The dark matter problem :: a historical perspective /
"Most astronomers and physicists now believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Though invisible to current direct detection methods, dark matter can explain a vari...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Cambridge ; New York :
Cambridge University Press,
2010.
|
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Zusammenfassung: | "Most astronomers and physicists now believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Though invisible to current direct detection methods, dark matter can explain a variety of astronomical observations. This book describes how this theory has developed over the past 75 years, and why it is now a central feature of extragalactic astronomy and cosmology. Current attempts to directly detect dark matter locally are discussed, together with the implications for particle physics. The author comments on the sociology of these developments, demonstrating how and why scientists work and interact. Modified Newtonian Dynamics (MOND), the leading alternative to this theory, is also presented. This fascinating overview will interest cosmologists, astronomers and particle physicists. Mathematics is kept to a minimum, so the book can be understood by non-specialists"--Provided by publisher. |
| Beschreibung: | 1 online resource (viii, 205 pages) : illustrations |
| Bibliographie: | Includes bibliographical references (pages 195-201) and index. |
| ISBN: | 9780511773570 0511773579 9780511776151 0511776152 9781139192309 1139192302 |
Internformat
MARC
| LEADER | 00000cam a2200000 a 4500 | ||
|---|---|---|---|
| 001 | ZDB-4-EBA-ocn651130259 | ||
| 003 | OCoLC | ||
| 005 | 20241004212047.0 | ||
| 006 | m o d | ||
| 007 | cr cnu---auuuu | ||
| 008 | 100201s2010 enka ob 001 0 eng d | ||
| 010 | |z 2010004532 | ||
| 040 | |a CDX |b eng |e pn |c CDX |d NRC |d N$T |d OCLCQ |d E7B |d OCLCQ |d REDDC |d OCLCQ |d YDXCP |d OCLCQ |d OCLCF |d OCLCQ |d CAMBR |d OCLCQ |d YDX |d OCLCO |d COCUF |d LOA |d MERUC |d K6U |d STF |d WRM |d OCLCQ |d OCLCA |d VT2 |d AU@ |d OCLCO |d OCLCQ |d WYU |d LVT |d AGLDB |d SNK |d OCLCO |d OCLCQ |d A6Q |d OCL |d UKCRE |d OCLCO |d OCLCQ |d OCLCO |d OCLCQ |d OCLCL | ||
| 015 | |a GBA999406 |2 bnb | ||
| 016 | 7 | |a 015391181 |2 Uk | |
| 019 | |a 646066512 |a 738749538 |a 985279670 |a 985391188 |a 993268633 |a 1000247843 |a 1037914501 |a 1038702863 |a 1055318088 |a 1066419516 |a 1076624129 |a 1153467233 | ||
| 020 | |a 9780511773570 |q (electronic bk.) | ||
| 020 | |a 0511773579 |q (electronic bk.) | ||
| 020 | |a 9780511776151 |q (electronic bk.) | ||
| 020 | |a 0511776152 |q (electronic bk.) | ||
| 020 | |a 9781139192309 |q (electronic bk.) | ||
| 020 | |a 1139192302 |q (electronic bk.) | ||
| 020 | |z 0521113016 |q (hardback) | ||
| 020 | |z 9780521113014 |q (hardback) | ||
| 020 | |z 1801058202 | ||
| 020 | |z 9781801058209 | ||
| 024 | 8 | |a 9786612653445 | |
| 024 | 8 | |a 40018010582 | |
| 035 | |a (OCoLC)651130259 |z (OCoLC)646066512 |z (OCoLC)738749538 |z (OCoLC)985279670 |z (OCoLC)985391188 |z (OCoLC)993268633 |z (OCoLC)1000247843 |z (OCoLC)1037914501 |z (OCoLC)1038702863 |z (OCoLC)1055318088 |z (OCoLC)1066419516 |z (OCoLC)1076624129 |z (OCoLC)1153467233 | ||
| 037 | |a 265344 |b MIL | ||
| 050 | 4 | |a QB791.3 |b .S25 2010 ebook | |
| 072 | 7 | |a SCI |x 015000 |2 bisacsh | |
| 082 | 7 | |a 523.1/126 |2 22 | |
| 084 | |a US 2200 |2 rvk | ||
| 084 | |a US 3440 |2 rvk | ||
| 084 | |a PHY 928f |2 stub | ||
| 084 | |a PHY 926f |2 stub | ||
| 049 | |a MAIN | ||
| 100 | 1 | |a Sanders, Robert H. |0 http://id.loc.gov/authorities/names/n2010007076 | |
| 245 | 1 | 4 | |a The dark matter problem : |b a historical perspective / |c Robert H. Sanders. |
| 260 | |a Cambridge ; |a New York : |b Cambridge University Press, |c 2010. | ||
| 300 | |a 1 online resource (viii, 205 pages) : |b illustrations | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a data file |2 rda | ||
| 504 | |a Includes bibliographical references (pages 195-201) and index. | ||
| 505 | 0 | |a Introduction -- Early history of the dark matter hypothesis -- The stability of disk galaxies : the dark-halo solution -- Direct evidence : extended rotation curves of spiral galaxies -- The maximum-disk : light traces mass -- Cosmology and the birth of astroparticle physics -- Clusters revisited : missing mass found -- CDM confronts galaxy rotation curves -- The new cosmology : dark matter is not enough -- An alternative to dark matter : Modified Newtonian Dynamics -- Seeing dark matter : the theory and practice of detection -- Reflections : a personal point of view. | |
| 520 | |a "Most astronomers and physicists now believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Though invisible to current direct detection methods, dark matter can explain a variety of astronomical observations. This book describes how this theory has developed over the past 75 years, and why it is now a central feature of extragalactic astronomy and cosmology. Current attempts to directly detect dark matter locally are discussed, together with the implications for particle physics. The author comments on the sociology of these developments, demonstrating how and why scientists work and interact. Modified Newtonian Dynamics (MOND), the leading alternative to this theory, is also presented. This fascinating overview will interest cosmologists, astronomers and particle physicists. Mathematics is kept to a minimum, so the book can be understood by non-specialists"--Provided by publisher. | ||
| 588 | 0 | |a Print version record. | |
| 650 | 0 | |a Dark matter (Astronomy) |x History. | |
| 650 | 6 | |a Matière sombre (Astronomie) |x Histoire. | |
| 650 | 7 | |a SCIENCE |x Cosmology. |2 bisacsh | |
| 650 | 7 | |a Dark matter (Astronomy) |2 fast | |
| 650 | 7 | |a Dunkle Materie |2 gnd | |
| 650 | 7 | |a Dunkle Materie |y Geschichte. |2 idsbb | |
| 650 | 7 | |a Dunkle Materie. |2 idszbz | |
| 650 | 7 | |a Kosmologie. |2 idszbz | |
| 655 | 7 | |a History |2 fast | |
| 758 | |i has work: |a The dark matter problem (Text) |1 https://id.oclc.org/worldcat/entity/E39PCFRvCmvFtVFCRhPpCmQPBd |4 https://id.oclc.org/worldcat/ontology/hasWork | ||
| 776 | 0 | 8 | |i Print version: |a Sanders, Robert H. |t Dark matter problem. |d Cambridge, UK ; New York : Cambridge University Press, 2010 |z 9780521113014 |w (DLC) 2010004532 |w (OCoLC)456838475 |
| 856 | 4 | 0 | |l FWS01 |p ZDB-4-EBA |q FWS_PDA_EBA |u https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=324102 |3 Volltext |
| 938 | |a Coutts Information Services |b COUT |n 14244922 | ||
| 938 | |a ebrary |b EBRY |n ebr10397305 | ||
| 938 | |a EBSCOhost |b EBSC |n 324102 | ||
| 938 | |a YBP Library Services |b YANK |n 3343339 | ||
| 938 | |a YBP Library Services |b YANK |n 11970993 | ||
| 938 | |a YBP Library Services |b YANK |n 3336278 | ||
| 938 | |a YBP Library Services |b YANK |n 3371128 | ||
| 994 | |a 92 |b GEBAY | ||
| 912 | |a ZDB-4-EBA | ||
| 049 | |a DE-863 | ||
Datensatz im Suchindex
| DE-BY-FWS_katkey | ZDB-4-EBA-ocn651130259 |
|---|---|
| _version_ | 1816881733265522688 |
| adam_text | |
| any_adam_object | |
| author | Sanders, Robert H. |
| author_GND | http://id.loc.gov/authorities/names/n2010007076 |
| author_facet | Sanders, Robert H. |
| author_role | |
| author_sort | Sanders, Robert H. |
| author_variant | r h s rh rhs |
| building | Verbundindex |
| bvnumber | localFWS |
| callnumber-first | Q - Science |
| callnumber-label | QB791 |
| callnumber-raw | QB791.3 .S25 2010 ebook |
| callnumber-search | QB791.3 .S25 2010 ebook |
| callnumber-sort | QB 3791.3 S25 42010 EBOOK |
| callnumber-subject | QB - Astronomy |
| classification_rvk | US 2200 US 3440 |
| classification_tum | PHY 928f PHY 926f |
| collection | ZDB-4-EBA |
| contents | Introduction -- Early history of the dark matter hypothesis -- The stability of disk galaxies : the dark-halo solution -- Direct evidence : extended rotation curves of spiral galaxies -- The maximum-disk : light traces mass -- Cosmology and the birth of astroparticle physics -- Clusters revisited : missing mass found -- CDM confronts galaxy rotation curves -- The new cosmology : dark matter is not enough -- An alternative to dark matter : Modified Newtonian Dynamics -- Seeing dark matter : the theory and practice of detection -- Reflections : a personal point of view. |
| ctrlnum | (OCoLC)651130259 |
| dewey-full | 523.1/126 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.1/126 |
| dewey-search | 523.1/126 |
| dewey-sort | 3523.1 3126 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>05186cam a2200805 a 4500</leader><controlfield tag="001">ZDB-4-EBA-ocn651130259</controlfield><controlfield tag="003">OCoLC</controlfield><controlfield tag="005">20241004212047.0</controlfield><controlfield tag="006">m o d </controlfield><controlfield tag="007">cr cnu---auuuu</controlfield><controlfield tag="008">100201s2010 enka ob 001 0 eng d</controlfield><datafield tag="010" ind1=" " ind2=" "><subfield code="z"> 2010004532</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">CDX</subfield><subfield code="b">eng</subfield><subfield code="e">pn</subfield><subfield code="c">CDX</subfield><subfield code="d">NRC</subfield><subfield code="d">N$T</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">E7B</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">REDDC</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">YDXCP</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">OCLCF</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">CAMBR</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">YDX</subfield><subfield code="d">OCLCO</subfield><subfield code="d">COCUF</subfield><subfield code="d">LOA</subfield><subfield code="d">MERUC</subfield><subfield code="d">K6U</subfield><subfield code="d">STF</subfield><subfield code="d">WRM</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">OCLCA</subfield><subfield code="d">VT2</subfield><subfield code="d">AU@</subfield><subfield code="d">OCLCO</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">WYU</subfield><subfield code="d">LVT</subfield><subfield code="d">AGLDB</subfield><subfield code="d">SNK</subfield><subfield code="d">OCLCO</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">A6Q</subfield><subfield code="d">OCL</subfield><subfield code="d">UKCRE</subfield><subfield code="d">OCLCO</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">OCLCO</subfield><subfield code="d">OCLCQ</subfield><subfield code="d">OCLCL</subfield></datafield><datafield tag="015" ind1=" " ind2=" "><subfield code="a">GBA999406</subfield><subfield code="2">bnb</subfield></datafield><datafield tag="016" ind1="7" ind2=" "><subfield code="a">015391181</subfield><subfield code="2">Uk</subfield></datafield><datafield tag="019" ind1=" " ind2=" "><subfield code="a">646066512</subfield><subfield code="a">738749538</subfield><subfield code="a">985279670</subfield><subfield code="a">985391188</subfield><subfield code="a">993268633</subfield><subfield code="a">1000247843</subfield><subfield code="a">1037914501</subfield><subfield code="a">1038702863</subfield><subfield code="a">1055318088</subfield><subfield code="a">1066419516</subfield><subfield code="a">1076624129</subfield><subfield code="a">1153467233</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780511773570</subfield><subfield code="q">(electronic bk.)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">0511773579</subfield><subfield code="q">(electronic bk.)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780511776151</subfield><subfield code="q">(electronic bk.)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">0511776152</subfield><subfield code="q">(electronic bk.)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9781139192309</subfield><subfield code="q">(electronic bk.)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">1139192302</subfield><subfield code="q">(electronic bk.)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="z">0521113016</subfield><subfield code="q">(hardback)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="z">9780521113014</subfield><subfield code="q">(hardback)</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="z">1801058202</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="z">9781801058209</subfield></datafield><datafield tag="024" ind1="8" ind2=" "><subfield code="a">9786612653445</subfield></datafield><datafield tag="024" ind1="8" ind2=" "><subfield code="a">40018010582</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)651130259</subfield><subfield code="z">(OCoLC)646066512</subfield><subfield code="z">(OCoLC)738749538</subfield><subfield code="z">(OCoLC)985279670</subfield><subfield code="z">(OCoLC)985391188</subfield><subfield code="z">(OCoLC)993268633</subfield><subfield code="z">(OCoLC)1000247843</subfield><subfield code="z">(OCoLC)1037914501</subfield><subfield code="z">(OCoLC)1038702863</subfield><subfield code="z">(OCoLC)1055318088</subfield><subfield code="z">(OCoLC)1066419516</subfield><subfield code="z">(OCoLC)1076624129</subfield><subfield code="z">(OCoLC)1153467233</subfield></datafield><datafield tag="037" ind1=" " ind2=" "><subfield code="a">265344</subfield><subfield code="b">MIL</subfield></datafield><datafield tag="050" ind1=" " ind2="4"><subfield code="a">QB791.3</subfield><subfield code="b">.S25 2010 ebook</subfield></datafield><datafield tag="072" ind1=" " ind2="7"><subfield code="a">SCI</subfield><subfield code="x">015000</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="082" ind1="7" ind2=" "><subfield code="a">523.1/126</subfield><subfield code="2">22</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">US 2200</subfield><subfield code="2">rvk</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">US 3440</subfield><subfield code="2">rvk</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 928f</subfield><subfield code="2">stub</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 926f</subfield><subfield code="2">stub</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">MAIN</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Sanders, Robert H.</subfield><subfield code="0">http://id.loc.gov/authorities/names/n2010007076</subfield></datafield><datafield tag="245" ind1="1" ind2="4"><subfield code="a">The dark matter problem :</subfield><subfield code="b">a historical perspective /</subfield><subfield code="c">Robert H. Sanders.</subfield></datafield><datafield tag="260" ind1=" " ind2=" "><subfield code="a">Cambridge ;</subfield><subfield code="a">New York :</subfield><subfield code="b">Cambridge University Press,</subfield><subfield code="c">2010.</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 online resource (viii, 205 pages) :</subfield><subfield code="b">illustrations</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">computer</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">online resource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="347" ind1=" " ind2=" "><subfield code="a">data file</subfield><subfield code="2">rda</subfield></datafield><datafield tag="504" ind1=" " ind2=" "><subfield code="a">Includes bibliographical references (pages 195-201) and index.</subfield></datafield><datafield tag="505" ind1="0" ind2=" "><subfield code="a">Introduction -- Early history of the dark matter hypothesis -- The stability of disk galaxies : the dark-halo solution -- Direct evidence : extended rotation curves of spiral galaxies -- The maximum-disk : light traces mass -- Cosmology and the birth of astroparticle physics -- Clusters revisited : missing mass found -- CDM confronts galaxy rotation curves -- The new cosmology : dark matter is not enough -- An alternative to dark matter : Modified Newtonian Dynamics -- Seeing dark matter : the theory and practice of detection -- Reflections : a personal point of view.</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">"Most astronomers and physicists now believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Though invisible to current direct detection methods, dark matter can explain a variety of astronomical observations. This book describes how this theory has developed over the past 75 years, and why it is now a central feature of extragalactic astronomy and cosmology. Current attempts to directly detect dark matter locally are discussed, together with the implications for particle physics. The author comments on the sociology of these developments, demonstrating how and why scientists work and interact. Modified Newtonian Dynamics (MOND), the leading alternative to this theory, is also presented. This fascinating overview will interest cosmologists, astronomers and particle physicists. Mathematics is kept to a minimum, so the book can be understood by non-specialists"--Provided by publisher.</subfield></datafield><datafield tag="588" ind1="0" ind2=" "><subfield code="a">Print version record.</subfield></datafield><datafield tag="650" ind1=" " ind2="0"><subfield code="a">Dark matter (Astronomy)</subfield><subfield code="x">History.</subfield></datafield><datafield tag="650" ind1=" " ind2="6"><subfield code="a">Matière sombre (Astronomie)</subfield><subfield code="x">Histoire.</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">SCIENCE</subfield><subfield code="x">Cosmology.</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Dark matter (Astronomy)</subfield><subfield code="2">fast</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Dunkle Materie</subfield><subfield code="2">gnd</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Dunkle Materie</subfield><subfield code="y">Geschichte.</subfield><subfield code="2">idsbb</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Dunkle Materie.</subfield><subfield code="2">idszbz</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Kosmologie.</subfield><subfield code="2">idszbz</subfield></datafield><datafield tag="655" ind1=" " ind2="7"><subfield code="a">History</subfield><subfield code="2">fast</subfield></datafield><datafield tag="758" ind1=" " ind2=" "><subfield code="i">has work:</subfield><subfield code="a">The dark matter problem (Text)</subfield><subfield code="1">https://id.oclc.org/worldcat/entity/E39PCFRvCmvFtVFCRhPpCmQPBd</subfield><subfield code="4">https://id.oclc.org/worldcat/ontology/hasWork</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Print version:</subfield><subfield code="a">Sanders, Robert H.</subfield><subfield code="t">Dark matter problem.</subfield><subfield code="d">Cambridge, UK ; New York : Cambridge University Press, 2010</subfield><subfield code="z">9780521113014</subfield><subfield code="w">(DLC) 2010004532</subfield><subfield code="w">(OCoLC)456838475</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="l">FWS01</subfield><subfield code="p">ZDB-4-EBA</subfield><subfield code="q">FWS_PDA_EBA</subfield><subfield code="u">https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=324102</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="938" ind1=" " ind2=" "><subfield code="a">Coutts Information Services</subfield><subfield code="b">COUT</subfield><subfield code="n">14244922</subfield></datafield><datafield tag="938" ind1=" " ind2=" "><subfield code="a">ebrary</subfield><subfield code="b">EBRY</subfield><subfield code="n">ebr10397305</subfield></datafield><datafield tag="938" ind1=" " ind2=" "><subfield code="a">EBSCOhost</subfield><subfield code="b">EBSC</subfield><subfield code="n">324102</subfield></datafield><datafield tag="938" ind1=" " ind2=" "><subfield code="a">YBP Library Services</subfield><subfield code="b">YANK</subfield><subfield code="n">3343339</subfield></datafield><datafield tag="938" ind1=" " ind2=" "><subfield code="a">YBP Library Services</subfield><subfield code="b">YANK</subfield><subfield code="n">11970993</subfield></datafield><datafield tag="938" ind1=" " ind2=" "><subfield code="a">YBP Library Services</subfield><subfield code="b">YANK</subfield><subfield code="n">3336278</subfield></datafield><datafield tag="938" ind1=" " ind2=" "><subfield code="a">YBP Library Services</subfield><subfield code="b">YANK</subfield><subfield code="n">3371128</subfield></datafield><datafield tag="994" ind1=" " ind2=" "><subfield code="a">92</subfield><subfield code="b">GEBAY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-4-EBA</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-863</subfield></datafield></record></collection> |
| genre | History fast |
| genre_facet | History |
| id | ZDB-4-EBA-ocn651130259 |
| illustrated | Illustrated |
| indexdate | 2024-11-27T13:17:24Z |
| institution | BVB |
| isbn | 9780511773570 0511773579 9780511776151 0511776152 9781139192309 1139192302 |
| language | English |
| oclc_num | 651130259 |
| open_access_boolean | |
| owner | MAIN DE-863 DE-BY-FWS |
| owner_facet | MAIN DE-863 DE-BY-FWS |
| physical | 1 online resource (viii, 205 pages) : illustrations |
| psigel | ZDB-4-EBA |
| publishDate | 2010 |
| publishDateSearch | 2010 |
| publishDateSort | 2010 |
| publisher | Cambridge University Press, |
| record_format | marc |
| spelling | Sanders, Robert H. http://id.loc.gov/authorities/names/n2010007076 The dark matter problem : a historical perspective / Robert H. Sanders. Cambridge ; New York : Cambridge University Press, 2010. 1 online resource (viii, 205 pages) : illustrations text txt rdacontent computer c rdamedia online resource cr rdacarrier data file rda Includes bibliographical references (pages 195-201) and index. Introduction -- Early history of the dark matter hypothesis -- The stability of disk galaxies : the dark-halo solution -- Direct evidence : extended rotation curves of spiral galaxies -- The maximum-disk : light traces mass -- Cosmology and the birth of astroparticle physics -- Clusters revisited : missing mass found -- CDM confronts galaxy rotation curves -- The new cosmology : dark matter is not enough -- An alternative to dark matter : Modified Newtonian Dynamics -- Seeing dark matter : the theory and practice of detection -- Reflections : a personal point of view. "Most astronomers and physicists now believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Though invisible to current direct detection methods, dark matter can explain a variety of astronomical observations. This book describes how this theory has developed over the past 75 years, and why it is now a central feature of extragalactic astronomy and cosmology. Current attempts to directly detect dark matter locally are discussed, together with the implications for particle physics. The author comments on the sociology of these developments, demonstrating how and why scientists work and interact. Modified Newtonian Dynamics (MOND), the leading alternative to this theory, is also presented. This fascinating overview will interest cosmologists, astronomers and particle physicists. Mathematics is kept to a minimum, so the book can be understood by non-specialists"--Provided by publisher. Print version record. Dark matter (Astronomy) History. Matière sombre (Astronomie) Histoire. SCIENCE Cosmology. bisacsh Dark matter (Astronomy) fast Dunkle Materie gnd Dunkle Materie Geschichte. idsbb Dunkle Materie. idszbz Kosmologie. idszbz History fast has work: The dark matter problem (Text) https://id.oclc.org/worldcat/entity/E39PCFRvCmvFtVFCRhPpCmQPBd https://id.oclc.org/worldcat/ontology/hasWork Print version: Sanders, Robert H. Dark matter problem. Cambridge, UK ; New York : Cambridge University Press, 2010 9780521113014 (DLC) 2010004532 (OCoLC)456838475 FWS01 ZDB-4-EBA FWS_PDA_EBA https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=324102 Volltext |
| spellingShingle | Sanders, Robert H. The dark matter problem : a historical perspective / Introduction -- Early history of the dark matter hypothesis -- The stability of disk galaxies : the dark-halo solution -- Direct evidence : extended rotation curves of spiral galaxies -- The maximum-disk : light traces mass -- Cosmology and the birth of astroparticle physics -- Clusters revisited : missing mass found -- CDM confronts galaxy rotation curves -- The new cosmology : dark matter is not enough -- An alternative to dark matter : Modified Newtonian Dynamics -- Seeing dark matter : the theory and practice of detection -- Reflections : a personal point of view. Dark matter (Astronomy) History. Matière sombre (Astronomie) Histoire. SCIENCE Cosmology. bisacsh Dark matter (Astronomy) fast Dunkle Materie gnd Dunkle Materie Geschichte. idsbb Dunkle Materie. idszbz Kosmologie. idszbz |
| title | The dark matter problem : a historical perspective / |
| title_auth | The dark matter problem : a historical perspective / |
| title_exact_search | The dark matter problem : a historical perspective / |
| title_full | The dark matter problem : a historical perspective / Robert H. Sanders. |
| title_fullStr | The dark matter problem : a historical perspective / Robert H. Sanders. |
| title_full_unstemmed | The dark matter problem : a historical perspective / Robert H. Sanders. |
| title_short | The dark matter problem : |
| title_sort | dark matter problem a historical perspective |
| title_sub | a historical perspective / |
| topic | Dark matter (Astronomy) History. Matière sombre (Astronomie) Histoire. SCIENCE Cosmology. bisacsh Dark matter (Astronomy) fast Dunkle Materie gnd Dunkle Materie Geschichte. idsbb Dunkle Materie. idszbz Kosmologie. idszbz |
| topic_facet | Dark matter (Astronomy) History. Matière sombre (Astronomie) Histoire. SCIENCE Cosmology. Dark matter (Astronomy) Dunkle Materie Dunkle Materie Geschichte. Dunkle Materie. Kosmologie. History |
| url | https://search.ebscohost.com/login.aspx?direct=true&scope=site&db=nlebk&AN=324102 |
| work_keys_str_mv | AT sandersroberth thedarkmatterproblemahistoricalperspective AT sandersroberth darkmatterproblemahistoricalperspective |