Puzzles in astrophysics in the past and present
Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do s...
Ausführliche Beschreibung
Autor*in: |
Berezinsky, V. S. [verfasserIn] |
---|
Format: |
Artikel |
---|---|
Sprache: |
Englisch |
Erschienen: |
2003 |
---|
Schlagwörter: |
---|
Anmerkung: |
© MAIK "Nauka/Interperiodica" 2003 |
---|
Übergeordnetes Werk: |
Enthalten in: Physics of atomic nuclei - Nauka/Interperiodica, 1993, 66(2003), 3 vom: März, Seite 423-434 |
---|---|
Übergeordnetes Werk: |
volume:66 ; year:2003 ; number:3 ; month:03 ; pages:423-434 |
Links: |
---|
DOI / URN: |
10.1134/1.1563699 |
---|
Katalog-ID: |
OLC2049896212 |
---|
LEADER | 01000caa a22002652 4500 | ||
---|---|---|---|
001 | OLC2049896212 | ||
003 | DE-627 | ||
005 | 20230504110320.0 | ||
007 | tu | ||
008 | 200820s2003 xx ||||| 00| ||eng c | ||
024 | 7 | |a 10.1134/1.1563699 |2 doi | |
035 | |a (DE-627)OLC2049896212 | ||
035 | |a (DE-He213)1.1563699-p | ||
040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
041 | |a eng | ||
082 | 0 | 4 | |a 530 |q VZ |
100 | 1 | |a Berezinsky, V. S. |e verfasserin |4 aut | |
245 | 1 | 0 | |a Puzzles in astrophysics in the past and present |
264 | 1 | |c 2003 | |
336 | |a Text |b txt |2 rdacontent | ||
337 | |a ohne Hilfsmittel zu benutzen |b n |2 rdamedia | ||
338 | |a Band |b nc |2 rdacarrier | ||
500 | |a © MAIK "Nauka/Interperiodica" 2003 | ||
520 | |a Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. | ||
650 | 4 | |a Radiation | |
650 | 4 | |a Elementary Particle | |
650 | 4 | |a Gamma Radiation | |
650 | 4 | |a Critical Review | |
650 | 4 | |a Particle Physic | |
773 | 0 | 8 | |i Enthalten in |t Physics of atomic nuclei |d Nauka/Interperiodica, 1993 |g 66(2003), 3 vom: März, Seite 423-434 |w (DE-627)131188437 |w (DE-600)1146378-8 |w (DE-576)032622155 |x 1063-7788 |7 nnns |
773 | 1 | 8 | |g volume:66 |g year:2003 |g number:3 |g month:03 |g pages:423-434 |
856 | 4 | 1 | |u https://doi.org/10.1134/1.1563699 |z lizenzpflichtig |3 Volltext |
912 | |a GBV_USEFLAG_A | ||
912 | |a SYSFLAG_A | ||
912 | |a GBV_OLC | ||
912 | |a SSG-OLC-PHY | ||
912 | |a SSG-OPC-AST | ||
912 | |a GBV_ILN_40 | ||
912 | |a GBV_ILN_70 | ||
912 | |a GBV_ILN_2014 | ||
912 | |a GBV_ILN_2279 | ||
951 | |a AR | ||
952 | |d 66 |j 2003 |e 3 |c 03 |h 423-434 |
author_variant |
v s b vs vsb |
---|---|
matchkey_str |
article:10637788:2003----::uzeiatohsciteat |
hierarchy_sort_str |
2003 |
publishDate |
2003 |
allfields |
10.1134/1.1563699 doi (DE-627)OLC2049896212 (DE-He213)1.1563699-p DE-627 ger DE-627 rakwb eng 530 VZ Berezinsky, V. S. verfasserin aut Puzzles in astrophysics in the past and present 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. Radiation Elementary Particle Gamma Radiation Critical Review Particle Physic Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 423-434 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:423-434 https://doi.org/10.1134/1.1563699 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 423-434 |
spelling |
10.1134/1.1563699 doi (DE-627)OLC2049896212 (DE-He213)1.1563699-p DE-627 ger DE-627 rakwb eng 530 VZ Berezinsky, V. S. verfasserin aut Puzzles in astrophysics in the past and present 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. Radiation Elementary Particle Gamma Radiation Critical Review Particle Physic Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 423-434 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:423-434 https://doi.org/10.1134/1.1563699 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 423-434 |
allfields_unstemmed |
10.1134/1.1563699 doi (DE-627)OLC2049896212 (DE-He213)1.1563699-p DE-627 ger DE-627 rakwb eng 530 VZ Berezinsky, V. S. verfasserin aut Puzzles in astrophysics in the past and present 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. Radiation Elementary Particle Gamma Radiation Critical Review Particle Physic Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 423-434 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:423-434 https://doi.org/10.1134/1.1563699 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 423-434 |
allfieldsGer |
10.1134/1.1563699 doi (DE-627)OLC2049896212 (DE-He213)1.1563699-p DE-627 ger DE-627 rakwb eng 530 VZ Berezinsky, V. S. verfasserin aut Puzzles in astrophysics in the past and present 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. Radiation Elementary Particle Gamma Radiation Critical Review Particle Physic Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 423-434 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:423-434 https://doi.org/10.1134/1.1563699 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 423-434 |
allfieldsSound |
10.1134/1.1563699 doi (DE-627)OLC2049896212 (DE-He213)1.1563699-p DE-627 ger DE-627 rakwb eng 530 VZ Berezinsky, V. S. verfasserin aut Puzzles in astrophysics in the past and present 2003 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © MAIK "Nauka/Interperiodica" 2003 Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. Radiation Elementary Particle Gamma Radiation Critical Review Particle Physic Enthalten in Physics of atomic nuclei Nauka/Interperiodica, 1993 66(2003), 3 vom: März, Seite 423-434 (DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 1063-7788 nnns volume:66 year:2003 number:3 month:03 pages:423-434 https://doi.org/10.1134/1.1563699 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 AR 66 2003 3 03 423-434 |
language |
English |
source |
Enthalten in Physics of atomic nuclei 66(2003), 3 vom: März, Seite 423-434 volume:66 year:2003 number:3 month:03 pages:423-434 |
sourceStr |
Enthalten in Physics of atomic nuclei 66(2003), 3 vom: März, Seite 423-434 volume:66 year:2003 number:3 month:03 pages:423-434 |
format_phy_str_mv |
Article |
institution |
findex.gbv.de |
topic_facet |
Radiation Elementary Particle Gamma Radiation Critical Review Particle Physic |
dewey-raw |
530 |
isfreeaccess_bool |
false |
container_title |
Physics of atomic nuclei |
authorswithroles_txt_mv |
Berezinsky, V. S. @@aut@@ |
publishDateDaySort_date |
2003-03-01T00:00:00Z |
hierarchy_top_id |
131188437 |
dewey-sort |
3530 |
id |
OLC2049896212 |
language_de |
englisch |
fullrecord |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2049896212</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504110320.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2003 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1134/1.1563699</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2049896212</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)1.1563699-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Berezinsky, V. S.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Puzzles in astrophysics in the past and present</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2003</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© MAIK "Nauka/Interperiodica" 2003</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radiation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Elementary Particle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Gamma Radiation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Critical Review</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Particle Physic</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Physics of atomic nuclei</subfield><subfield code="d">Nauka/Interperiodica, 1993</subfield><subfield code="g">66(2003), 3 vom: März, Seite 423-434</subfield><subfield code="w">(DE-627)131188437</subfield><subfield code="w">(DE-600)1146378-8</subfield><subfield code="w">(DE-576)032622155</subfield><subfield code="x">1063-7788</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:66</subfield><subfield code="g">year:2003</subfield><subfield code="g">number:3</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:423-434</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1134/1.1563699</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">66</subfield><subfield code="j">2003</subfield><subfield code="e">3</subfield><subfield code="c">03</subfield><subfield code="h">423-434</subfield></datafield></record></collection>
|
author |
Berezinsky, V. S. |
spellingShingle |
Berezinsky, V. S. ddc 530 misc Radiation misc Elementary Particle misc Gamma Radiation misc Critical Review misc Particle Physic Puzzles in astrophysics in the past and present |
authorStr |
Berezinsky, V. S. |
ppnlink_with_tag_str_mv |
@@773@@(DE-627)131188437 |
format |
Article |
dewey-ones |
530 - Physics |
delete_txt_mv |
keep |
author_role |
aut |
collection |
OLC |
remote_str |
false |
illustrated |
Not Illustrated |
issn |
1063-7788 |
topic_title |
530 VZ Puzzles in astrophysics in the past and present Radiation Elementary Particle Gamma Radiation Critical Review Particle Physic |
topic |
ddc 530 misc Radiation misc Elementary Particle misc Gamma Radiation misc Critical Review misc Particle Physic |
topic_unstemmed |
ddc 530 misc Radiation misc Elementary Particle misc Gamma Radiation misc Critical Review misc Particle Physic |
topic_browse |
ddc 530 misc Radiation misc Elementary Particle misc Gamma Radiation misc Critical Review misc Particle Physic |
format_facet |
Aufsätze Gedruckte Aufsätze |
format_main_str_mv |
Text Zeitschrift/Artikel |
carriertype_str_mv |
nc |
hierarchy_parent_title |
Physics of atomic nuclei |
hierarchy_parent_id |
131188437 |
dewey-tens |
530 - Physics |
hierarchy_top_title |
Physics of atomic nuclei |
isfreeaccess_txt |
false |
familylinks_str_mv |
(DE-627)131188437 (DE-600)1146378-8 (DE-576)032622155 |
title |
Puzzles in astrophysics in the past and present |
ctrlnum |
(DE-627)OLC2049896212 (DE-He213)1.1563699-p |
title_full |
Puzzles in astrophysics in the past and present |
author_sort |
Berezinsky, V. S. |
journal |
Physics of atomic nuclei |
journalStr |
Physics of atomic nuclei |
lang_code |
eng |
isOA_bool |
false |
dewey-hundreds |
500 - Science |
recordtype |
marc |
publishDateSort |
2003 |
contenttype_str_mv |
txt |
container_start_page |
423 |
author_browse |
Berezinsky, V. S. |
container_volume |
66 |
class |
530 VZ |
format_se |
Aufsätze |
author-letter |
Berezinsky, V. S. |
doi_str_mv |
10.1134/1.1563699 |
dewey-full |
530 |
title_sort |
puzzles in astrophysics in the past and present |
title_auth |
Puzzles in astrophysics in the past and present |
abstract |
Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. © MAIK "Nauka/Interperiodica" 2003 |
abstractGer |
Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. © MAIK "Nauka/Interperiodica" 2003 |
abstract_unstemmed |
Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given. © MAIK "Nauka/Interperiodica" 2003 |
collection_details |
GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST GBV_ILN_40 GBV_ILN_70 GBV_ILN_2014 GBV_ILN_2279 |
container_issue |
3 |
title_short |
Puzzles in astrophysics in the past and present |
url |
https://doi.org/10.1134/1.1563699 |
remote_bool |
false |
ppnlink |
131188437 |
mediatype_str_mv |
n |
isOA_txt |
false |
hochschulschrift_bool |
false |
doi_str |
10.1134/1.1563699 |
up_date |
2024-07-04T00:25:48.559Z |
_version_ |
1803606030874050560 |
fullrecord_marcxml |
<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2049896212</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504110320.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2003 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1134/1.1563699</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2049896212</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)1.1563699-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Berezinsky, V. S.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Puzzles in astrophysics in the past and present</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2003</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© MAIK "Nauka/Interperiodica" 2003</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract About 400 years have passed since the great discoveries by Galileo, Kepler, and Newton, but astronomy still remains an important source of discoveries in physics. They start with puzzles, with phenomena difficult to explain, and phenomena which in fact need new physics for explanation. Do such puzzles exist now? There are at least three candidates: absence of absorption of TeV gamma radiation in extragalactic space (violation of Lorentz invariance?), absence of GZK cutoff in the spectrum of ultrahigh-energy cosmic rays (new particle physics?), tremendous energy (up to $ 10^{54} $ erg) released in gamma ray bursts on a time scale of a second (collapsing stars or sources of a new type?). Do these puzzles really exist? A critical review of these phenomena is given.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Radiation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Elementary Particle</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Gamma Radiation</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Critical Review</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Particle Physic</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Physics of atomic nuclei</subfield><subfield code="d">Nauka/Interperiodica, 1993</subfield><subfield code="g">66(2003), 3 vom: März, Seite 423-434</subfield><subfield code="w">(DE-627)131188437</subfield><subfield code="w">(DE-600)1146378-8</subfield><subfield code="w">(DE-576)032622155</subfield><subfield code="x">1063-7788</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:66</subfield><subfield code="g">year:2003</subfield><subfield code="g">number:3</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:423-434</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1134/1.1563699</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2014</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">66</subfield><subfield code="j">2003</subfield><subfield code="e">3</subfield><subfield code="c">03</subfield><subfield code="h">423-434</subfield></datafield></record></collection>
|
score |
7.4011316 |