Published December 2006 | Version v1
Journal article Metadata-only

Dark matter annihilation in the Galaxy

Creators

  • 1. Inst. for Nuclear Reseaerch, RAS, Moscow (Russian Federation)
  • 2. INFN, Lab. Nazionali del Gran Sasso, Assegri (AQ) (Italy)
  • 3. Inst. for Nuclear Research, RAS, Moscow (Russian Federation)

Description

The awaited Dark Matter (DM) neutralino annihilation signal from the Galactic halo crucially depends on the presence of small-scale clumps. A mass function of the DM small-scale clumps is calculated in the standard cosmological scenario. The final distribution of clumps in the Galaxy is influenced by their tidal destruction. The basic sources of clump destruction are considered

Abstract (Russian)

Ожидаемый сигнал, обусловленный аннигиляцией нейтралино темной материи (ТМ), зависит от присутствия маломасштабных сгустков (clumps). Рассчитывается массовая функция этих сгустков. Конечное распределение сгустков в Галактике определяется их приливным разрушением. Рассматриваются основные источники такого разрушения сгустков

Additional details

Additional titles

Augmented title (English)
neutralinos

Publishing Information

Journal Title
Yadernaya Fizika
Journal Volume
69
Journal Issue
12
Journal Page Range
p. 2113-2122
ISSN
0044-0027
CODEN
IDFZA7

Conference

Title
5. International conference on nonaccelerator new physics (NANP-2005)
Dates
20-25 Jun 2005
Place
Dubna (Russian Federation)

INIS

Country of Publication
Russian Federation
Country of Input or Organization
Russian Federation
INIS RN
39021317
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ANNIHILATION; GALAXIES; MASS DISTRIBUTION; NEUTRAL PARTICLES; NONLUMINOUS MATTER; NUMERICAL SOLUTION
Descriptors DEC
DISTRIBUTION; INTERACTIONS; MATHEMATICAL SOLUTIONS; MATTER; PARTICLE INTERACTIONS; SPATIAL DISTRIBUTION

Optional Information

Notes
36 refs., 6 figs.