growth of yield
    of heavy particles, large orbital momentum at
    non-central collisions, etc.).

5
CR generation in plasma pinches(B.A.Trubnikov
et al.)
This model was considered at previous CRIS 2004
and has been published in its Proceedings Nucl.
Phys. B (Proc. Suppl.) 136 (2004) 218-223 where
the references to the original papers of authors
(B.A.Trubnikov V.P.Vlasov, S.K.Zhdanov ) are
given. Therefore I mention the main ideas and
results only.
6
CR generation in plasma pinches
In cosmic plasma (of any origin) electrical
discharges "cosmic lightnings" can occur, at
which cylindrical pinches are formed.
Plasma jets are squeezed out of pinch neck. These
jets are accelerated particle beams.

7
CR generation in plasma pinches
Energy distribution of particles in jets has
the form
which does not depend on pinch sizes, currents in
pinches and other parameters, which determine a
proportionality coefficient only. Model
has no limitation for accelerated particle energy
since in plasma pinch neck
density ? ? ?, when its radius r ? 0.
8
Other interesting consequences
  • The composition of accelerated particles will be
    the same as composition of cosmic plasma, which
    consists mainly of hydrogen.
  • Model explains the absence of point sources of
    cosmic rays since pinches, f.e. near Supernova,
    can be oriented in any direction.
  • At the same time, generation of particles in
    narrow jets in cylindrical pinches can explain
    the appearance of correlated particles.
  • In comparison with other models, which work
    during SN explosions only, this mechanism works
    permanently, therefore it has to be considered as
    main source of CR.

9
List of unusual events
  • In hadron experiments

halos, alignment, penetrating cascades, Centauros
(Pamir-Chacaltaya)
?
?
long-flying component, Anti-Centauros (Tien-Shan).
  • In muon experiments

excess of VHE ( 100 TeV) single (MSU) and
multiple (LVD) muons
?
observation of VHE muons (Japan, NUSEX), the
probability to detect which is very small.
?
  • In EAS investigations

change of EAS energy spectrum in the atmosphere,
which is explained now as a change of primary
energy spectrum.
?
changes of behavior of N?(Ne) and Xmax(Ne)
dependences, which are explained now as the
heaving of CR composition.
?
It is important All these events appear at PeV
energies of primary particles.
10
Alignment
11
Penetrating cascade
12
Muon flux excess
13
Muon bundles excess
14
The knee in EAS energy spectrum
15
Missing energy determination
16
(No Transcript)
17
Mean ltln Agt obtained from Nm/Ne ratio
18
Xmax
19
What we need to explain these data?
Model of hadron interactions which gives
  • Threshold behaviour (unusual events appear at
  • several PeV only).
  • 2. Large cross section (to change EAS spectrum
    slope).
  • 3. Large yield of leptons (excess of VHE muons
    and missing energy).
  • 4. Large orbital (or rotational) momentum
    (alignment).
  • 5. Violation of isotopic invariance (Centauros
    and Anti- Centauros) .
  • Two possible models are suitable for that.

20
New massive short-lived particles(as usual
resonance states)
Pluses 1. According to Chew-Frautschi
diagram, spin J depends on mass M as J 0.9 M 2,
where M is in Gev. For M 1
TeV, spin J will be 106 (!) 2. This very
large value of J can explain - a long
life-time of new resonance state, which is
necessary for decays into weakly interacting W,
Z-bosons - experimental results on alignment
observations.
Minus 1. Small cross-section of such
particle production
21
Chew-Frautschi diagram
22
Quark-gluon plasma(better, Quark-gluon matter)
gives
  • Threshold behavior, since high temperature and
    density are required.
  • 2. Large cross section, since transition from
    quark-quark interaction to some collective
    interaction of many quarks gives
    .
  • 3. As was shown by Zuo-Tang Liang and Xin-Nian
    Vang in non-central collisions a globally
    polarized QGP with large orbital angular
    momentum must appear.
  • Centrifugal barrier
    will be less for heavy particles (quarks and
    W, Z-bosons), which are necessary to explain
    leptons production.

23
Potential barrier for different masses
24
Some remarks about composition
1. At present, information about the composition
is
extracted from results of EAS investigations,
namely from data on the number of muons N?
and Xmax elongation rate, taking into
account results of simulations. 2. If new
state of matter with mass 1 TeV is
generated, the number of secondary particles will
be increased due to decays of W, Z-bosons
into hadrons (on average 20 in each). 3.
This leads to a more quick development of shower
(decreasing of Xmax) and to increasing N?.
4. Taking into account a missing energy, instead
of proton shower with energy E0, "iron"
shower with lower energy will be observed.
25
How to explain the ankle appearance?
  • With increasing of interaction energy, mass and
    energy of excitation of resonance state can be so
    large that it begins to decay into hadrons
    immediately.
  • Average missing energy and number of muons will
    be decreased and the development of EAS will
    return to a normal behavior.

26
Region of missing energy
27
Cut-off influence existing approach
28
Cut-off influence new approach
29
Two versions of cut-off influence
?
30
Conclusions
  • Consideration of UHECR spectrum and interaction
    shows that there is a very close interconnection
    between them.
  • New model of CR acceleration in plasma pinches
    and a possibility of generation of quark-gluon
    plasma resonances with large angular momentum
    allow to formulate a new approach to UHECR
    description.
  • This approach shows that it is impossible to
    solve problems of UHECR (especially of
    GZK-cutoff) without the solution of the knee
    problem.

31
Addendum-1
  • To obtain unambiguous solution of VHE, UHE, and
    EHE CR problems it is necessary to investigate
    them at one array by unified methods beginning
    from 1 PeV or lower.
  • 2. The array must include various detectors
    for measurements of all EAS component
    characteristics and especially muon energy in the
    range more than 10 TeV.
  • In fact, it is necessary to construct the united
    world-wide cosmophysical array like LHC in
    accelerator physics.
  • In opposite case we will discuss problems of the
    knee, the ankle and cutoff 50 years more (in
    2008, it will be 50 years from the knee
    discovery).

32
Addendum-2
  • 5. Apparently the best country for deployment
    of this united array is USA. In this case even
    some equilibrium appears
  • - in Europe the biggest accelerator,
  • - in USA the biggest cosmophysical
    observatory.
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