Endre søk
RefereraExporteraLink to record
Permanent link

Direct link
Referera
Referensformat
  • apa
  • harvard1
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Annet format
Fler format
Språk
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Annet språk
Fler språk
Utmatningsformat
  • html
  • text
  • asciidoc
  • rtf
Theoretical and Phenomenological Studies of Neutrino Physics
KTH, Skolan för teknikvetenskap (SCI), Teoretisk fysik, Teoretisk partikelfysik.ORCID-id: 0000-0001-5948-9152
2007 (engelsk)Doktoravhandling, med artikler (Annet vitenskapelig)
Abstract [en]

This thesis is devoted to the theory and phenomenology of neutrino physics. While the standard model of particle physics has been extremely successful, it fails to account for massive neutrinos, which are necessary to describe the observations of neutrino oscillations made by several different experiments. Thus, neutrino physics is a possible window for exploring the physics beyond the standard model, making it both interesting and important for our fundamental understanding of Nature.

Throughout this thesis, we will discuss different aspects of neutrino physics, ranging from taking all three types of neutrinos into account in neutrino oscillation experiments to exploring the possibilities of neutrino mass models to produce a viable source of the baryon asymmetry of the Universe. The emphasis of the thesis is on neutrino oscillations which, given their implication of neutrino masses, is a phenomenon where other results that are not describable in the standard model could be found, such as new interactions between neutrinos and fermions.

sted, utgiver, år, opplag, sider
Stockholm: Teoretisk fysik , 2007. , s. xii, 102, [7]
Serie
Trita-FYS, ISSN 0280-316X ; 2007:31
Emneord [en]
neutrino mass, neutrino mixing, neutrino oscillations, matter effects, non-standard effects, the day-night effect, solar neutrinos, accelerator neutrinos, exact solutions, three-flavor effects, large density, neutrino decay, neutrino decoherence, neutrino absorption, non-standard neutrino interactions, seesaw mechanism, stability criteria, leptogenesis
HSV kategori
Identifikatorer
URN: urn:nbn:se:kth:diva-4415ISBN: 978-91-7178-646-3 (tryckt)OAI: oai:DiVA.org:kth-4415DiVA, id: diva2:12206
Disputas
2007-06-11, Oskar Kleins auditorium (FR4), Huvudbyggnaden, AlbaNova, Roslagstullsbacken 21, Stockholm, 10:00
Opponent
Veileder
Merknad
QC 20100630Tilgjengelig fra: 2007-05-31 Laget: 2007-05-31 Sist oppdatert: 2010-06-30bibliografisk kontrollert
Delarbeid
1. Day-night effect in solar neutrino oscillations with three flavors
Åpne denne publikasjonen i ny fane eller vindu >>Day-night effect in solar neutrino oscillations with three flavors
2004 (engelsk)Inngår i: Physical Review D. Particles and fields, ISSN 0556-2821, E-ISSN 1089-4918, Vol. 69, nr 7, s. 073006-1-073006-9Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We investigate the effects of a nonzero leptonic mixing angle theta(13) on the solar neutrino day-night asymmetry. Using a constant matter density profile for the Earth and well-motivated approximations, we derive analytical expressions for the nu(e) survival probabilities for solar neutrinos arriving directly at the detector and for solar neutrinos which have passed through the Earth. Furthermore, we numerically study the effects of a nonzero theta(13) on the day-night asymmetry at detectors and find that they are small. Finally, we show that if the uncertainties in the parameters theta(12) and Deltam(2) as well as the uncertainty in the day-night asymmetry itself were much smaller than they are today, this effect could, in principle, be used to determine theta(13).

sted, utgiver, år, opplag, sider
The American Physical Society, 2004
Emneord
SUPERBEAMS, article, elementary particle, flavor, mathematical analysis, neutrino, night, oscillation, solar energy
HSV kategori
Identifikatorer
urn:nbn:se:kth:diva-7244 (URN)10.1103/PhysRevD.69.073006 (DOI)000221253900014 ()2-s2.0-42749106442 (Scopus ID)
Forskningsfinansiär
Swedish Research Council, 621-2001-1611Swedish Research Council, 621-2002-3577Swedish Research Council, 621-2001-1978
Merknad
QC 20100630Tilgjengelig fra: 2011-06-21 Laget: 2007-05-31 Sist oppdatert: 2017-12-14bibliografisk kontrollert
2. Exact series solution to the two flavor neutrino oscillation problem in matter
Åpne denne publikasjonen i ny fane eller vindu >>Exact series solution to the two flavor neutrino oscillation problem in matter
2004 (engelsk)Inngår i: Journal of Mathematical Physics, ISSN 0022-2488, E-ISSN 1089-7658, Vol. 45, nr 11, s. 4053-4063Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

In this paper, we present a real nonlinear differential equation for the two flavor neutrino oscillation problem in matter with an arbitrary density profile. We also present an exact series solution to this nonlinear differential equation. In addition, we investigate numerically the convergence of this solution for different matter density profiles such as constant and linear profiles as well as the Preliminary Reference Earth Model describing the Earth's matter density profile. Finally, we discuss other methods used for solving the neutrino flavor evolution problem.

sted, utgiver, år, opplag, sider
American Institute of Physics, 2004
Emneord
neutrino oscillations, flavour model, nonlinear differential equations, Earth, convergence of numerical methods
HSV kategori
Identifikatorer
urn:nbn:se:kth:diva-7245 (URN)10.1063/1.1793330 (DOI)000224945900005 ()2-s2.0-22544485995 (Scopus ID)
Forskningsfinansiär
Swedish Research Council, 621-2001-1611Swedish Research Council, 621-2002-3577
Merknad
QC 20100630 QC 20110915Tilgjengelig fra: 2011-06-17 Laget: 2007-05-31 Sist oppdatert: 2017-12-14bibliografisk kontrollert
3. Effective neutrino mixing and oscillations in dense matter
Åpne denne publikasjonen i ny fane eller vindu >>Effective neutrino mixing and oscillations in dense matter
2005 (engelsk)Inngår i: Physics Letters B, ISSN 0370-2693, E-ISSN 1873-2445, Vol. 609, nr 3-4, s. 330-338Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We investigate the effective case of two-flavor neutrino oscillations in infinitely dense matter by using a perturbative approach. We begin by briefly summarizing the conditions for the three-flavor neutrino oscillation probabilities to take on the same form as the corresponding two-flavor probabilities. Then, we proceed with the infinitely dense matter calculations. Finally, we study the validity of the approximation of infinitely dense matter when the effective matter potential is large, but not infinite, this is done by using both analytic and numeric methods.

sted, utgiver, år, opplag, sider
Elsevier B.V., 2005
Emneord
analytic method; article; calculation; mathematical computing; mathematical model; neutrino; oscillation; probability; validation process
HSV kategori
Identifikatorer
urn:nbn:se:kth:diva-7246 (URN)10.1016/j.physletb.2005.01.063 (DOI)000227534200022 ()2-s2.0-14144254930 (Scopus ID)
Forskningsfinansiär
Swedish Research Council, 621-2001-1611Swedish Research Council, 621-2002-3577
Merknad

QC 20100630

Tilgjengelig fra: 2011-06-17 Laget: 2007-05-31 Sist oppdatert: 2017-12-14bibliografisk kontrollert
4. Damping signatures in future neutrino oscillation experiments
Åpne denne publikasjonen i ny fane eller vindu >>Damping signatures in future neutrino oscillation experiments
2005 (engelsk)Inngår i: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, Vol. 2005, nr 06, s. 049-Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We discuss the phenomenology of damping signatures in the neutrino oscillation probabilities, where either the oscillating terms or the probabilities can be damped. This approach is a possibility for tests of damping effects in future neutrino oscillation experiments, where we mainly focus on reactor and long-baseline experiments. We extensively motivate different damping signatures due to small corrections by neutrino decoherence, neutrino decay, oscillations into sterile neutrinos, or other mechanisms, and classify these signatures according to their energy ( spectral) dependencies. We demonstrate, at the example of short baseline reactor experiments, that damping can severely alter the interpretation of results, e. g., it could fake a value of sin(2)(2 theta(13)) smaller than the one provided by Nature. In addition, we demonstrate how a neutrino factory could constrain different damping models with emphasis on how these different models could be distinguished, i.e., how easily the actual type of effect could be identified. We find that the damping models cluster in different categories, which can be much better distinguished from each other than models within the same cluster.

sted, utgiver, år, opplag, sider
IOP Publishing, 2005
Emneord
Solar and atmospheric neutrinos, neutrino physics
HSV kategori
Identifikatorer
urn:nbn:se:kth:diva-7247 (URN)10.1088/1126-6708/2005/06/049 (DOI)000230409600036 ()2-s2.0-22144490532 (Scopus ID)
Forskningsfinansiär
Swedish Research Council, 621-2001-1611Swedish Research Council, 621-2002-3577
Merknad

QC 20100630

Tilgjengelig fra: 2011-06-17 Laget: 2007-05-31 Sist oppdatert: 2017-12-14bibliografisk kontrollert
5. Non-standard Hamiltonian effects on neutrino oscillations
Åpne denne publikasjonen i ny fane eller vindu >>Non-standard Hamiltonian effects on neutrino oscillations
2007 (engelsk)Inngår i: The European Physical Journal C, ISSN 1434-6044, Vol. 49, nr 4, s. 1023-1039Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We investigate non-standard Hamiltonian effects on neutrino oscillations, which are effective additional contributions to the vacuum or matter Hamiltonian. Since these effects can enter in either the flavor or mass basis, we develop an understanding of the difference between these bases representing the underlying theoretical model. In particular, the simplest of these effects are classified as "pure" flavor or mass effects, where the appearance of such a "pure" effect can be quite plausible as a leading non-standard contribution from theoretical models. Compared to earlier studies investigating particular effects, we aim for a top-down classification of a possible "new physics" signature at future long-baseline neutrino oscillation precision experiments. We develop a general framework for such effects with two neutrino flavors and discuss the extension to three neutrino flavors, and we demonstrate the challenges for a neutrino factory to distinguish the theoretical origin of these effects with a numerical example as well. We find how the precision measurements of neutrino oscillation parameters can be altered by non-standard effects alone (not including non-standard interactions in the creation and detection processes) and that the non-standard effects on Hamiltonian level can be distinguished from other non-standard effects (such as neutrino decoherence and decay) if we consider the specific imprint of the effects on the energy spectra of several different oscillation channels at a neutrino factory.

sted, utgiver, år, opplag, sider
Springer-Verlag / Società Italiana di Fisica, 2007
Emneord
Mass Varying Neutrinos, Matter, Spectroscopy, Golden
HSV kategori
Identifikatorer
urn:nbn:se:kth:diva-7248 (URN)10.1140/epjc/s10052-006-0177-3 (DOI)000244692500011 ()2-s2.0-33847628889 (Scopus ID)
Forskningsfinansiär
Swedish Research Council, 621-2001-1611Swedish Research Council, 621-2002-3577Swedish Research Council, 621- 2005-3588
Merknad
QC 20100630Tilgjengelig fra: 2011-06-17 Laget: 2007-05-31 Sist oppdatert: 2011-06-17bibliografisk kontrollert
6. Effects of non-standard interactions in the MINOS experiment
Åpne denne publikasjonen i ny fane eller vindu >>Effects of non-standard interactions in the MINOS experiment
2008 (engelsk)Inngår i: Physics Letters B, ISSN 0370-2693, E-ISSN 1873-2445, Vol. 660, nr 5, s. 522-528Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We investigate the effects of non-standard interactions on the determination of the neutrino oscillation parameters Delta m(31)(2), theta(23), and theta(13) in the MINOS experiment. We show that adding non-standard interactions to the analysis lead to an extension of the allowed parameter space to larger values of Delta m(31)(2) and smaller theta(23), and basically removes all predictability for theta(13). In addition, we discuss the sensitivities to the non-standard interaction parameters of the MINOS experiment alone. In particular, we examine the degeneracy between theta(13) and the non-standard interaction parameter epsilon(e tau). We find that this degeneracy is responsible for the removal of the theta(13) predictability and that the possible bound on vertical bar epsilon(e tau)vertical bar is competitive with direct bounds only if a more stringent external bound on theta(13) is applied.

sted, utgiver, år, opplag, sider
Elsevier B.V., 2008
Emneord
Neutrino oscillation experiments, line-experiment-simulator, matter, spectroscopy, physics
HSV kategori
Identifikatorer
urn:nbn:se:kth:diva-7249 (URN)10.1016/j.physletb.2008.01.049 (DOI)000254034000014 ()2-s2.0-39149110271 (Scopus ID)
Forskningsfinansiär
Swedish Research Council, 621-2005-3588
Merknad
QC 20100630Tilgjengelig fra: 2011-06-17 Laget: 2007-05-31 Sist oppdatert: 2017-12-14bibliografisk kontrollert
7. Stability and leptogenesis in the left-right symmetric seesaw mechanism
Åpne denne publikasjonen i ny fane eller vindu >>Stability and leptogenesis in the left-right symmetric seesaw mechanism
Vise andre…
2007 (engelsk)Inngår i: Journal of High Energy Physics (JHEP), ISSN 1126-6708, E-ISSN 1029-8479, Vol. 4, s. 022-1-022-25Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We analyze the left-right symmetric type I+II seesaw mechanism, where an eight-fold degeneracy among the mass matrices of heavy right-handed neutrinos M-R is known to exist. Using the stability property of the solutions and their ability to lead to successful baryogenesis via leptogenesis as additional criteria, we discriminate among these eight solutions and partially lift their eight-fold degeneracy. In particular, we find that viable leptogenesis is generically possible for four out of the eight solutions.

Emneord
baryogenesis, neutrino physics
HSV kategori
Identifikatorer
urn:nbn:se:kth:diva-7250 (URN)10.1088/1126-6708/2007/04/022 (DOI)000246396400022 ()
Merknad
QC 20100630 QC 20110518Tilgjengelig fra: 2011-05-18 Laget: 2007-05-31 Sist oppdatert: 2017-12-14bibliografisk kontrollert

Open Access i DiVA

fulltekst(814 kB)2059 nedlastinger
Filinformasjon
Fil FULLTEXT01.pdfFilstørrelse 814 kBChecksum SHA-1
964af04dcbda71f967080df686cb613329365408972d8598984c65acb1d4431c9a33ba1d
Type fulltextMimetype application/pdf

Personposter BETA

Blennow, Mattias

Søk i DiVA

Av forfatter/redaktør
Blennow, Mattias
Av organisasjonen

Søk utenfor DiVA

GoogleGoogle Scholar
Totalt: 2059 nedlastinger
Antall nedlastinger er summen av alle nedlastinger av alle fulltekster. Det kan for eksempel være tidligere versjoner som er ikke lenger tilgjengelige

isbn
urn-nbn

Altmetric

isbn
urn-nbn
Totalt: 1390 treff
RefereraExporteraLink to record
Permanent link

Direct link
Referera
Referensformat
  • apa
  • harvard1
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Annet format
Fler format
Språk
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Annet språk
Fler språk
Utmatningsformat
  • html
  • text
  • asciidoc
  • rtf