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An Open Letter to the Scientific Community
cosmologystatement.org
(Published
in New Scientist, May 22, 2004)
The big bang today relies on a
growing number of hypothetical entities, things that we have never observed--
inflation, dark matter and dark energy are the most prominent examples. Without
them, there would be a fatal contradiction between the observations made by
astronomers and the predictions of the big bang theory. In no other field of
physics would this continual recourse to new hypothetical objects be accepted
as a way of bridging the gap between theory and observation. It would, at the
least, raise serious questions about the validity of the underlying theory.
But the big bang theory can't
survive without these fudge factors. Without the hypothetical inflation
field, the big bang does not predict the smooth, isotropic cosmic background
radiation that is observed, because there would be no way for parts of the universe
that are now more than a few degrees away in the sky to come to the same
temperature and thus emit the same amount of microwave radiation.
Without some kind of dark
matter, unlike any that we have observed on Earth despite 20 years of
experiments, big-bang theory makes contradictory predictions for the density
of matter in the universe. Inflation requires a density 20 times larger than
that implied by big bang nucleosynthesis, the theory's explanation of the
origin of the light elements. And without dark energy, the theory predicts
that the universe is only about 8 billion years old, which is billions of
years younger than the age of many stars in our galaxy.
What is more, the big bang
theory can boast of no quantitative predictions that have subsequently been
validated by observation. The successes claimed by the theory's supporters
consist of its ability to retrospectively fit observations with a steadily
increasing array of adjustable parameters, just as the old Earth-centered
cosmology of Ptolemy needed layer upon layer of epicycles.
Yet the big bang is not the only
framework available for understanding the history of the universe. Plasma
cosmology and the steady-state model both hypothesize an evolving universe
without beginning or end. These and other alternative approaches can also
explain the basic phenomena of the cosmos, including the abundances of light
elements, the generation of large-scale structure, the cosmic background
radiation, and how the redshift of far-away galaxies increases with distance.
They have even predicted new phenomena that were subsequently observed,
something the big bang has failed to do.
Supporters of the big bang
theory may retort that these theories do not explain every cosmological
observation. But that is scarcely surprising, as their development has been
severely hampered by a complete lack of funding. Indeed, such questions and
alternatives cannot even now be freely discussed and examined. An open
exchange of ideas is lacking in most mainstream conferences. Whereas Richard
Feynman could say that "science is the culture of doubt", in
cosmology today doubt and dissent are not tolerated, and young scientists
learn to remain silent if they have something negative to say about the
standard big bang model. Those who doubt the big bang fear that saying so
will cost them their funding.
Even observations are now
interpreted through this biased filter, judged right or wrong depending on
whether or not they support the big bang. So discordant data on red shifts,
lithium and helium abundances, and galaxy distribution, among other topics,
are ignored or ridiculed. This reflects a growing dogmatic mindset that is
alien to the spirit of free scientific inquiry.
Today, virtually all financial
and experimental resources in cosmology are devoted to big bang studies. Funding
comes from only a few sources, and all the peer-review committees that
control them are dominated by supporters of the big bang. As a result, the
dominance of the big bang within the field has become self-sustaining,
irrespective of the scientific validity of the theory.
Giving support only to projects
within the big bang framework undermines a fundamental element of the
scientific method -- the constant testing of theory against observation. Such
a restriction makes unbiased discussion and research impossible. To redress
this, we urge those agencies that fund work in cosmology to set aside a
significant fraction of their funding for investigations into alternative
theories and observational contradictions of the big bang. To avoid bias, the
peer review committee that allocates such funds could be composed of
astronomers and physicists from outside the field of cosmology.
Allocating funding to
investigations into the big bang's validity, and its alternatives, would allow
the scientific process to determine our most accurate model of the history of
the universe.
If you want to sign this statement ,
please click here
Original
Signers
| Scientists and Engineers | Independent Researchers | Other
Signers
Signed:
(Institutions for identification only)
Highlighted names
are linked to related web pages
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Halton Arp, Max-Planck-Institute Fur Astrophysik (Germany)
Andre Koch Torres Assis, State University of Campinas (Brazil)
Yuri Baryshev, Astronomical Institute, St.
Petersburg State University (Russia)
Ari Brynjolfsson, Applied Radiation Industries
(USA)
Hermann Bondi, Churchill College, University of Cambridge (UK)
Timothy Eastman, Plasmas International (USA)
Chuck Gallo, Superconix, Inc.(USA)
Thomas Gold, Cornell University (emeritus) (USA)
Amitabha Ghosh, Indian Institute of Technology, Kanpur (India)
Walter J. Heikkila, University of Texas at Dallas (USA)
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Michael Ibison, Institute for Advanced
Studies at Austin (USA)
Thomas Jarboe, University of Washington (USA)
Jerry W. Jensen, ATK Propulsion (USA)
Menas Kafatos, George Mason University (USA)
Eric J. Lerner, Lawrenceville Plasma Physics (USA)
Paul Marmet, Herzberg Institute of Astrophysics (retired)
(Canada)
Paola Marziani, Istituto Nazionale di
Astrofisica, Osservatorio Astronomico di Padova (Italy)
Gregory Meholic, The Aerospace Corporation (USA)
Jacques Moret-Bailly, Université Dijon (retired) (France)
Jayant Narlikar, IUCAA(emeritus) and College de France (India, France)
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Marcos Cesar Danhoni Neves, State
University of Maringá (Brazil)
Charles D. Orth, Lawrence Livermore National
Laboratory (USA)
R. David Pace, Lyon College (USA)
Georges Paturel, Observatoire de Lyon (France)
Jean-Claude Pecker, College de France (France)
Anthony L. Peratt, Los Alamos National Laboratory (USA)
Bill Peter, BAE Systems Advanced Technologies (USA)
David Roscoe, Sheffield University (UK)
Malabika Roy, George Mason University (USA)
Sisir Roy, George Mason University (USA)
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Konrad Rudnicki, Jagiellonian
University (Poland)
Domingos S.L. Soares, Federal University of Minas Gerais
(Brazil)
John L. West, Jet Propulsion Laboratory,
California Institute of Technology (USA)
James F. Woodward, California State University, Fullerton (USA)
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New signers of the Open
letter since publication
Scientists and Engineers
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Jorge Marao Universidade Estadual de
Londrina Brazi
Martin John Baker, Loretto School Musselburgh, UK
Peter
J Carroll, Psychonaut Institute, UK
Roger Y. Gouin, Ecole Superieure d'Electricite, France
John Murray, Sunyata Composite Ltd, UK
Jonathan Chambers, University of Sheffield, UK
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Michel A. Duguay, Laval
University, Canada
Qi Pan, Fitzwilliam College, Cambridge, UK
Fred Rost, University of NSW (Emeritus), Australia
Louis Hissink, Consulting Geologist, Australia
Hetu Sheth, Earth Sciences, Indian Institute of Technology Bombay, India
Lassi Hyvärinen, IBM(Ret), France
Max Whisson, University of Melbourne, Australia
R.S.Griffiths, CADAS, UK
Adolf Muenker, Brane Industries, USA
Emre Isik Akdeniz University Turkey
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Felipe de Oliveira Alves, Federal
University of Minas Gerais, Brazil
Jean-Marc Bonnet-Bidaud, Service d'Astrophysique, CEA, France
Kim George, Curtin University of Technology, Australia
Tom Van Flandern,
Meta Research, USA
Doneley Watson, IBM (ret.), USA
Fred Alan Wolf, Have Brains / Will Travel, USA
Robert Wood, IEEE, Canada
D. W. Harris, L-3 Communications, USA
Eugene
Sittampalam, Engineering consultant, Sri Lanka
Joseph.B. Krieger, Brooklyn College, CUNY, USA
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Pablo Vasquez, New Jersey Institute of
Technology, USA
Peter F. Richiuso, NASA, KSC, USA
Roger A. Rydin, University of Virginia (Emeritus), USA
Stefan Rydstrom, Royal Institute of Technology, Sweden
Sylvan J. Hotch, The MITRE Corporation (Retired), USA
Thomas R. Love, CSU Dominguez Hills, USA
Andrew Coles, Embedded Systems, USA
Eit Gaastra,
infinite universe researcher, The Netherlands
Franco Selleri, Università di Bari, Dipartimento di Fisica, Italy
Gerald Pease, The Aerospace Corporation, USA ..............................................................
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S.N. Arteha, Space Research Institute, Russia
Miroslaw Kozlowski, Warsaw University (emeritus), Poland
John
Hartnett, School of Physics, University of Western Australia, Australia
Robert Zubrin, Pioneer Astronautics, USA
Tibor Gasparik, SUNY at Stony Brook, USA
Alexandre Losev, Bulgarian Academy of Sciences, Bulgaria
Henry Hall, University of Manchester, UK
José da Silva, Universidade Federal de Minas Gerais, Brazil
Markus Rohner, Griesser AG, Switzerland
William C. Mitchell, Institute for
Advanced Cosmological Studies, USA
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Aurea Garcia-Rissmann, UFSC, Brazil
Cristian R. Ghezzi, Universidade Estadual de Campinas, Brazil
Daniel Nicolato Epitácio Pereira, Federal University of Rio de
Janeiro, Brazil
Gregory M. Salyards, US Naval Sea Systems Command (ret.), USA
Luiz Carlos Barbosa, Unicamp, Brazil
Luiz Carlos Jafelice, Federal University of the Rio Grande do Norte,
Brazil
Michael Sosteric, Athabasca University, Canada
Steven Langley Guy, University of Elizabeth (Physics Department), Australia
Robert Fritzius, Shade Tree Physics, USA
Irineu Gomes Varella, Escola Municipal de
Astrofísica, Brazil
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90
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Tom Walther, Southern Cross University
Australia , Australia
Mauro Cosentino, University of São Paulo, Brazil
Moacir Lacerda, Univeersidade Federal de Mato Grosso do Sul, Brazil
Roberto Assumpcao, PUC Minas, Brazil
Roberto Lopes Parra, University of Sao Paulo, Brazil
Ronaldo Junio Camppos Batista, Universidade Federal de Minas Gerais, Brazil
Ermenegildo Caccese, University of Basilicata, Italy
Felipe Sofia Zanuzzo, Federal University of São Carlos, Brazil
Edival de Morais, Sociedade Brasileira de Física, Brazil
Graham Coupe, KAZ Technology Services, Australia
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Gordon Petrie, High Altitude
Observatory, NCAR, USA,
Jose
B. Almeida, University of Minho, Portugal,
Antonio Cleiton, Laboratório de Sistemas
Complexos - UFPI, Brazil
Sergey Karpov, L.V.Kirensky Institute of Physics Russian Academy of
Sciences, Russia
Wagner Patrick Junqueira de Souza Coelho Nicácio, Universidade
Federal de Minas Gerais, Brazil
Sokolov Vladimir, Special Astrophysical Observatory of RAS,
Russia
Edwin G. Schasteen, TAP-TEN Research Foundation International, USA
Gerry Zeitlin, openseti.org, USA
Henry H. Bauer, Virginia Polytechnic Institute & State University, USA
Yasha Fard,H.R. Cosmology Institute, Canada
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Roberto Caimmi, Astronomy Department,
Padua University, Italy
Tobias Keller,
ETH (SFIT) Zurich, Earth Sciences, Switzerland,
Deborah Foch,
Center for the Study of Extraterrestrial Intelligence, USA,
Henry Reynolds, UC Santa Cruz, USA,
Paramahamsa Tewari, Nuclear Power Corporation (ret.),India
Jouko Seppänen, Helsinki University of Technology, Finland,
Cristiane Ribeiro Bernardes, Universidade Federal de Minas Gerais, Brazil
Eric Blievernicht. TRW, USA
Dr. Robert
Bennett, Kolbe Center, USA,
Hilton Ratcliffe, Astronomical Society of South Africa, South Africa .......................................
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Wieslaw Sztumski, Silesian
University, Poland
Lars Wåhlin,Colutron Research Corporation,USA
Riccardo
Scarpa, European Southern Observatory, Italy,
Olivier Marco, European Southern Observatory, France
Joseph Garcia, International
Radiation Protection, Germany,
Arkadiusz Jadczyk, International Institute of Mathematical Physics,
Lithuania
Jean de Pontcharra, Commissariat à l'Energie Atomique, France
Gerardus D. Bouw, Baldwin-Wallace College, USA
Josef Lutz, Chemnitz University of Technology, Germany,
Harold E. Puthoff, Institute for Advanced Studies at Austin, USA.
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Hermann
Dürkop, Nabla Systemberatung, Germany,
Klaus Fischer, Universität Trier, Germany,
Werner Holzmüller, University Leipzig, Germany
Sol Aisenberg, International Technology Group, USA
Richard Gancarczyk, University of Nottingham, UK
Steve Humphry, Murdoch University, Australia
Alberto Bolognesi, Università di Perugia, Italy
Daniele Carosati, Armenzano Observatory, Italy
Brendan Dean, H.R. Cosmology Institute, Canada
W. Jim
Jastrzebski, Warsaw University, Poland ..................................................
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140
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Gero Rupprecht, European Southern Observatory, Germany
Rainer Herrmann TEWS-Elektronik Germany
Felix Pharand
University of Montreal Canada
Jerry Bergman Northwest State University
USA
Tibor Gasparik SUNY at Stony Brook USA
Rei Gunn University of Nantucket
USA
Sinan
Alis Eyuboglu Twin Observatories Turkey
Esat Rennan Pekünlü University of EGE Turkey
Anne M. Hofmeister Washington U. USA
Quentin Foreman IEEE New Zealand
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150
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Marc Berndl University of
Toronto Canada
Y. P.
Varshni University of Ottawa Canada
Robert Martinek McMaster University Canada
Bob Criss Washington University USA
Sol Aisenberg, International Technology Group, USA
Paul LaViolette, The Starburst Foundation, U.S.A.
Seetesh Pandé, Universite Claude Bernard, Lyon France
TAHIR MAQSOOD, PSA, PAKISTAN
Hartmut Traunmüller, University of Stockholm, Sweden
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Nico F. Benschop, Amspade Research, Netherlands
Aaron Blake, USAF, USA
M. Ross Fergus, University of Memphis, USA
Sonu
Bhaskar, Council of Scientific and Industrial Research, India
Frederico V. F., Lima Universidade de Sao
Paulo, Brazil
Andrei
Kirilyuk, Institute of Metal Physics of the National Academy of
Sciences of Ukraine, Ukraine
Christian Jooss, Institut fuer Materialphysik,
University of Goettingen, Germany
Sonu
Bhaskar, BCISR, India
Robert O. Myers, ROM Technologies, USA
Ana Cristina Oliveira, Universidade Federal de Minas Gerais, Brazil
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170
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John Wey, Idaho National Laboratory,
USA
Jorge Francisco
Maldonado Serrano, UIS, Colombia
Pasquale Galianni, Dipartimento di Fisica
Università di Lecce, Italy
Martín López-Corredoira, Instituto de
Astrofísica de Canarias, Spain
Michael A.
Ivanov, Belarus State University of Informatics and Radioelectronics,
Belarus
Xiao Jianhua , Shanghai Jiaotong University,
China
Pierre J. Beaujon, Hoornbeeck College, The Netherlands
J.Georg von Brzeski Helios Labs. USA
vidyardhi
nanduri , Cosmology Research center , India
Mike Rotch NBSA USA
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